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Full text of "The Theory of Sound"

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First Edition prinUd 1877. 
Second Edition revised and enlarged 1894. 


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IN the work, of which the present volume is an instalment, 
my endeavour has been to lay before the reader a connected 
exposition of the theory of sound, which should include the 
more important of the advances made in modem times by Mathe- 
maticians and Physicists. The importance of the object which 
I have had in view will not, I think, be disputed by those com- 
petent to judge. At the present time many of the most valuable 
contributions to science are to be found only in scattered 
periodicals and transactions of societies, published in various 
parts of the world and in several languages, and are often 
practically inaccessible to those who do not happen to live in 
the neighbourhood of large public libraries. In such a state of 
things the mechanical impediments to study entail an amount 
of unremunerative labour and consequent hindrance to the 
advancement of science which it would be difficult to over- 

Since the well-known Article on Sound in the EncyclopoBdia 
Metropolitana, by Sir John Herschel (1845), no complete work 
has been published in which the subject is treated mathemati- 
cally. By the premature death of Prof. Donkin the scientific 
world was deprived of one whose mathematical attainments in 
combination with a practical knowledge of music qualified him 
in a special manner to write on Sound. The first part of his 
Acoustics (1870), though little more than a firagment, is sufficient 
to shew that my labours would have been unnecessary had Prof. 
Donkin lived to complete his work. 

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In the choice of topics to be dealt with in a work on Sound, 
I have for the most part followed the example of my predecessors. 
To a great extent the theory of Sound, as commonly understood, 
covers the same ground as the theory of Vibrations in general ; 
but, unless some limitation were admitted, the consideration of 
such subjects as the Tides, not to speak of Optics, would have 
to be included. As a general rule we shall confine ourselves to 
those classes of vibrations for which our ears afford a ready 
made and wonderfully sensitive instrument of investigation. 
Without ears we should hardly care much more about vibrations 
than without eyes we should care about light. 

The present volume includes chapters on the vibrations of 
systems in general, in which, I hope, will be recognised some 
novelty of treatment and results, followed by a more detailed 
consideration of special systems, such as stretched strings, bars, 
membranes, and plates. The second volume, of which a con- 
siderable portion is already written, will commence with aerial 

My best thanks are due to Mr H. M. Taylor of Trinity College, 
Cambridge, who has been good enough to read the proofs. By 
his kind assistance several errors and obscurities have been 
eliminated, and the volume generally has been rendered less im- 
perfect than it would otherwise have been. 

Any corrections, or suggestions for improvements, with which 
my readers may favour me will be highly appreciated. 

TsBLiNa Place, Withax, 
April, 1877. 

IN this second edition all corrections of importfince are noted, 
and new matter appears either as fresh sections, e.g. § 32 a, 
or enclosed in square brackets [ ]. Two new chapters X a, X B 
are interpolated, devoted to Curved Plates or Sheila, and to 
Electrical Vibrations. Much of the additional matter relates to 
the more difficult parts of the subject and will be passed over 
by the reader on a first perusal. 

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In the mathematical investigations I have usually employed 
such methods as present themselves naturally to a physicist. 
The pure mathematician will complain, and (it must be confessed) 
sometimes with justice, of deficient rigour. But to this question 
there are two sides. For, however important it may be to 
maintain a uniformly high standard in pure mathematics, the 
physicist may occasionally do well to rest content with argu- 
ments which are fairly satisfectory and conclusive from his point 
of view. To his mind, exercised in a different order of ideas, 
the more severe procedure of the pure mathematician may appear 
not more but less demonstmtive. And further, in many cases 
of difficulty to insist upon the highest standard would mean 
the exclusion of the subject altogether in view of the space 
that would be required. 

In the first edition much stress was laid upon the establish- 
ment of general theorems by means of Lagi-ange's method, and 
I am more than ever impressed with the advantages of this 
procedure. It not unfrequently happens that a theorem can be 
thus demonstrated in all its generality with less mathematical 
apparatus than is required for dealing with particular cases by 
special methods. 

During the revision of the proof-sheets I have again had the 
very great advantage of the cooperation of Mr H. M. Taylor, 
until he was unfortunately compelled to desist. To him and 
to several other friends my thanks are due for valuable sug- 

July, 1894. 

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§§ 1 — 27 INTRODUCTION .... 1 

Sound due to Vibrations. Finite velocity of Propagation. Velocity inde- 
pendent of Pitch. Begnault's experiments. Sound propagated in water. 
Wheatstone^s experiment. Enfeeblement of Sound by distance. Notes 
and Noises. Musical notes due to periodic vibratioffitr Siren of Gagniard 
de la Tour. Pitch dependent upon Period. Relationship between 
musical notes. The same ratio of periods corresponds to the same 
interval in all parts of the scale. Harmonic scales. Diatonic scales. 
Absolute Pitch. Necessity of Temperament. Equal Temperament. 
Table of Frequencies. Analysis of Notes. Notes and Tones. Quality 
dependent upon harmonic overtones. Resolution of Notes by ear un- 
certain. Simple tones correspond to simple pendulous vibrations. 


§§28 — 42 a HARMONIC MOTIONS . . . .19 

Composition of harmonic motions of like period. Harmonic Curve. Com- 
position of two vibrations of nearly equal period. Beats. Fourier's 
Theorem. [Beats of approximate consonances.] Vibrations in perpen- 
dicular directions/ Lissajous' Cylinder. Lissajous* Figures. Black- 
burn's pendulum. Ealeidophone. Optical methods of composition 
and analysis. The vibration microscope. Intermittent Illumination. 
[Resultant of a large number of vibrations whose phases are accidentally 

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Independence of amplitude and period. Frictional force proportional to 
velocity. Forced vibrations. Principle of Superposition. Beats due 
to superposition of forced and free . vibrations. Various degrees of 
damping. String with Load. Method of Dimensions. Ideal Tuning- 
fork. Forks give nearly pure tones. Forks as standards of pitch. 
[Dependence upon temperature. Slow ver$us quick heats.] Scheibler's 
methods of tuning. Scheibler's Tonometers. Compound Pendulum. 
Forks driven by electro-magnetism. [Phonic wheel.] Fork Interrupter. 
Resonance. [Intermittent vibrations.] General solution for one degree 
of freedom. [Instability.] Terms of the second order give rise to 
derived tones. [Maintenance. Methods of determining absolute pitch.] 



Generalized co-ordinates. Expression for potential energy. Statical theo- 
rems. Initial motions. Expression for kinetic energy. Reciprocal 
theorem. Thomson's [Kelvin's] theorem. Lagrange's equations. The 
dissipation function. Coexistence of small motions. Free vibrations 
without friction. Normal co-ordinates. The free periods fulfil a 
stationary condition. An accession of inertia increases the free periods. 
A relaxation of spring increases the free periods. The greatest free 
period is an absolute maximum. Hypothetical types of vibration. 
Example from string. Approximately simple systems. String of 
. variable density. Normal functions. Conjugate property. [Introduc- 
tion of one constraint. Several constraints.] Determination of con- 
stants to suit arbitrary initial conditions. Stokes' theorem. 



Oases in which the three functions T, F, V are simultaneously reducible to 
sums of squares. Generalization of Young's theorem on the nodal 
points of strings. Equilibrium theory. Systems started from rest as 
defiected by a force applied at one point. Systems started from the 
equilibrium configuration by an impulse applied at one point. Systems 
started from rest as deflected by a force uniformly distributed. Influ- 
ence of rmall frictional forces on the vibrations of a system. Solution 
of the general equations for free vibrations. [Routh's theorems. In- 
stability.] Impressed Forces. Principle of the persistence of periods. 
Inexorable motions. Reciprocal Theorem. Application to free vibrations. 
Statement of reciprocal theorem for harmonic forces. Applications. 
Extension to oases in which the constitution of the system is a function 
of the period. [Reaction at driving point.] Equations for two degrees 
of freedom. Roots of determinantal equation. Intermittent vibrations. 
March of periods as inertia is gradually increased. Reaction of a 
dependent system. 

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Law of extension of a string. Transverse vibrations. Solution of the pro- 
blem for a string whose mass is concentrated in equidistant points. 
Derivation of solution for continuous string. Partial differential equa- 
tion. Expressions for V and T. Most general form of simple harmonic 
motion. Strings with fixed extremities. General motion of a string 
periodic. Mersenne's Laws. Sonometer. Normal modes of vibration. 
Determination of constants to suit arbitrary initial circumstances. Case 
of plucked string. Expressions for T and F in terms of normal co-ordi- 
nates. Normal equations of motion. String excited by plucking. 
Young's theorem. String excited by an impulse. Problem of piano- 
forte string. Friction proportional to velocity. Comparison with equi- 
librium theory. Periodic force applied at one point. Modifications due 
to yielding of the extremities. Proof of Fourier's theorem. Effects 
of a finite load. Correction for rigidity. Problem of violin string. 
Strings stretched on curved surfaces. Solution for the case of the 
sphere. Correction for irregularities' of density. [Arbitrary displace- 
ment of every period.] Theorems of Sturm and Liouville for a string 
of variable density. [Density proportional to a;-'. Nodes of forced vibra- 
tions.] Propagation of waves along an unlimited string. Positive and 
negative waves. Stationary Vibrations. Reflection at a fixed point 
Deduction of solution for finite string. Graphical method. Progressive 
wave with friction. [Reflection at a junction of two strings. Gradual 
transition. Effect of imperfect flexibility.] 



OF BARS 242 

Classification of the vibrations of Bars. Differential equation for longi- 
tudinal vibrations. Numerical values of the constants for steel. Solu- 
tion for a bar free at both ends. Deduction of solution for a bar with 
one end free, and one fixed. Both ends fixed. Influence of small load. 
Solution of problem for bar with large load attached. [Reflection at a 
junction.] Correction for lateral motion. Savart's '*son rauque." 
Differential equation for torsional vibrations. Comparison of velocities 
of longitudinal and torsional waves. 


§§160— 192 a LATERAL VIBRATIONS OF BARS . . . 255 

Potential energy of bending. Expression for kinetic energy. Derivation 
of differential equation. Terminal conditions. General solution for 
a harmonic vibration. Conjugate property of the normal functions. 
Values of integrated squares. Expression of F in terms of normal 

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oo-ordinates. Normal equations of motion. Determination of constants 
to suit initial conditions. Case of rod started by a blow. Bod started 
from rest as deflected by a lateral force. In certain cases the series of 
normal functions ceases to converge. Form of the normal functions for 
a free-free bar. Laws of dependence of frequency on length and thick- 
ness. [Numerical formuls for tuning-forks.] Case when both ends are 
clamped. Normal functions for a clamped-free bar. Calculation of 
periods. Comparisons of pitch. Discussion of the gravest mode of 
vibration of a free-free bar. Three nodes. Four nodes. Gravest mode 
for clamped-free bar. Position of nodes. Supported bar. Calculation 
of period for clamped-free bar from hypothetical type. Solution of 
problem for a bar with a loaded end. £ffect of additions to a bar. 
Influence of irregularities of density. Correction for rotatory inertia. 
Boots of functions derived linearly from normal functions. Formation 
of equation of motion when there is permanent tension. Special ter- 
minal conditions. Besultant of two trains of waves of nearly equal 
period. Fourier^s solution of problem for infinite bar. [Circular Bing.] 


§§193 — 213 a VIBRATIONS OF MEMBBANES . . 306 

Tension of a membrane. Equation of motion. Fixed rectangular bound- 
ary. Expression for V and T in terms of normal co-ordinates. Normal 
equations of vibration* Examples of impressed forces. Frequency for 
an elongated rectangle depends mainly on the shorter side. Cases in 
which different modes of vibration have the same period. Derived 
modes thence arising. Effect of slight irregularities. An irregularity 
may remove indeterminateness of normal modes. Solutions applicable 
to a triangle. Expression of the general differential equation by polar 
co-ordinates. Of the two functions, which occur in the solution, one is 
excluded by the condition at the pole. Expressions for Bessel's func- 
tions. Formulie relating thereto. Table of the flrst two functions. 
Fixed circular boundary. Conjugate property of the normal functions 
without restriction of boundary. Values of integrated squares. Ex- 
pressions for T and V in terms of normal functions. Normal equations 
of vibration for circular membrane. Special case of free vibrations. 
Vibrations due to a harmonic force uniformly distributed. [Force 
applied locally at the centre.] Pitches of the various simple tones. 
Table of the roots of Bessel's functions. Nodal Figures. Circular 
membrane with one radius fixed. Bessers functions of fractional order. 
Effect of small load. Vibrations of a membrane whose boundary is 
approximately circular. In many cases the pitch of a membrane may 
be calculated from the area alone. Of all membranes of equal area tbat 
of circular form has the gravest pitch. Pitch of a membrane whose 
boundary is an ellipse of small eccentricity. Method of obtaining limits 
in cases that cannot be dealt with rigorously. Comparison of fre- 
quencies in various cases of membranes of equal area. History of the 
problem. Bourget's experimental investigations. [Kettle-drums. Nodal 
curves of forced vibrations.] 

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§§ 214 — 235 a vibrations of plates . . 352 

Potential Energy of Bending. Transformation of 8V. Superficial differ- 
ential equation. Boundary conditions. Conjugate property of normal 
functions. Transformation to polar co-ordinates. Form of general 
solution continuous through pole. Equations determining the periods 
for a free circular plate. EiichhofF's calctdations. Comparison with 
observation. Badii of nodal circles. Oeneralization of solution. Ir- 
regularities give rise to beats. [Oscillation of nodes.] Case of clamped, 
or supported, edge. [Telephone plate.] Disturbance of Chladni's 
figures. [Movements of sand.] History of problem. Mathieu's criti- 
cisms. Rectangular plate with supported edge. Rectangular plate with 
free edge. Boundary conditions. One special case (/li=0) is amenable 
to mathematical treatment. Investigation of nodal figures. Wheat- 
stone's application of the method of superposition. Comparison of 
Wheatstone's figures with those really applicable to a plate in the case 
/A=0. Gravest mode of a square plate. Calculation of period on hypo- 
thetical type. Nodal figures inferred from considerations of symmetry. 
Hexagon. Comparison between circle and square. Law connecting 
pitch and thickness. In the case of a clamped edge any contraction of 
the boundary raises the pitch. No gravest form for a free plate of 
given area. In similar plates the period is as the linear dimension. 
Wheatstone's experiments on wooden plates. Eoanig's experiments. 
Vibrations of cylinder, or ring. Motion tangential as well as normal. 
Relation between tangential and normal motions. Expressions for 
kinetic and potential energies. Equations of vibration. Frequencies 
of tones. Comparison with Chladni. [Fenkner's observations.] Tan- 
gential friction excites tangential motion. Experimental verification. 
Beats due to irregularities. [Examples of glass bells. Church bells.] 

§ 235 b — 235 h curved plates or shells . . 395 

[Extensional Vibrations. Frequency independent of thickness. Inexten- 
sional or flexural vibrations. Frequency proportional to thickness. 
General conditions of inextension. Surface of second degree. Applica- 
tion to sphere. Principal extensions of cylindrical surface. Potential 
energy. Frequencies of extensional vibrations. Plane plate. Other 
particular cases of cylinder. Potential energy of bending. Sphere. 
Plane plate. Potential energy for cylindrical shell. Statical problems. 
Frequency of flexural vibrations of cylindrical shell. Extensional 
vibrations of spherical shell. Flexural vibrations of spherical shell. 
Normal modes. Potential energy. Kinetic energy. Frequencies in case 
of hemisphere. Saucer of 120°. References.] 

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§ 235 i — 235 y electrical vibrations . . . 433 

[Calculation of periods. Forced vibrations. Insertion of a leyden equivalent 
to a negative inductance. Initial currents in a secondary circuit. In- 
versely as the number of windings. Reaction of secondary circuit. 
Train of circuits. Initial currents alternately opposite in sign. Per- 
sistences. Resistance and inductance of two conductors in parallel. 
Extreme values of frequency. Contiguous wires. Several conductors in 
parallel. Induction balance. Theory for simple harmonic currents. Two 
conditions necessary for balance. Wheatstone's bridge. Generalized 
resistance. Current in bridge. Approximate balance. Hughes' ar- 
rangement. Interrupters. Inductometers. Symmetrical arrangement. 
Electromagnetic screening. Cylindrical conducting core. Time-con- 
stant of free currents. Induced electrical vibrations. Reaction upon 
primary circuit. Induced currents in a wire. Maxwell's formulas. 
Impedance. Kelvin's theory of cables. Heaviside's generalization. 
Attenuation and distortion of signals. Bell's telephone. Push and 
pull theory. Experiment upon bipolar telephone. Minimum current 
audible. Microphone.] 

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1. The sensation of sound is a thing aui generis, not com- 
parable with any of our other sensations. No one can express 
the relation between a sound and a colour or a smell. Directly 
or indirectly, all questions connected with this subject must 
come for decision to the ear, as the organ of hearing; and 
from it there can be no appeal. But we are not therefore to 
infer that all acoustical investigations are conducted with the 
unassisted ear. When once we have discovered the physical 
phenomena which constitute the foundation of sound, our ex- 
plorations are in great measure transferred to another field lying 
within the dominion of the principles of Mechanics. Important 
laws are in this way arrived at, to which the sensations of the ear 
cannot but conform. 

2. Very cursory observation often suffices to shew that 
sounding bodies are in a state of vibration, and that the phe- 
nomena of sound and vibration are closely connected. When a 
vibrating bell or string is touched by the finger, the sound ceases 
at the same moment that the vibration is damped. But, in order 
to affect the sense of hearing, it is not enough to have a vibrating 
instrument ; there must also be an uninterrupted communication 
between the instrument and the ear. A bell rung in vacuo, with 
proper precautions to prevent the communication of motion, 
remains inaudible. In the air of the atmosphere, however, 
sounds have a universal vehicle, capable of conveying . them 
without break from the most variously constituted sources to 
the recesses of the ear. 

3. The passage of sound is not instantaneous. When a gun 
is fired at a distance, a very perceptible interval separates the 

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report from the flash. This represents the time occupied by 
sound in travelling from the gun to the observer, the retardation 
of the flash due to the finite velocity of light being altogether 
negligible. The first accurate experiments were made by some 
members of the French Academy, in 1738. Cannons were fired, 
and the retardation of the reports at different distances observed. 
The principal precaution necessary is to reverse alternately the 
direction along which the sound travels, in order to eliminate the 
influence of the motion of the air in mass. Down the wind, for 
instance, sound travels relatively to the earth faster than its 
proper rate, for the velocity of the wind is added to that proper 
to the propagation of sound in still air. For still dry air at a 
temperature of O^C, the French observers found a velocity of 337 
metres per second. Observations of the same character were 
made by Arago and others in 1822 ; by the Dutch physicists Moll, 
van Beek and Kuytenbrouwer at Amsterdam; by Bravais and 
Martins between the top of the Faulhom and a station below; 
and by others. The general result has been to give a somewhat 
lower value for the velocity of sound — about 332 metres per 
second. The effect of alteration of temperature and pressure on 
the propagation of sound will be best considered in connection with 
the mechanical theory. 

4. It is a direct consequence of observation, that within wide 
limits, the velocity of sound is independent, or at least very nearly 
independent, of its intensity, and also of its pitch. Were this 
otherwise, a quick piece of music would be heard at a little 
distance hopelessly confused and discordant. But when the dis- 
turbances are very violent and abrupt, so that the alteratious of 
density concerned are comparable with the whole density of the 
air, the simplicity of this law may be departed from. 

6. An elaborate series of experiments on the propagation of 
sound in long tubes (water-pipes) has been made by Regnault\ 
He adopted an automatic arrangement similar in principle to that 
used for measuring the speed of projectiles. At the moment when 
a pistol is fired at one end of the tube a wire convejdng an electric 
current is ruptured by the shock. This causes the withdrawal of a 
tracing point which was previously marking a line on a revolving 
drum. At the further end of the pipe is a stretched membrane so 
arranged that when on the arrival of the sound it yields to the 
1 Mimmrti de VAcadimie de France, t. xzztil 

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impulse, the circuit, which was ruptured during the passage of the 
sound, is recompleted. At the same moment the tracing point 
falls back on the drum. The blank space left unmarked corre- 
sponds to the time occupied by the sound in making the journey, 
and, when the motion of the drum is known, gives the means of 
detennining it. The length of the journey between the first wire 
and the membrane is found by direct measurement. In these 
experiments the velocity of sound appeared to be not quite inde- 
pendent of the diameter of the pipe, which varied horn ©"'•lOS 
to 1"**100. The discrepancy is perhaps due to friction, whose 
influence would be greater in smaller pipes. 

6. Although, in practice, air is usually the vehicle of sound, 
other gases, liquids and solids are equally capable of conveying 
it. In most cases, however, the means of making a direct measure- 
ment of the velocity of sound are wanting, and we are not yet in 
a position to consider the indirect methods. But in the case of 
water the same difficulty does not occur. In the year 1826, 
Colladon and Sturm investigated the propagation* of sound in the 
Lake of Geneva. The striking of a bell at one station was 
simultaneous with a flash of gunpowder. The observer at a 
second station measured the interval between the flash and the 
arrival of the sound, applying his ear to a tube carried beneath 
the surface. At a temperature of 8®C., the velocity of sound in 
water was thus found to be 1435 metres per second. 

7. The conveyance of sound by solids may be illustrated by a 
pretty experiment due to Wheatstone. One end of a metallic wire 
is connected with the sound-board of a pianoforte, and the other 
taken through the partitions or floors into another part of the 
building, where naturally nothing would be audible. If a reso- 
nance-boaixl (such as a violin) be now placed in contact with the 
wire, a tune played on the piano is easily heard, and the sound 
seems to emanate from the resonance-board. [Mechanical tele- 
phones upon this principle have been introduced into practical 
use for the conveyance of speech.] 

8. In an open space the intensity of sound falls off with great 
rapidity as the distance from the source increases. The same 
amount of motion has to do duty over surfaces ever increasing as 
the squares of the distance. Anything that confines the sound 
will tend to diminish the falling off of intensity. Thus over the 
flat surface of still water, a sound carries further than over broken 

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ground; the corner between a smooth pavement and a vertical 
wall is still better ; but the most effective of all is a tube-like 
enclosure, which prevents spreading altogether. The use of 
speaking tubes to facilitate communication between the different 
parts of a building is well known. If it were not for certain effects 
(frictional and other) due to the sides of the tube, sound might 
be thus conveyed with little loss to very great distances. 

9. Before proceeding further we must consider a distinction, 
which is of great importance, though not free from diflBculty. 
Sounds may be classed as musical and unmusical; the former 
for convenience may be called notes and the latter noises. The 
extreme cases will raise no dispute; every one recognises the 
difference between the note of a pianoforte and the creaking of a 
shoe. But it is not so easy to draw the line of separation. In the 
first place few notes are free from all unmusical accompaniment. 
With organ pipes especially, the hissing of the wind as it escapes 
at the mouth may be heard beside the proper note of the pipe. 
And, secondly, many noises so far partake of a musical character 
as to have a definite pitch. This is more easily recognised in a 
sequence, giving, for example, the common chord, than by continued 
attention to an individual instance. The experiment may be made 
by drawing corks from bottles, previously tuned by pouring water 
into them, or by throwing down on a table sticks of wood of suitable 
dimensions. But, although noises are sonietimes not entirely 
unmusical, and notes are usually not quite free from noise, there is 
no difficulty in recognising which of the two is the simpler pheno- 
menon. There is a certain smoothness and continuity about the 
musical note. Moreover by sounding together a variety of notes — 
for example, by striking simultaneously a number of consecutive 
keys on a pianoforte — we obtain an approximation to a noise; 
while no combination of noises could ever blend into a musical 

10. We are thus led to give our attention, in the first instance, 
mainly to musical sounda These arrange themselves naturally 
in a certain order according to pitch — a quality which all can 
appreciate to some extent. Trained ears can recognise an enormous 
number of gradations — more than a thousand, probably, within 
the compass of the human voice. These gradations of pitch are 
not, like the degrees of a thermometric scale, without special 
mutual relations. Taking any given note as a starting point. 

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10.] PITCH. 5 

musicians can single out certain others, which hear a definite 
relation to the first, and are known as its octave, fifth, &c. The 
corresponding diflferences of pitch are called intervals, and are 
spoken of as always the same for the same relationship. Thus, 
wherever they may occur in the scale, a note and its octave are 
separated by the interval of the octave. It will be our object later 
to explain, so far as it can be done, the origin and nature of the 
consonant intervals, but we must now turn to consider the physical 
aspect of the question. 

Since sounds are produced by vibrations, it is natural to 
suppose that the simpler sounds, viz. musical notes, correspond to 
periodic vibrations, that is to say, vibrations which after a certain 
interval of time, called the period, repeat themselves with perfect 
regularity. And this, with a limitation presently to be noticed, 
is true. 

11. Many contrivances may be proposed to illustrate the 
generation of a musical note. One of the simplest is a revolving 
wheel whose milled edge is pressed against a card. Each 
projection as it strikes the card gives a slight tap, whose regular 
recurrence, as the wheel turns, produces a note of definite pitch, 
rising in the scale, cw the velocity of rotation increases. But the 
most appropriate instrument for the fundamental experiments on 
notes is undoubtedly the Siren, invented by Cagniard de la Tour. 
It consists essentially of a stiflf disc, capable of revolving about its 
centre, and pierced with one or more sets of holes, arranged at 
equal intervals round the circumference of circles concentric with 
the disc. A windpipe in connection with bellows is presented 
perpendicularly to the disc, its open end being opposite to one of 
the circles, which contains a set of holes. When the bellows are 
worked, the stream of air escapes freely, if a hole is opposite to the 
end of the pipe; but otherwise it is obstructed. As the disc turns, 
a succession of puffs of air escape through it, until, when the 
velocity is suflScient, they blend into a note, whose pitch rises 
continually with the rapidity of the puffs. We shall have occasion 
later to describe more elaborate forms of the Siren, but for our 
immediate purpose the present simple arrangement will su£5ce. 

12. One of the most important facts in the whole science is 
exemplified by the Siren — namely, that the pitch of a note depends 
upon the period of its vibration. The size and shape of the holes, 
the force of the wind, and other elements of the problem may be 

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varied ; but if the number of puffs in a given time, such as one 
second, remains unchanged, so also does the pitch. We may even 
dispense with wind altogether, and produce a note by allowing 
the comer of a card to tap against the edges of the holes, as they 
revolve ; the pitch will still be the same. Observation of other 
sources of sound, such as vibrating solids, leads to the same con- 
clusion, though the difficulties are often such as to render 
necessary rather refined experimental methods. 

But in saying that pitch depends upon period, there 
lurks an ambiguity, which deserves attentive consideration^ 
as it will lead us to a point of great importance. If a 
variable quantity be periodic in any time t, it is also periodic 
in the times 2t, 3t, &c. Conversely, a recurrence within a given 
period T, does not exclude a more rapid recurrence within 
periods which are the aliquot parts of t. It would appear 
accordingly that a vibration really recurring in the time ^ (for 
example) may be regarded as having the period t, and therefore 
by the law just laid down as producing a note of the pitch defined 
by T. The force of this consideration cannot be entirely evaded by 
defining as the period the least time required to bring about a 
repetition. In the first place, the necessity of such a restriction 
is in itself almost sufficient to shew that we have not got to the 
root of the matter ; for although a right to the period t may be 
denied to a vibration repeating itself rigorously within a time ^r, 
yet it must be allowed to a vibration that may differ indefinitely 
little therefrom. In the Siren experiment, suppose that in one 
of the circles of holes containing an even number, every alternate 
hole is displaced along the arc of the circle by the same amount. 
The displacement may be made so small that no change can be 
detected in the resulting note; but the periodic time on which 
the pitch depends has been doubled. And secondly it is evident 
from the nature of periodicity, that the superposition on a vibra- 
tion of period T, of others having periods Jt, Jt...&c., does not 
disturb the period t, while yet it cannot be supposed that the 
addition of the new elements has left the quality of the sound un- 
changed. Moreover, since the pitch is not affected by their 
presence, how do we know that elements of the shorter periods 
were not there from the beginning? 

13. These considerations lead us to expect remarkable rela- 
tions between the notes whose periods are as the reciprocals of the 

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natural numbers. Nothing can be easier than to investigate the 
question by means of the Siren. Imagine two circles of holes, the 
inner containing any convenient number, and the outer twice as 
many. Then at whatever speed the disc may turn, the period of 
the vibration engendered by blowing the first set will necessarily 
be the double of that belonging to the second. On making the 
experiment the two notes are found to stand to each other in 
the relation of octaves ; and we conclude that in passing from any 
note to its octave, the frequency of vibration is doubled. A similar 
method of experimenting shews, that to the ratio of periods 3 : 1 
corresponds the interval known to musicians as the twelfth, made 
up of an octave and a fifth; to the ratio of 4:1, the double 
octave ; and to the ratio 5:1, the interval made up of two octaves 
and a major third. In order to obtain the intervals of the fiffch 
and third themselves, the ratios must be made 3 : 2 and 5 : 4 

14. From these expeiiments it appears that if two notes 
stand to one another in a fixed relation, then, no matter at what 
part of the scale they may be situated, their periods are in a 
certain constant ratio characteristic of the relation. The same 
may be said of their frequencies^, or the number of vibrations 
which they execute in a given time. The ratio 2 : 1 is thus 
characteristic of the octave interval. If we wish to .combine 
two intervals, — for instance, starting from a given note, to take 
a step of an octave and then another of a fifth in the same 
direction, the coiTesponding ratios must be compounded : 

2 3_3 

The twelfth part of an octave is represented by the ratio v^2 : 1, 
for this is the step which repeated twelve times leads to an 
octave above the starting point. If we wish to have a measure 
of intervals in the proper sense, we must take not the character- 
istic ratio itself, but the logarithm of that ratio. Then, and then 
only, will the measure of a compound interval be the sum of the 
measures of the components. 

1 A single word to denote the number of vibrations executed in the unit of time 
is indispensable : I know no better than * frequency,* which was used in this sense 
by Young. The same word is employed by Prof. Everett in his exceUent edition 
of Desohaners Natural Philosophy, 

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16. From the intervals of the octave, fifth, and third con- 
sidered above, others known to musicians may be derived. The 
difference of an octave and a fifth is called a fourth^ and has the 

3 4 
ratio 2-r^«K' This process of subtracting an interval from 

the octave is called inverting it. By inverting the major third 
we obtain the minor sixth. Again, by subtraction of a major 
third from a fifth we obtain the minor third ; and from this by 
inversion the major sixth. The following table exhibits side by 
side the names of the intervals and the corresponding ratios of 
frequencies : 

Octave 2: 1 

Fifth 3:2 

Fourth 4:3 

Major Third 5:4. 

Minor Sixth 8:5 

Minor Third 6 :5 

Major Sixth 5:3 

These are all the consonant intervals comprised within the 
limits of the octave. It will be remarked that the corresponding 
ratios are all expressed by means of snudl whole numbers, and 
that this is more particularly the case for the more consonant 

The notes whose frequencies are multiples of that of a given 
one, are called its harmonics, and the whole series constitutes 
a harmonic scale. As is well known to violinists, they may all 
be obtained from the same string by touching it lightly with the 
finger at certain points, while the bow is drawn. 

The establishment of the connection between musical intervals 
and definite ratios of frequency — a fundamental point in Acoustics 
— is due to Mersenne (1636). It was indeed known to the 
Greeks in what ratios the lengths of strings must be changed 
in order to obtain the octave and fifth; but Mersenne demon- 
strated the law connecting the length of a string with the period 
of its vibration, and made the first determination of the actual 
rate of vibration of a known musical note. 

16. On any note taken as a key-note, or tonic, a diatonic 
scale may be founded, whose derivation we now proceed to ex- 
plain. If the key-note, whatever may be its absolute pitch, be 
called Do, the fifth above or dominant is Sol, and the fifth below 

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16.] NOTATION. 9 

or subdominant is Fa. The common chord on any note is pro- 
duced by combining it with its major third, and fifth, giving the 

ratios of frequency 1 • 7 • « or 4:5:6. Now if we take the 

common chord on the tonic, on the dominant, and on the sub- 
dominant, and transpose them when necessary into the octave 
Ijring immediately above the tonic, we obtain notes whose fre- 
quencies arranged in order of magnitude are : 

Do Re Mi Fa Sol La Si Do 

, 9 -5 4 3 5 15 

8' 4' 3' 2' 3' 8 ' 

Here the common chord on Do is Do— Mi — Sol, with the 

5 3 

ratios 1 : -r : - ; the chord on Sol is Sol — Si — Re, with the ratios 

2:-g-:2xg = l ^t^k; and the chord on Fa is Fa — La — Do, 

still with the same ratios. The scale is completed by repeating 
these notes above and below at intervals of octaves. 

If we take as our Do, or key-note, the lower c of a tenor voice, 
the diatonic scale will be 

c d e f g a b c'. 

Usage diflfers slightly as to the mode of distinguishing the 
different octaves ; in what follows I adopt the notation of Helm- 
holtz. The octave below the one just referred to is written with 
capital letters — C, D, &c. ; the next below that with a suflSx — 
C,, D„ &C. ; and the one beyond that with a double suffix — C,,, &c. 
On the other side accents denote elevation by an octave — c', c", 
&c. The notes of the four strings of a violin are written in this 
notation, g — d' — a'— e". The middle c of the pianoforte is c'. 
[In French notation c' is denoted by ut,.] 

17. With respect to an absolute standard of pitch there has 
been no uniform practice. At the Stuttgard conference in 1834, 
c' = 264 complete vibrations per second was recommended. This 
corresponds to a' = 440. The French pitch makes a' = 436. In 
Handel's time the pitch was much lower. If c' were taken at 256 
or 2*, all the c*s would have frequencies represented by powers 
of 2. This pitch is usually adopted by physicists and acoustical 
instrument makers, and has the advantage of simplicity. 

The determination ab initio of the frequency of a given note is 
an operation requiring some care. The simplest method in prin- 

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ciple is by means of the Siren, which is driven at such a rate as to 
give a note in unison with the given one. The number of turns 
effected by the disc in one second is given by a counting apparatus, 
which can be thrown in and out of gear at the beginning and end 
of a measured interval of time. This multiplied by the number of 
effective holes gives the required frequency. The consideration of 
other methods admitting of greater accuracy must be deferred. 

18. So long as we keep to the diatonic scale of c, the notes 
above written are all that are required in a musical composition. 
But it is frequently desired to change the key-note. Under these 
cifcumstances a singer with a good natural ear, accustomed to 
perform without accompaniment, takes an entirely fresh departure, 
constructing a new diatonic scale on the new key-note. In this 
way, after a few changes of key, the original scale will be quite 
departed from, and an immense variety of notes be used. On an 
instrument with fixed notes like the piano and organ such a 
multiplication is iraprswsticable, and some compromise is necessary 
in order to allow the same note to perform different functions. 
This is not the place to discuss the question at any length; we 
will therefore take as an illustration the simplest, as well as the 
commonest case — modulation into the key of the dominant. 

By definition, the diatonic scale of c consists of the common 
chords founded on c, g and f. In like manner the scale of g con- 
sists of the chords founded on g, d and c. The chords of c and g 
are then common to the two scales ; but the third and fifth of d 
introduce new notes. The third of d written f jt has a frequency 

9 5 45 

^ X J = ^ , and is far removed from any note in the scale of c. 

9 3 27 

But the fifth of d, with a frequency z^a^T^> differs but little 

from a, whose frequency is ^ . In ordinary keyed instruments the 

interval between the two; represented by ^ , and called a comma, 

is neglected, and the two notes by a suitable compromise or ' 
temperament are identified. 

19. Various systems of temperament have been used; the 
simplest and that now most generally used, or at least aimed at, 
is the equal temperament. On referring to the table of frequencies 
for the diatonic scale, it will be seen that the intervals from Do to 
Re, from Re to Mi, from Fa to Sol, from Sol to La, and from La 

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9 10 
to Si, are nearly the same, being represented by - or -q- ; while the 



intervals firom Mi to Fa and from Si to Do, represented by j^ , are 

about half as much. The equal temperament treats these ap- 
proximate relations as exact, dividing the octave into twelve equal 
parts called mean semitones. From these twelve notes the diatonic 
scale belonging to any key may be selected according to the 
following rule. Taking the key-note as the first, fill up the series 
with the third, fifth, sixth, eighth, tenth, twelfth and thirteenth 
notes, counting upwards. In this way all diflSculties of modulation 
are avoided, as the twelve notes serve as well for one key as for 
another. But this advantage is obtained at a sacrifice of true 
intonation. The equal temperament third, being the third part of 
an octave, is represented by the ratio v^ : 1, or approximately 
1-2599, while the true third is 1'25. The tempered third is thus 
higher than the true by the interval 126 : 125. The ratio of the 
tempered fifth may be obtained from the consideration that seven 
semitones make a fifth, while twelve go to an octave. The ratio is 


therefore 2^"^ : 1, which = 1-4983. The tempered fifth is thus too 
low in the ratio 1*4983 : 1*5, or approximately 881 : 882. This 
error is insignificant ; and even the error of the third is not of 
much consequence in quick music on instruments like the piano- 
forte. But when the notes are held, as in the harmonium and 
organ, the consonance of chords is materially impaired. 

20. The following Table, giving the twelve notes of the chro- 
matic scale according to the system of equal temperament, will be 
convenient for reference'. The standard employed is a' = 440; in 

























































































3322-5 1 









3520-0 ; 









3729-2 1 









3951-0 ' 

^ Zamminer, Die Musik und die mtuikaliichen Inttrumente, Giessen, 1855. 

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order to adapt the Table to any other absolute pitch, it is only 
necessary to multiply throughout by the proper constant. 

The ratios of the intervals of the equal temperament scale are 
given below (Zamminer) : — 

Note. Freqaency. | Note. Freqaency. 

c =1-00000 

Cjt 2^=1-05946 

d 2^ = M2246 

d$ 2^ = 1-18921 

e 2^^=1-25992 


fj{ 2^ = 1-41421 

g 2^^=1-49831 

gj 2^=1-58740 

a 2^^7=1-68179 

ajt 2^ = 1-78180 

f 2^7=1-33484 I b 2^7=188775 

c' = 2-000 

21. Returning now for a moment to the physical aspect of the 
question, we will assume, what we shall afterwards prove to be 
true within wide limits, — that, when two or more sources of sound 
agitate the air simultaneously, the resulting disturbance at any 
point in the external air, or in the ear-passage, is the simple sum 
(in the extended geometrical sense) of what would be caused by 
each source acting separately. Let us consider the disturbance 
due to a simultaneous sounding of a note and any or all of its 
harmonics. By definition, the complex whole forms a note having 
the same period (and therefore pitch) as its graveat element. We 
have at present no criterion by which the two can be distinguished, 
or the presence of the higher harmonics recognised. And yet— in 
the case, at any rate, where the component sounds have an inde- 
pendent origin — it is usually not difficult to detect them by the 
ear, so as to effect an analysis of the mixture. This is as much as 
to say that a strictly periodic vibration may give rise to a sensa- 
tion which is not simple, but susceptible of further analysis. In 
point of fisLct, it has long been known to musicians that under 
certain circumstances the harmonics of a note may be heard along 
with it, even when the note is due to a single source, such as a 
vibrating string ; but the significance of the fact was not under- 
stood. Since attention has been drawn to the subject, it has been 
proved (mainly by the labours of Ohm and Helmholtz) that almost 
all musical notes ai-e highly compound, consisting in fact of the 
notes of a harmonic scale, from which in particular cases one or 

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more members may be missing. The reason of the uncertainty 
and difficulty of the analysis will be touched upon presently. 

22. That kind of note which the ear cannot further resolve is 
called by Helmholtz in German a ' ton* Tyndall and other recent 
writei's on Acoustics have adopted ' tone' as an English equivalent, 
— a practice which will be followed in the present work. The 
thing is so important, that a convenient word is almost a matter 
of necessity. Notes then are in general made up of tones, the 
pitch of the note being that of the gravest tone which it contains. 

23. In strictness the quality of pitch must be attached in the 
first instance to simple tones only ; otherwise the difficulty of dis- 
continuity before referred to presents itself. The slightest change 
in the nature of a note may lower its pitch by a whole octave, as 
was exemplified in the case of the Siren. We should now rather 
say that the effect of the slight displacement of the alternate 
holes in that experiment was to introduce a new feeble tone an 
octave lower than any previously present. This is sufficient to 
alter the period of the whole, but the great mass of the sound 
remains very nearly as before. 

In most musical notes, however, the fundamental or gravest 
tone is present in sufficient intensity to impress its character on 
the whole. The effect of the harmonic overtones is then to modify 
the quality or character^ of the note, independently of pitch. 
That such a distinction exists is well known The notes of a violin, 
tuning fork, or of the human voice with its different vowel sounds, 
&c., may all have the same pitch and yet differ independently of 
loudness ; and though a part of this difference is due to accom- 
panying noises, which are extraneous to their nature as notes, still 
there is a part which is not thus to be accounted for. Musical 
notes may thus be classified as variable in three ways: First, pitch. 
This we have already sufficiently considered. Secondly, character, 
depending on the proportions in which the harmonic overtones are 
combined with the fundamental : and thirdly, loudness. This has 
to be taken last, because the ear is not capable of comparing 
(with any precision) the loudness of two notes which differ much 
in pitch or character. We shall indeed in a future chapter give a 
mechanical measure of the intensity of sound, including in one 
system all gradations of pitch ; but this is nothing to the point. 

^ German, 'Elangfarbe'— Fienoh, 'timbre.' The word 'character' is used in 
this sense by Everett. 

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We are here concerned with the intensity of the sensation of 
sound, not with a measure of its physical cause. The difference of 
loudness is, however, at once recognised as one of more or less ; so 
that we have hardly any choice but to regard it as dependent 
cceteris paribue on the magnitude of the vibrations concerned. 

24. We have seen that a musical note, as such, is due to a 
vibration which is necessarily periodic; but the converse, it is 
evident, cannot be true without limitation. A periodic repetition 
of a noise at int^i-vals of a second — for instance, the ticking of a 
clock — would not result in a musical note, be the repetition ever 
so perfect. In such a case we may say that the fundamental tone 
lies outside the limits of hearing, and although some of the 
harmonic overtones would fall within them, these would not give 
rise to a musical note or even to a chord, but to a noisy mass of 
sound like that produced by striking simultaneously the twelve 
notes of the chromatic scale. The experiment may be made with 
the Siren by distributing the holes quite irregularly round the 
circumference of a circle, and turning the disc with a moderate 
velocity. By the construction of the instrument, everything 
recurs after each complete revolution. 

26. The principal remaining difficulty in the theory of notes 
and tones, is to explain why notes are sometimes analysed by the 
ear into tones, and sometimes not. If a note is really complex, 
why is not the fact immediately and certainly perceived, and the 
components disentangled ? The feebleness of the harmonic over- 
tones is not the reason, for, as we shall see at a later stage of our 
inquiry, they are often of surprising loudness, and play a prominent 
part in music. On the other hand, if a note is sometimes perceived 
as a whole, why does not this happen always ? These questions 
have been carefully considered by Helmholtz\ with a tolerably 
satisfactory result. The difficulty, such as it is, is not peculiar to 
Acoustics, but may be paralleled in the cognate science of Physio- 
logical Optics. 

The knowledge of external things which we derive from the 
indications of our senses, is for the most part the result of inference. 
When an object is before us, certain nerves in our retinae are 
excited, and certain sensations are produced, which we are 
accustomed to associate with the object, and we forthwith infer its 
presence. In the case of an unknown object the process is much 
^ Tonempfindungeny 3rd edition, p. 9S. 

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the same. We interpret the sensations to which we are subject so 
as to form a pretty good idea of their exciting cause. From the 
slightly different perspective views received by the two eyes we 
infer, often by a highly elaborate process, the actual relief and 
distance of the object, to which we might otherwise have had no 
clue. These inferences are made with extreme rapidity and quite 
unconsciously. The whole life of each one of us is a continued 
lesson in interpreting the signs presented to us, and in drawing 
conclusions as to the actualities outside. Only so far as we succeed 
in doing this, are our sensations of any use to us in the ordinary 
affairs of life. This being so, it is no wonder that the study of our 
sensations themselves falls into the background, and that subjective 
phenomena, as they are called, become exceedingly difficult of 
observation. As an instance of thi^, it is sufficient to mention the 
'blind spot' on the retina, which might a priori have been 
expected to manifest itself as a conspicuous phenomenon, though 
as a fact probably not one person in a hundred million would find 
it out for themselves. The application of these remarks to the 
question in hand is tolerably obvious. In the daily use of our ears 
our object is to disentangle from the whole mass of sound that 
may reach us, the parts coming from sources which may interest 
us at the moment. When we listen to the conversation of a friend, 
we fix our attention on the sound proceeding from him and 
endeavour to grasp that as a whole, while we ignore, as far as 
possible, any other sounds, regarding them as an interruption. 
There are usually sufficient indications to assist us in making this 
partial analysis. When a man speaks, the whole sound of his 
voice rises and falls together, and we have no difficulty in recog- 
nising its unity. It would be no advantage, but on the contrary 
a great source of confusion, if we were to carry the analjrsis further, 
and resolve the whole mass of sound present into its component 
tones. Although, as regards sensation, a resolution into tones 
might be expected, the necessities of our position and the practice 
of our lives lead us to stop the analysis at the point, beyond 
which it would cease to be of service in deciphering our sensa- 
tions, considered as signs of external objects^ 

But it may sometimes happen that however much we may 
wish to form a judgment, the materials for doing so are absolutely 

1 Most probably the power of attending to the important and ignoring the 
unimportant part of our sensations is to a great extent inherited — to how great an 
extent we shall perhaps never know. 

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wanting. When a note and its octave are sounding close together 
and with perfect uniformity, there is nothing in our sensations to 
enable us to distinguish, whether the notes have a double or a 
single origin. In the mixture stop of the organ, the pressing down 
of each key admits the wind to a group of pipes, giving a note and 
its first three or four harmonics. The pipes of each group always 
sound together, and the result is usually perceived as a single 
note, although it does not proceed from a single source. 

26. The resolution of a note into its component tones is a 
matter of very diflFerent difficulty with different individuals. A 
considerable effort of attention is required, particularly at first ; 
and, until a habit has been formed, some external aid in the shape 
of a suggestion of what is to be listened for, is very desirable. 

The difficulty is altogether very similar to that of learning to 
draw. From the machinery of vision it might have been expected 
that nothing would be easier than to make, on a plane surface, a 
representation of surrounding solid objects ; but experience shews 
that much practice is generally required. 

We shall return to the question of the analysis of notes at a 
later stage, after we have treated of the vibrations of strings, with 
the aid of which it is best elucidated; but a very instructive 
experiment, due originally to Ohm and improved by Helmholtz, 
may be given here. Helmholtz^ took two bottles of the shape 
represented in the figure, one about twice as large as the other. 
These were blown by streams of air directed 
across the mouth and issuing from gutta-percha 
tubes, whose ends had been softened and pressed 
flat, so as to reduce the bore to the form of a 
narrow slit, the tubes being in connection with 
the same bellows. By pouring in water when 
the note is too low and by partially obstructing 
the mouth when the note is too high, the bottles 
may be made to give notes with the exact 
interval of an octave, such as b and b'. The 
larger bottle, blown alone, gives a somewhat muffled sound similar 
in character to the vowel U ; but, when both bottles are blown, 
the character of the resulting sound is sharper, resembling rather 
the vowel O. For a short time after the notes had been heard 
separately Helmholtz was able to distinguish them in the mixture ;. 

^ Tonempfindungen, p. 109. 

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but as the memory of their separate impressions fisMled, the higher 
note seemed by degrees to amalgamate with the lower, which at 
the same time became louder and acquired a sharper character. 
This blending of the two notes may take place even when the high 
note is the louder. 

27. Seeing now that notes are usually compound, and that 
only a particular sort called tones are incapable of further analysis, 
we are led to inquire what is the physical characteristic of tones, 
to which they owe their peculiarity? What sort of periodic vibra- 
tion is it, which produces a simple tone? According to what 
mathematical function of the time does the pressure vary in 
the passage of the ear ? No question in Acoustics can be more 

The simplest periodic functions with which mathematicians 
are acquainted are the circular functions, expressed by a sine or 
cosine; indeed there are no others at all approaching them in 
simplicity. They may be of any period, and admitting of no 
other variation (except magnitude), seem well adapted to produce 
simple tones. Moreover it has been proved by Fourier, that the 
most general single-valued periodic function can be resolved into 
a series of circular functions, having periods which are submultiples 
of that of the given function. Again, it is a consequence of the 
general theory of vibration that the particular type, now suggested 
as corresponding to a simple tone, is the only one capable of 
preserving its integrity among the vicissitudes which it may 
have to undergo. Any other kind is liable to a sort of physical 
analysis, one part being diflferently aflfected from another. If the 
analysis within the ear proceeded on a different principle from that 
effected according to the laws of dead matter outside the ear, 
the consequence would be that a sound originally simple might 
become compound on its way to the observer. There is no reason 
to suppose that anything of this sort actually happens. When it 
is added that according to all the ideas we can form on the subject, 
the analysis within the ear must take place by means of a physical 
machinery, subject to the same laws as prevail outside, it will be 
seen that a strong case has been made out for regarding tones as 
due to vibmtions expressed by circular functions. We are not 
however left entirely to the guidance of general considerations like 
these. In the chapter on the vibration of strings, we shall see 
that in many cases theory informs us beforehand of the nature of 
B. 2 

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the vibration executed by a string, and in particular whether any 
specified simple vibration is a component or not Here we have 
a decisive test. It is found by experiment that, whenever according 
to theory any simple vibration is present, the corresponding tone 
can be heard, but, whenever the simple vibration is absent, then 
the tone cannot be heard. We are therefore justified in asserting 
that simple tones and vibrations of a circular type are indissolubly 
connected. This law was discovered by Ohm. 

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28. The vibrations expressed by a circular function of the 
time and variously designated as simple, pendulous, or harmonic, 
are so important in Acoustics that we cannot do better than devote 
a chapter to their consideration, before entering on the dynamical 
part of our subject. The quantity, whose variation constitutes 
the ' vibration/ may be the displacement of a particle measured 
in a given direction, the pressure at a fixed point in a fluid 
medium, and so on. In any case denoting it by u, we have 

w = acos 

(v*-) (>^ 

in which a denotes the amplitude, or extreme value of • u ; r is 
the periodic tims, or period, after the lapse of which the values 
of u recur ; and e determines the phase of the vibration at the 
moment from which t is measured. 

Any number of harmonic vibrations of the sams period affect- 
ing a variable quantity, compound into another of the same tj^e, 
whose elements are determined as follows : 

ti = Sa cos 


= cos — 2acos€ + sm — zasme 

T T 

= rco8(2^-6») (2), 

if r={(2acoee)» + (2asine)«ji (3), 

and tan ^ = Sa sin 6 -r Sa cos 6 (4). 

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For example, let there be two components, 

t* = aco8( e\'^a coe( 6 I; 

then r = {a« + a'«+2aa' cos (€-€)}* (5), 

tantf = ; — ; -J (6). 

acos6 + a cose 

Particular cases may be noted. If the phases of the two com- 

ponents agree, 

. , ^ /27rt \ 
t^=s(a + ajcos( €j. y 

If the phases differ by half a period, 

w = (a — a ) cos ( € 1 , 

so that if a' "= a, t^ vanishes. In this case the vibrations are often 
said to interfere, but the expression is rather misleading. Two 
sounds may very properly be said to interfere, when they together 
cause silence; but the mere superposition of two vibrations 
(whether rest is the consequence, or not) cannot properly be so 
called. At least if this be interference, it is difficult to say what 
non-interference can be. It will appear in the course of this 
work that when vibrations exceed a certain intensity they no 
longer compound by mere addition; this mutual action might 
more properly be called interference, but it is a phenomenon 
of a totally different nature from that with which we are now 

Again, if the phases differ by a quarter or by three-quarters of 
a period, cos (c — e') = 0, and 

Harmonic vibrations of given period may be represented 
by lines drawn from a pole, the lengths of the lines being pro- 
portional to the amplitudes, and the inclinations to the phases 
of the vibrations. The resultant of any number of harmonic 
vibrations is then represented by the geometrical resultant of 
the corresponding lines. For example, if they are disposed 
symmeftrically round the pole, the resultant of the lines, or 
vibrations, is zero. 

29. If we measure off along an axis of x distances pro- 
portional to the time, and take u for an ordinate, we obtain the 
harmonic curve, or curve of sines. 

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u = aco8 


where X, called the wave-length, is written in place of t, both 
quantities denoting the range of the independent variable corre- 
sponding to a complete recurrence of the function. The harmonic 
curve is thus the locus of a point subject at once to a uniform 
motion, and to a harmonic vibration in a perpendicular direc- 
tion. In the next chapter we shall see that the vibration of a 
tuning fork is simple harmonic; so that if an excited tuning 
fork be moved with uniform velocity parallel to the line of its 
handle, a tracing point attached to the end of one of its prongs 
describes a harmonic curve, which may be obtained in a permanent 
form by allowing the tracing point to bear gently on a piece of 
smoked paper. In Fig. 2 the continuous lines are two harmonic 
curves of the same wave-length and amplitude, but of different 

phases ; the dotted ^curve represents half their resultant, being 
the locus of points midway between those in which the two 
curves are met by any ordinate. 

30. If two harmonic vibrations of different periods coexist^ 

/27rt \ , , /27rt A 
I* = a cos ( 6 j -H a cos ( — -, — e j. 

The resultant cannot here be represented as a simple harmonic 
motion with other elements. If r and r be incommensurable, the 
value of u never recurs ; but, if t and t' be in the ratio of two 
whole numbers, u recurs after the lapse of a time equal to the 
least common multiple of r and r'; but the vibration is not 
simple harmonic. For example, when a note and its fifth are 
sounding together, the vibration recurs after a time equal to 
twice the period of the graver. 

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One case of the composition of harmonic vibrations of different 
periods is worth special discussion, namely, when the difference 
of the periods is small. If we fix our attention on the course 
of things diuring an interval of time including merely a few 
periods, we see that the two vibrations are nearly the same as 
if their periods were absolutely equal, in which case they would, 
as we know, be equivalent to another simple harmonic vibration 
of the same period. For a few periods then the resultant 
motion is approximately simple harmonic, but the same har- 
monic will not continue to represent it for long. The vibration 
having the shorter period continually gains on its fellow, thereby 
altering the difference of phase on which the elements of the 
resultant depend. For simplicity of statement let us suppose 
that the two components have equal amplitudes, frequencies 
represented by m and n, where m — h is small, and that when 
first observed their phases agree. At this moment their effects 
conspire, and the resultant has an amplitude double of that of 
the components. But after a time 1 -r 2 (m — n) the vibration 
m will have gained half a period relatively to the other; and 
the two, being now in complete disagreement, neutralize each 
other. After a further interval of time equal to that above 
named, m will have gained altogether a whole vibration, and 
complete accordance is once more re-established. The resultant 
motion is therefore approximately simple harmonic, with an 
amplitude not constant, but varying from zero to twice that of 
the components, the frequency of these alterations being m— n. 
If two tuning forks with frequencies 500 and 501 be equally 
excited, there is every second a rise and fall of sound corre- 
sponding to the coincidence or opposition of their vibrations. 
This phenomenon is called beats. We do not here fully discuss 
the question how the ear behaves in the presence of vibrations 
having nearly equal frequencies, but it is obvious that if the motion 
in the neighbourhood of the ear almost cease for a considerable 
fraction of a second, the sound must appear to fall. For reasons 
that will afterwards appear, beats are best heard when the in- 
terfering sounds are simple tonea Consecutive notes of the 
stopped diapason of the organ shew the phenomenon very 
well, at least in the lower parts of the scale. A permanent inter- 
ference of two notes may be obtained by mounting two stopped 
organ pipes of similar construction and identical pitch side by 
side on the same wind chest. The vibrations of the two pipes 

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adjust themselves to complete opposition, so that at a little 
distance nothing can be heard, except the hissing of the wind. 
If by a rigid wall between the two pipes one sound could be 
cut off, the other would be instantly restored. Or the balance, 
on which silence depends, may be upset by connecting the ear 
with a tube, whose other end lies close to the mouth of one of the 

By means of beats two notes may be tuned to unison with 
great exactness. The object is to make the beats as slow as 
possible, since the number of beats in a second is equal to the 
difference of the frequencies of the notes. Under favourable 
circumstances. beats so slow as one in 30 seconds may be recog- 
nised, and would indicate that the higher note gains only two 
vibrations a minute on the lower. Or it might be desired merely 
to ascertain the difference M the frequencies of two notes nearly 
in unison, in which case nothing more is necessary than to count 
the number of beats. It will be remembered that the difference 
of frequencies does not determine the interval between the two 
notes; that depends on the ratio of frequencies. Thus the 
rapidity of the beats given by two notes nearly in unison is 
doubled, when both are taken an exact octave higher. 


u = acos (2'rrmt — e) + a' cos (iimt — €'), 
where m — n is small 

Now cos (27171* — e') may be written 

cos [2'rrmt — 27r (m — n) t — e'}, 
and we have 

t* = rcos(27rm*— ^) (1), 

where r" = a« + a''+ 2aa'cos{27r(m-n)* + 6' -6} (2), 

^ asinc + a'sin {27r(m — n)* + 6'} .«v 

tan u — ■ ; — ; rs — ; rr— — 7> \o). 

a cos e + a cos [27r (m — n) f + e j 

The resultant vibration may thus be considered as harmonic 
with elements r and d, which are not constant but slowly varying 
functions of the time, having the frequency m — n. The ampli- 
tude r IB at its maximum when 

cos {27r (m -7i) < + e' - €} = + 1, 
and at its minimum when 

COS {27r (m - n) * + 6' — 6} = — 1, 
the corresponding values being a + a' and a — a respectively. 

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31. Another case of great importance is the composition of 
Vibrations corresponding to a tone and its harmonics. It is known 
that the most general single-valued finite periodic function can 
be expressed by a series of simple harmonics — 

U = ao + l^i OnCOSl— 6nl (1), 

a theorem usually quoted as Fourier's. Analytical proofs will be 
found in Todhunter's Integral Calculus and Thomson and Taits 
Natural Philosophy; and a line of argument almost if not quite 
amounting to a demonstration will be given later in this work. 
A few remarks are all that will be required here. 

Fourier's theorem is not obvioua A vague notion is not un- 
common that the infinitude of arbitrary constants in the series 
of necessity endows it with the capacity of representing an arbi- 
trary periodic function. That this is an error will be apparent, 
when it is observed that the same argument would apply equally, 
if one term of the series were omitted ; in which case the ex- 
pansion would not in general be possibla 

Another point worth notice is that simple harmonics are not 
the only functions, in a series of which it is possible to expand 
one arbitrarily given. Instead of the simple elementary term 

we might take 

formed by adding a similar one in the same phase of half the 
amplitude and period. It is evident that these terms would 
serve as well as the others; for 


f2mU \ ( /2'jmt \ 1 /^nt \] 

1 ( /Svnt \ . 1 /Uimt \) 

— ad infin.y 

so that each term in Fourier's series, and therefore the sum of 
the series, can be expressed by means of the double elementary 

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31.] Fourier's theorem. 25 

terms now suggested This is mentioned here, because students, 
not being acquainted with other expansions, may imagine that 
simple harmonic functions are by nature the only ones qualified 
to be the elements in the development of a periodic function. 
The reason of the preeminent importance of Fourier's series in 
Acoustics is the mechanical one referred to in the preceding 
chapter, and to be explained more fully hereafter, namely, that, 
in general, simple harmonic vibrations are the only kind that are 
propagated through a vibrating system without suffering decom- 

32. As in other cases of a similar character, e.g. Taylor's 
theorem, if the possibility of the expansion be known, the co- 
efficients may be determined by a comparatively simple process. 
We may write (1) of § 31 

W = ilo + 2^i ilnCOS-— -+2^.ifi„8in-— - (1). 

T T 

Multiplying by cos (inirt/r) or sin (2n7rt/T), and integrating 
over a complete period fi:om ^ = to < = t, we find 

. 2 r 2n7r< ,A 
An = - I wcos at 

T J T 

T J T 

An immediate integration gives 

ilo = - Twcft (3), 

T J 

indicating that Aq is the mean value of v throughout the period. 

The degree of convergency in the expansion of u depends in 
general on the continuity of the function and its derivatives. 
The series formed by successive differentiations of (1) converge 
less and less rapidly, but still remain convergent, and arithmetical 
representatives of the differential coefficients of u, so long as 
these latter are everywhere finite. Thus (Thomson and Tait, 
§ 77), if all the derivatives up to the m^ inclusive be free 
from infinite values, the series for u is more convergent than 
one with 


for coefficients. 

1 i 1 1 &c 
* 2^' 3«' 4»»' ' 

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32 a. The general explanation of the b^ts heard when two 
pure tones nearly in unison are sounded simultaneously has been 
discussed in § 30. But the occurrence of beats is not confined to 
the case of approximate unison, at least when we have to deal 
with compound notes. Suppose for example that the interval 
IB an octave. The graver note then usually includes a tone 
coincident in pitch with the fundamental tone of the higher note. 
If the interval be disturbed, the previously coincident tones 
separate from one another, and give rise to beats of the same 
firequency as if they existed alone. There is usually no difficulty 
in observing these beats; but if one or both of the component 
tones concerned be very faint, the aid of a resonator may be 

In general we may consider that each consonant interval is 
characterized by the coincidence of certain component tones, and 
if the interval be disturbed the previously coincident tones 
give rise to beats. Of course it may happen in any particular 
case that the tones which would coincide in pitch are absent from 
one or other of the notes. The disturbance of the interval 
would then, according to the above theory, not be attended 
by beats. In practice faint beats are usually heard; but the 
discussion of this phenomenon, as to which authorities are not 
entirely agreed, must be postponed. 

33. Another class of compounded vibrations, interesting from 
the facility with which they lend themselves to optical observa- 
tion, occur when two harmonic vibrations affecting the same par- 
ticle are executed in perpendicular directions, more especially 
when the periods are not only commensurable, but in the ratio 
of two small whole numbers. The motion is then completely 
periodic, with a period not many times greater than those of the 
components, and the curve described is re-entrant. If u and v 
be the co-ordinates, we may take 

w = a cos (27m< — €), v = 6cos2im'^ (1). 

First let us suppose that the periods are equal, so that n' ^n\ 
the elimination of t gives for the equation of the curve described, 

representing in general an ellipse, whose position and dimensions 
depend upon the amplitudes of the original vibrations and upon 

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the difference of their phases. If the phases differ by a quarter 
period, cos € » 0, and the equation becomes 

— 4--- = 1 

In this case the axes of the ellipse coincide with those of 
co-ordinates. If further the two components have equal ampli- 
tudes, the locus degenerates into the circle 

which is described with uniform velocity. This shews how a 
uniform circular motion may be analysed into two rectilinear 
harmonic motions, whose directions are perpendicular. 

If the phases of the components agree, e » 0, and the ellipse 
degenerates into the coincident straight lines 

or if the difference of phase amount to half a period, into 


When the unison of the two vibrations is exact, the elliptic 
path remains perfectly steady, but in practice it will almost 
always happen that there is a slight difference between the 
periods. The consequence is that though a fixed ellipse represents 
the curve described with sufficient accuracy for a few periods, 
the ellipse itself gradually changes in correspondence with the 
alteration in the magnitude of 6. It becomes therefore a matter 
of interest to consider the system of ellipses represented by (2), 
supposing a and b constants, but e variable. 

Since the extreme values of u and v are ±a, ±b respectively, 
the ellipse is in all cases inscribed in the rectangle whose sides 
are 2a, 26. Starting with the phases in agreement, or e^O, we 

have the ellipse coincident with the diagonal — 1~^' -^ 

€ increases from to ^v, the ellipse opens out until its equation 

a»^6> ^• 
From this point it closes up again, ultimately coinciding with 

the other diagonal ~ + i == 0» corresponding to the increase of € ft^m 

J^ to ^. After this, as € ranges from tt to 27r, the ellipse retraces 

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its course until it again coincides with the first diagonal. The 
sequence of changes is exhibited in Fig. 3. 








C ) 


^ ^-^ 


The ellipse, having already four given tangents, is completely 
determined by its point of contact P (Fig. 4) with the line v = 6. 


F/ G. -4. 

P A 


"^ ^ 






In order to connect this with e, it is sufficient to observe that 
when t; = &, cos27m^ = l; and therefore tt = acos€. Now if the 
elliptic paths be the result of the superposition of two harmonic 
vibrations of nearly coincident pitch, € varies uniformly with the 
time, so that P itself executes a harmonic vibration along A A' 
with a frequency equal to the difference of the two given fre- 

34. Lissajous^ has shewn that this sjrstem of ellipses may be 
regarded as the different aspects of one and the same ellipse 
described on the surfisice of a transparent cylinder. In Fig. 5 

1 AwuOm de Chimie (8) lx. 147, 1857. 

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A A' SB represents the cylinder, of which AS is a plane section. 
Seen from an infinite distance in the direction of the common 
tangent at il to the plane sections, the cylinder is projected into a 
rectangle, and the ellipse into its diagonal. Suppose now that the 
cylinder turns upon its axis, carrying the plane section with it. 
Its own projection remains a constant rectangle in which the pro- 

F/G. 6. 

jection of the ellipse is inscribed. Fig. 6 represents the posi- 
tion of the cylinder after a rotation through a right angle. It 
appears therefore that by turning the cylinder round we obtain in 
succession all the ellipses corresponding to the paths described by 
a point subject to two harmonic vibrations of equal period and fixed 
amplitudes. Moreover if the cylinder be turned continuously 
with uniform velocity, which insures a harmonic motion for P, 
we obtain a complete representation of the varjdng orbit de- 
scribed by the point when the periods of the two components 
differ slightly, each complete revolution answering to a gain or 
loss of a single vibration^ The revolutions of the cylinder are 
thus synchronous with the beats which would result from the 
composition of the two vibrations, if they were to act in the same 

36. Vibrations of the kind here considered are very easily 
realized experimentally. A heavy pendulum-bob, hung fi^m a 
fixed point by a long wire or string, describes ellipses under the 
action of gravity, which may in particular cases, according to the 
circumstances of projection, pass into straight lines or circles. 
But in order to see the orbits to the best advantage, it is necessary 
that they should be described so quickly that the impression 
on the retina made by the moving point at any part of its course 
has not time to fade materially, before the point comes round again 
to renew its action. This condition is fulfilled by the vibration of 
a silvered bead (giving by reflection a luminous point), which is 

^ By a Tibrstion will always be meant in this work a complete oyole of changes. 

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attached to a straight metallic wire (such as a knitting-needle)* 
firmly clamped in a vice at the lower end. When the system is set 
into vibration, the luminous point describes ellipses, which appear 
as fine lines of light. These ellipses would gradually contract in 
dimensions under the influence of friction until they subsided 
into a stationary bright point, without undergoing any other 
change^ were it not that in all probability, owing to some want 
of symmetry, the wire has slightly differing periods according to 
the plane in which the vibration is executed. Under these cir- 
cumstances the orbit is seen to undergo the cycle of changes 
already explained. # 

36. So far we have supposed the periods of the component 
vibrations to be equal, or nearly equal ; the next case in order of 
simplicity is when one is the double of the other. We have 

t^ = a cos (im-rrt — c), t; = 6 cos 2mrt. 
The locus resulting from the elimination of t may be written 



- = cose 


i^i-^y^^-W^-t «■ 

which for all values of e represents a curve inscribed in the rect- 
angle 2a, 26. If € « 0, or ir, we have 



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representing parabolas. Fig. 7 shews the various curves for the 
intervals of the octave, twelfth, and fifth. 

To all these systems Lissajous' method of representation by 
the transparent cylinder is applicable, and when the relative 
phase is altered, whether from the different circumstances of 
projection in different cases, or continuously owing to a slight 
deviation from exactness in the ratio of the periods, the cylinder 
will appear to turn, so as to present to the eye different aspects of 
the same line traced on its surface. 

37. There is no difficulty in arranging a vibrating system so 
that the motion of a point shall consist of two harmonic vibrations 
in' perpendicular planes, with their periods in any assigned ratio. 
The simplest is that known as Blackburn's pendulum. A wire 
ACB ia fastened at A and B, two fixed points at the same level. 
The bob P is attached to its middle point by another wire CF. 
For vibrations in the plane of the diagram, the point of suspension 
is practically (7, provided that the wires are sufficiently stretched ; 
but for a motion perpendicular to this plane, the bob turns about 
D, carrying the wire ACB with it. The periods of vibration in 

the principal planes are in the ratio of the square roots of CF and 
DF. Thus if DO = 30P, the bob describes the figures of the 
octave. To obtain the sequence of curves corresponding to 
approximate unison, ACB must be so nearly tight, that CD is 
relatively small. 

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38. Another contrivance called the kaleidophone was origin- 
ally invented by Wheatstone. A straight thin bar of steel carrying- 
a bead at its upper end is fastened in a vice, as explained in a 
previous paragraph. If the section of the bar is square, or circular, 
the period of vibration is independent of the plane in which it is 
performed. But let us suppose that the section is a rectangle 
with unequal sides. The stiffness of the bar — the force with 
which it resists bending — is then greater in the plane of greater 
thickness, and the vibrations in this plane have the shorter period. 
By a suitable adjustment of the thicknesses, the two periods of 
vibration may be brought into any required ratio, and the cor- 
responding curve exhibited. 

The defect in this ai*rangeraent is that the same bar will give 
only one set of figures. In order to overcome this objection 
the following modification has been devised. A slip of steel is 
taken whose rectangular section is very elongated, so that as 
regards bending in one plane the stiffness is so great as to amount 
practically to rigidity. The bar is divided into two parts, and the 
broken ends reunited, the two pieces being turned on one another 
through a right angle, so that the plane, which contains the small 
thickness of one, contains the great thickness of the other. When 
the compound rod is clamped in a vice at a point below the junc- 
tion, the period of the vibration in one direction, depending almost 
entirely on the length of the upper piece, is nearly constant ; but 
that in the second direction may be controlled by varying the 
point at which the lower piece is clamped. 

39. In this arrangement the luminous point itself executes 
the vibrations which are to be observed ; but in Lissajous' form of 
the experiment, the point of light remains really fixed, while its 
image is thrown into apparent motion by means of successive 
reflection from two vibrating mirrors. A small hole in an opaque 
screen placed close to the flame of a lamp gives a point of light, 
which is observed after reflection i)i the mirrors by means of a 
small telescope. The mirrors, usually of polished steel, are attached 
to the prongs of stout tuning forks, and the whole is so disposed 
that wbeu the forks are thrown into vibration the luminous point 
appears to describe harmonic motions in perpendicular directions, 
owing to the angular motions of the reflecting surfaces. The 
amplitudes and periods of these harmonic motions depend upon 
those of the corresponding forks, and may be made such as to give 

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with enhanced brilliancy any of the figures possible with the 
kaleidophone. By a similar arrangement it is possible to project 
the figures on a screen. In either case they gradually contract as 
the vibrations of the forks die away. 

40. The principles of this chapter have received an important 
application in the investigation of rectilinear periodic motions. 
When a point, for instance a particle of a sounding string, is 
vibrating with such a period as to give a note within the limits of 
hearing, its motion is much too rapid to be followed by the eye ; 
so that, if it be required to know the character of the vibration, 
some indirect method must be adopted. The simplest, theo- 
retically, is to compound the vibration under examination with a 
uniform motion of translation in a perpendicular direction, as when 
a tuning-fork draws a harmonic curve on smoked paper. Instead 
of moving the vibrating body itself, we may make use of a revolv- 
ing mirror, which provides us with an image in motion. In this 
way we obtain a representation of the function characteristic of 
the vibration, with the abscissa proportional to time. 

But it often happens that the application of this method would 
be difficult or inconvenient. In such cases we may substitute for 
the uniform motion a harmonic vibration of suitable period in the 
same direction. To fix our ideas, let us suppose that the point, 
whose motion we wish to investigate, vibrates vertically with a 
period r, and let us examine the result of combining with this a 
horizontal harmonic motion, whose period is some multiple of t, 
say, riT. Take a rectangiilar piece of paper, and with axes parallel 
to its edges draw the curve representing the vertical motion (by 
setting off abscissae proportional to the time) on such a scale that 
the paper just contains n repetitions or waves, and then bend the 
paper round so as to form a cylinder, with a re-entrant curve run- 
ning round it. A point describing this curve in such a manner 
that it revolves uniformly about the axis of the cylinder will 
appear from a distance to combine the given vertical motion of 
period T, with a horizontal harmonic motion of period nr. Con- 
versely therefore, in order to obtain the representative curve of 
the vertical vibrations, the cylinder containing the apparent path 
must be imagined to be divided along a generating line, and 
developed into a plane. There is less difficulty in conceiving the 
cylinder and the situation of the curve upon it, when the adjust- 
ment of the periods is not quite exact, for then the cylinder 
B. 3 

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appears to turn, and the contrary motions serve to distinguish 
those parts of the curve which lie on its nearer and further face. 

41. The auxiliary harmonic motion is generally obtained 
optically, by means of an instrument called a vibration-microscope 
invented by Lissajous. One prong of a large tuning-fork carries 
a lens, whose axis is perpendicular to the direction of vibration ; 
and which may be used either by itself, or as the object-glass of 
a compound microscope formed by the addition of an eye-piece 
independently suppoiiied. In either case a stationary point i& 
thrown into apparent harmonic motion along a line parallel to 
that of the fork's vibration. 

The vibration-microscope may be applied to test the rigour 
and universality of the law connecting pitch and period. Thus 
it will be found that any point of a vibrating body which gives 
a pure miisical note will appear to describe a re-entrant curve, 
when examined with a vibration-microscope whose note is in 
strict unison with its own. By the same means the ratios of 
frequencies characteristic of the consonant intervals may be 
verified; though for this latter purpose a more thoroughly 
acoustical method, to be described in a future chapter, may be 

42. Another method of examining the motion of a vibrating 
body depends upon the use of intermittent illumination^ Suppose, 
for example, that by means of suitable apparatus a series of 
electric sparks are obtained at regular intervals t. A vibrating 
body, whose period is also t, examined by the light of the sparks- 
must appear at rest, because it can be seen only in one position. 
If, however, the period of the vibration diflFer from t ever so 
little, the illuminated position varies, and the body will appear 
to vibrate slowly with a frequency which is the difference of that 
of the spark and that of the body. The type of vibration can 
then be observed with facility. 

The series of sparks can be obtained from an induction-coil, 
whose primary circuit is periodically broken by a vibrating fork,, 
or by some other interrupter of sufficient regularity. But a better 
result is afforded by sunlight rendered intermittent with the aid of 
a fork, whose prongs carry two small plates of metal, parallel ta 
the plane of vibration and close together. In each plate is a slit 

^ Plateau, Bull, de VAead. roy. de Belgique, t. iii, p. 364, 1836. 

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parallel to the prongs of the fork, and so placed as to afford a 
free passage through the plates when the fork is at rest, or passing 
through the middle point of its vibrations. On the openAig so 
formed, a beam of sunlight is concentrated by means of a burning- 
glass, and the object under examination is placed in the cone of 
rays diverging on the further side*. When the fork is made to 
vibrate by an electro-magnetic arrangement, the illumination is cut 
oflF except when the fork is passing through its position of equi- 
librium, or nearly so. The flashes of light obtained by this method 
are not so instantaneous as electric sparks (especially when a 
jar is connected with the secondary wire of the coil), but in my 
experience the regularity is more perfect. Care should be taken 
to cut off extraneous light as far as possible, and the effect is then 
very striking. 

A similar result may be arrived at by looking at the vibrating 
body through a series of holes arranged in a circle on a revolving 
disc. Several series of holes may be provided on the same 
disc, but the observation is not satisfactory without some pro- 
vision for securing uniform rotation. 

Except with respect to the sharpness of definition, the result is 
the same when the period of the light is any multiple of that of 
the vibrating body. This point must be attended to when the 
revolving wheel is used to determine an unknown frequency. 

When the frequency of intermittence is an exact multiple of 
that of the vibration, the object is seen without apparent motion, 
but generally in more than one position. This condition of things 
is sometimes advantageous. 

Similar effects arise when the frequencies of the vibrations 
and of the flashes are in the ratio of two small whole numbers. 
If, for example, the number of vibrations in a given time be half 
as great again as the number of flashes, the body will appear 
stationary, and in general double. 

42 a. We have seen (§ 28) that the resultant of two isoperiodic 
vibrations of equal amplitude is wholly dependent upon their phase 
relation, and it is of interest to inquire what we are to expect 
from the composition of a large number (n) of equal vibmtions 
of amplitude unity, of the same period, and of phases accidentally 
determined. The intensity of the resultant, represented by the 
square of the amplitude § 245, will of course depend upon the 

1 Topler, Phil. Mag. Jan. 1867. 

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precise manner in which the phases are distributed, and may vary 
from n^ to zero. But is there a definite intensity which becomes 
more and more probable when n is increased without limit ? 

The nature of the question here mised is well illustrated by 
the special case in which the possible phases are restricted to two 
opposite phases. We may then conveniently discard the idea of 
phase, and regard the amplitudes as at random positive or negative. 
If all the signs be the same, the intensity is n^ ; if, on the other 
hand, there be as many positive as negative, the result is zero. 
But although the intensity may range from to n', the smaller 
values are more probable than the greater. 

The simplest part of the problem relates to what is called in 
the theory of probabilities the " expectation " of intensity, that 
is, the mean intensity to be expected after a great number of 
trials, in each of which the phases are taken at random. The 
chance that all the vibrations are positive is (^)*^, and thus the 
expectation of intensity corresponding to this contingency is 
{\Y.n^. In like manner the expectation corresponding to the 
number of positive vibrations being (/i— 1) is 


and so on. The whole expectation of intensity is thus 

^ n(n-l)(n-2) ^^_g^^ I ^^^ 

Now the sum of the (n + 1) terms of this series is simply n, as 
may be proved by comparison of coefficients of a;* in the equivalent 

(e« + e-*)** = 2« (l-h ia:» + . . .)*» 

= e*** + n e <*»-*>* + '^ , "^ - e('»-^J*+ . . .. 
X . z 

The expectation of intensity is therefore n, and this whether n be 
great or small. 

The same conclusion holds good when the phases are unre- 
stricted. From (3) § 28, if Oi = Oa = . . . = 1, 

r* = (cos €i + cos es +...)" H- (sin €i + sin Cj + . . . )* 

= 71 + 22 cos (€,-€,) (2), 

where under the sign of summation are to be included the cosines 
of the ^(?i — 1) diflFerences of phase. When the phases are 

Digitized by 


42 a.] PHASES AT RANDOM, 37 

accidental, the sum is as likely to be positive as negative, and 
thus the mean value of r* is n. 

The reader must be on his guard here against a fallacy which 
has misled some eminent authors. We have not proved that when 
n is large there is any tendency for a single combination to give 
an intensity equal to n, but the quite different proposition that in 
a large number of trials, in each of which the phases are dis- 
tributed at random, the mean intensity will tend more and more 
to the value n. It is true that even in a single combination there 
is no reason why any of the cosines in (2) should be positive 
rather than negative. From this we may infer that when n is 
increased the sum of the terms tends to vanish in comparison with 
the number of terms ; but, the number of the terms being of the 
order n^ we can infer nothing as to the value of the sum of the 
series in comparison with n. 

So far there is no diiBculty; but a complete investigation of 
this subject involves an estimate of the relative probabilities of 
resultants lying within assigned limits of magnitude. For example, 
we ought to be able to say what is the probability that the 
intensity due to a large number (n) of equal components is less 
than ^n. This problem may conveniently be considered here, though 
it is naturally beyond the reach of elementary methods. We will 
commence by taking it under the restriction that the phases are 
of two opposite kinds only. 

Adopting the statistical method of statement, let us suppose 
that there are an immense number JV of independent combinations, 
each consisting of n unit vibrations, positive or negative, and com- 
bined accidentally. When N is sufficiently large, the statistics 
become regular; and the number of combinations in which the 
resultant amplitude is found equal to x may be denoted by 
N ,f{n, x), where /is a definite function of n and a?. Now suppose 
that each of the N combinations receives another random contri- 
bution of ± 1, and inquire how many of them will subsequently 
possess a resultant x. It is clear that those only can do so which 
originally had amplitudes x — l, or a?+l. Half of the former, 
and half of the latter number will acquire the amplitude x, so 
that the number required is 

iNf(n,x-^l) + iNfin,x + l). 
But this must be identical with the number corresponding to 
n + 1 and x, so that 

/(n-hl,^)«i/(n,^-l)^i/(»,^-hl) (3). 

Digitized by 



This equation of differences holds good for all integral values 
of X and for all positive integral values of n. If /(n, x) be given 
for one value of n, the equation suflSces to determine / (n, x) for 
all higher integral values of n. For the present purpose the 
initial value of n is zero. In that case we know that /(a?) = for 
all values of x other than zero, and that when x = 0,/(0, 0) = 1. 

The problem proposed in the above form is perfectly definite ; 
but for our immediate object it suffices to limit ourselves to the 
supposition that n is great, regarding /(n, x) -sa a continuous 
function of continuous variables n and x, much as in the analogfMiS 
problem ofg 120, 121, 122. 

Writing (3) in the form 

f(n + 1, x) ^/(n, x) = i/(n, a^ - 1) + if(n, x+l) --/(n, x). . .(4), 

we see that the left-hand member may then be identified with 
dfldn, and the right-hand member with i^^fjda^, so that under 
these circumstances the differential equation to which (3) reduces 
is of the well-known form 

dn^ 2dx^ ^^^• 

The analogy with the conduction of heat is indeed very close ; 
and the methods developed by Fourier for the solution of problems 
in the latter subject are at once applicable. The special condition 
here is that initially, that is when n = 0, / must vanish for all 
values of x other than zero. As may be verified by differentiation, 
the special solution of (5) is then 

f{n,x) = ^e-^l^ <«>• 

in which il is an arbitrary constant to be determined from the 
consideration that the whole number of combinations is N. Thus, 
if dx be large in comparison with unity, the number of combina- 
tions which have amplitudes between x and x-^-dxia 


AN [^-> 

while -T- / er^f^dx = N, 

In J -00 

80 that in virtue of the known equality 



J —OP 

A . V2^ =. 1. 


Digitized by ' 

42 a.] PHASES AT RANDOM. 39 

The final result for the number of combinations which have 
amplitudes between x and x + dxis accordingly 

-n^—\^'^^""^ W- 

V(27m) ^ 

The mean intensity is expressed by 
1 /■+* 
as before. 

We will now pass on to the more important problem in which 
the phases of the n unit vibrations are distributed at random over 
the entire period. In each combination the resultant amplitude 
is denoted by r and the phase (referred to a given epoch) by 6 ; 
and rectangular coordinates are taken so that 
4? = r cos Q, y = ^ sin Q, 
Thus any point (a?, y) in the plane of reference represents a 
vibration of amplitude r and phase d, and the whole system of 
N vibrations is represented by a distribution of points, whose 
density it is our object to determine. Since no particular phase 
can be singled out for distinction, we know beforehand that the 
density of distribution will be independent of Q. 
Of the infinite number N of points we suppose that 
^/K ^, y) dxdy 
are to be found within the infinitesimal area dxdy, and we will 
inquire as before how this number would be changed by the 
addition to the n component vibrations of one more unit vibration 
of accidental phase. Any vibration which after the addition is 
represented by the point a?, y must before have corresponded to 
the point 

fl?' = a? — cos <^, y'ssy — sin<^, 

where ^ represents the phase of the additional unit vibration. 
And, if for the moment ^ be regarded as given, to the area dxdy 
corresponds an equal area dafdy. Again, all values of ^ being 
equally probable, the factor necessary under this head is d<t>/2'n: 
Accordingly the whole number to be found in dxdy after the 
superposition of the additional unit is 

Ndxdypfin, x\ yO #/27r ; 

and this is to be equated to 

Ndxdyf{n + 1, x, y) ; 

/(n+1, x, rj)=.j^f{n, x\ y')d^\%ir (8). 



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The value of /(w, x, y) is obtained by introduction of the 
values of x\ y' and expansion : 

80 that 

Also, n being very great, 

/(n 4- 1, X, y) -f{n, x, y) « dfjdn ; 
and (8) reduces to 

dn" ^Kdx'^ df) ^"^^^ 

the usual equation for the conduction of heat in two dimensions. 

In addition to (9), /has to satisfy the special condition of 
evanescence when n = for all points other than the origin. The 
appropriate solution is necessarily symmetrical round the origin, 
and takes the form 

/(n, a?,y) = il7i-^e-'«'+i^/« (10), 

as may be verified by differentiation. The constant ul is to be 
determined by the condition that the whole number is N. Thus 


and the number of vibrations within the area dxdy becomes 

^ e-.^^l^'dxdy (11). 

If we wish to find the number of vibrations which have 
amplitudes between r and r + dr, we must introduce polar 
coordinates and integrate with respect to 0, The required number 

is thus 

2Nrr^e'-^l''rdr (12)^ 

The result may also be expressed by saying that the probability 
of a resultant amplitude between r and r'\-dr when a large 
number n of unit vibrations are compounded at random is 

2rr^e^l''rdr (13). 

1 PhiU Mag, Aug. 18S0. 

Digitized by VjOOQIC 

42 a.] 



The mean intensity is given by 

as was to be expected. 

The probability of a resultant amplitude less than r is 



e-^l^rdr = 1 - e-*"'" . 


or, which is the same thing, the probability of a resultant ampli- 
tude greater than r is 

c-^'/n (15). 

The following table gives the probabilities of intensities less 
than the fractions of n named in the first column. For example, 
the probability of intensity less than n is '6321. 



















' 300 


It will be seen that, however great n may be, there is a 
i-easonable chance of considerable relative fluctuations of intensity 
in different combinations. 

If the amplitude of each component be a, instead of unity, as 
we have hitherto supposed for brevity, the probability of a resultant 
amplitude between r and r + dr is 




The result is thus a function of n and a only through na", and 
would be unchanged if for example the amplitude became ^a and 
the number 4n. From this it follows that the law is not altered, 
even if the components have different amplitudes, provided always 
that the whole number of each kind is very great; so that if there 
be n components of amplitude a, nf of amplitude 0, and so on, the 
probability of a resultant between r and r + dr is 



wa' + n'^ + , 


That this is the case may perhaps be made more clear by the 

* consideration of a particular case. Let us suppose in the first 

place that n+4n^ unit vibrations are compounded at random. 

Digitized by 



The appropriate law is given at once by (13) on substitution of 
n + 4tn' for n, that is 

2(n + 4nO-'e-^''/<'»+*^Vdr (18). 

Now the combination of n-|-4n' unit vibrations may be re- 
garded as arrived at by combining a random combination of n 
unit vibrations with a second random combination of 4n' units, 
and the second random combination is the same as if due to a 
random combination of n' vibrations each of amplitude 2. Thus 
(18) applies equally well to a random combination of (n + ?i') 
vibrations, n of which are of amplitude unity and nf of ampli- 
tude 2. 

Although the result has no application to the theory of vibra- 
tions, it may be. worth notice that a similar method applies to the 
composition in three dimensions of unit vectors, whose directions 
are accidental. The equation analogous to (8) gives in place of 


dn Q\d3? df"^ dsi*)' 
The appropriate solution, analogous to (13), is 


e-rVfn^d^ (18)^ 

expressing the probability of a resultant amplitude Ijdng between 
r and r H- dr. 

Here again the mean value of r*, to be expected in a great 
number of independent combinations, is n. 

Digitized by 




43. The material systems, with whose vibrations Acoustics is 
concerned, are usually of considerable complication, and are sus- 
ceptible of very various modes of vibration, any or all of which 
may coexist at any particular moment. Indeed in some of the 
most important musical instruments, as strings and organ-pipes, 
the number of independent modes is theoretically infinite, and 
the consideration of several of them is*essential to the most prac- 
tical questions relating to the nature of the consonant chords. 
Cases, however, often present themselves, in which one mode is 
of paramount importance ; and even if this were not so, it would 
still be proper to commence the consideration of the general 
problem with the simplest case — that of one degree of freedom. 
It need not be supposed that the mode treated of is the only one 
possible, because so long as vibrations of other modes do not occur 
their possibility under other circumstances is of no moment. 

44. The condition of a system possessing one degree of free- 
dom is defined by the value of a single co-ordinate w, whose origin 
may be taken to correspond to the position of equilibrium. The 
kinetic and potential energies of the system for any given position 
are proportional respectively to ?i* and w* : — 

T = \mu\ F = i/AU« (1). 

where m and fi are in general functions of u. But if we limit 
ourselves to the consideration of positions in the immedidte neigh' 
hourhood of that corresponding to equilibrium, u is a small quantity, 
and m and fi are sensibly constant. On this understanding we 

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now proceed. If there be no forces, either resulting from internal 
friction or viscosity, or impressed on the system from without, the 
whole energy remains constant. Thus 

T+r= constant. 

Substituting for T and V their values, and diflferentiating with 
respect to the time, we obtain the equation of motion 

wtt + zii^sO (2) 

of which the complete integral is 

. w = acos(nt — a) (3), 

where ?i-=/A-*-m, representing a harmonic vibration. It will be 
seen that the period alone is determined by the nature of the 
system itself; the amplitude and phase depend on collateral cir- 
cumstances. If the differential equation were exact, that is to 
say, if T were strictly proportional to u\ and V to w", then, without 
any restriction, the vibrations of the system about its configuration 
of equilibrium would be accurately harmonic. But in the majority 
of cases the proportionality is only approximate, depending on an 
assumption that the displacement u is always small — ^how small 
depends on the nature of the particular system and the degree of 
approximation required ; and then of course we must be careful 
not to push the application of the integral beyond its proper 

But, although not to be stated without a limitation, the prin- 
ciple that the vibrations of a system about a configuration of 
equilibrium have a period depending on the structure of the 
system and not on the particular circumstances of the vibration, 
is of supreme importance, whether regarded from the theoretical 
or the practical side. If the pitch and the loudness of the note 
given by a musical instrument were not within wide limits in- 
dependent, the art of the performer on many instruments, such 
as the violin and pianoforte, would be revolutionized. 

The periodic time _ 

. = 2^ = 2^^ (4). 

so that an increase in m, or a decrease in /x, protracts the duration 
of a vibration. By a generalization of the language employed in 
ijie case of a material particle urged towards a position of equili- 
brium by a spring, m may be called the inertia of the system, and 

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ft the force of the equivalent spring. Thus an augmentation of 
mass, or a relaxation of spring, increases the periodic time. By 
means of this principle we may sometimes obtain limits for 
the value of a period, which cannot, or cannot easily, be calculated 

45. The absence of all forces of a frictional character is an 
ideal case, never realized but only approximated to in practice. 
The original energy of a vibration is always dissipated sooner or 
later by conversion into heat. But there is another source of loss, 
which though not, properly speaking, dissipative, yet produces 
results of much the same nature. Consider the case of a tuning- 
fork vibrating in vacuo. The internal friction will in time stop 
the motion, and the original energy will be transformed into 
heat. But now suppose that the fork is transferred to an open 
space. In strictness the fork and the air surrounding it consti- 
tute a single system, whose parts cannot be treated separately. 
In attempting, however, the exact solution of so complicated a 
problem, we should generally be stopped by mathematical diffi- 
culties, and in any case an approximate solution would be de- 
sirable. The effect of the air during a few periods is quite insig- 
nificant, and becomes important only by accumulation. We are 
thus led to consider its effect as a disturbance of the motion which 
would take place in vacuo. The disturbing force is periodic (to 
the same approximation that the vibrations are so), and may be 
divided into two parts, one proportional to the acceleration, and 
the other to the velocity. The former produces the same effect as 
an alteration in the mass of the fork, and we have nothing more 
to do with it at present. The latter is a force arithmetically pro- 
portional to the velocity, and always acts in opposition to the 
motion, and therefore produces effects of the same character as 
those due to friction. In many similar cases the loss of motion 
by communication may be treated under the same head as that 
due to dissipation proper, and is represented in the differential 
equation with a degree of approximation sufficient for acoustical 
purposes by a term proportional to the velocity. Thus 

tt + /cti + n*u = (1) 

is the equation of vibration for a system with one degree of 
freedom subject to frictional forces. The solution is 

u = ile-***cos{Vw^- J/c> . t-a] (2). 

Digitized by 



If the friction be so great that \/^ > n^ the solution changes its 
form, and no longer corresponds to an oscillatory motion ; but in 
all acoustical applications /e is a small quantity. Under these 
circumstances (2) may be regarded as expressing a harmonic 
vibration, whose amplitude is not constant, but diminishes in 
geometrical progression, when considered after equal intervals of 
time. The difference of the logarithms of successive extreme 
excursions is nearly constant, and is called the Logarithmic Decre- 
ment. It is expressed by \tcT, if t be the periodic time. 

The frequency, depending on n' — \/c\ involves only the second 
power o( k; so that to the first order of approximation the friction 
has no effect on the peiHod, — a principle of very general application. 

The vibration here considered is called the free vibration. It 
is that executed by the system, when disturbed from equilibrium, 
and then left to itself 

46. We must now turn our attention to another problem, not 
less important, — the behaviour of the system, when subjected to an 
external force varying as a harmonic function of the time. In 
order to save repetition, we may take at once the more general 
case including friction. If there be no friction, we have only to 
put in our results k = 0. The differential equation is 

w+/«i + 7i*a= Ecospt (1). 

Assume u = aco&(pt—€) (2), 

and substitute : 

a (n' — p') cos (p^ — e) — xpa sin (pt — e) 

= ^cos € cos (p^ - e) - ^sin € sin {pt — e) ; 
whence, on equating coefiicients of cos (pt — e), sin (pt — e), 

a(n«-p») = ^cos€| 

a.pK = Esm€} ^"^^^ 

so that the solution may be written 

-ffsine / ^ V 
w=~^<5os(p^-€) (4), 

where tan€= - - — , (5). 

71* — p* ^ ^ 

This is called sl forced vibration; it is the response of the system 
to a force imposed upon it from without, and is maintained by the 
continued operation of that force. The amplitude is proportional 

Digitized by 



to E — the magnitude of the force, and the period is the same 
as that of the force. 

Let us now suppose E given, and trace the effect on a given 
system of a variation in the period of the force. The effects 
produced in different cases are not strictly similar; because the 
frequency of the vibrations produced is always the same as that of 
the force, and therefore variable in the comparison which we are 
about to institute. We may, however, compare the energy of the 
system in different cases at the moment of passing through the 
position of equilibrium. It is necessary thus to specify the moment 
at which the energy is to be computed in each case, because the 
total energy is not invariable throughout the vibration. During 
one part of the period the system receives energy from the 
impressed force, and during the remainder of the period yields it 
back again. 

From(4), ifu = 0, 

energy oz u^ oc sin' e, 

and is therefore a maximum, when sin e = 1, or, from (5),p = n. If 
the maximum kinetic energy be denoted by T^, we have 

2'=rosin»e (6). 

The kinetic energy of the motion is therefore the greatest possible, 
when the period of the force is that in which the system would 
vibrate freely under the influence of its own elasticity (or other 
internal forces), ttnthout friction. The vibration is then by (4) 
and (5), 


u = — sin nt ; 


and, if k be small, its amplitude is very great. Its phase is a 
quarter of a period behind that of the force. 

The case, where p = n, may also be treated independently. 
Since the period of the actual vibration is the same as that 
natural to the system, 

u + nhL = 0, 

so that the differential equation (1) reduces to 

whence by integration 

u^ - \ co^pt dt== — smpt, 
as before. 

Digitized by 



If p be less than n, the retardation of phase relatively to the 
force lies between zero and a quarter period, and when p is greater 
than n, between a quarter period and a half period. 

In the case of a system devoid of friction, the solution is 

U=-- ^C08 pt (7). 

When p is smaller than n, the phase of the vibration agrees with 
that of the force, but when p is the greater, the sign of the vibra- 
tion is changed. The change of phase from complete agreement 
to complete disagreement, which is gradual when friction acts, 
here takes place abruptly as p passes through the value n. At the 
same time the expression for the amplitude becomes infinite. Of 
course this only means that, in the case of equal periods, friction 
must be taken into account, however small it may be, and however 
insignificant its result when p and n are not approximately equal. 
The limitation as to the magnitude of the vibration, to which we 
are all along subject, must also be borne in mind. 

That the excursion should be at its maximum in one direction 
while the generating force is at its maximum in the opposite 
direction, as happens, for example, in the canal theory of the tides, 
is sometimes considered a paradox. Any difficulty that may be 
felt will be removed by considering the extreme case, in which the 
** spring " vanishes, so that the natural period is infinitely long. In 
fact we need only consider tha force acting on the bob of a com- 
mon pendulum swinging freely, in which case the excursion on one 
side is greatest when the action of gravity is at its maximum 
in the opposite direction. When on the other hand the inertia of 
the system is very small, we have the other extreme case in which 
the so-called equilibrium theory becomes applicable, the force and 
excursion being in the same phase. 

When the period of the force is longer than the natural period, 
the effect of an increasing friction is to introduce a retardation 
in the phase of the displacement varying from zero up to a quarter 
period. If, however, the period of the natural vibration be the 
longer, the original retardation of half a period is diminished by 
something short of a quarter period ; or the effect of friction is to 
accelerate the phase of the displacement estimateii from that corre- 
sponding to the absence of friction. In either case the influence 
of friction is to cause an approximation to the state of things that 
would prevail if friction were paramount. 

Digitized by 



If a force of nearly equal period with the fi^e vibrations 
vary slowly to a maximum and then slowly decrease, the dis- 
placement does not reach its maximum until after the force has 
begun to diminish. Under the operation of the force at its 
maximum, the vibration continues to increase until a certain limit 
is approached, and this increase continues for a time even although 
the force, having passed its maximum, begins to diminish. On 
this principle the retardation of spring tides behind the days of 
new and full moon has been explained*. 

47. From the linearity of the equations it follows that the 
motion resulting from the simultaneous action of any number of 
forces is the simple sum of the motions due to the forces taken 
separately. Each force causes the vibration proper to itself, 
without regard to the presence or absence of any others. The 
peculiarities of a force are thus in a manner transmitted into the 
motion of the system. For example, if the force be periodic in 
time T, so will be the resulting vibration. Each harmonic element 
of the force will call forth a corresponding harmonic vibration 
in the system. But since the retardation of phase e, and the ratio 
of amplitudes a: E,ia not the same for the different components, 
the resulting vibration, though periodic in the same time, is dif- 
ferent in character from the force. It may happen, for instance, 
that one of the components is isochronous, or nearly so, with the 
free vibration, in which case it will manifest itself in the motion 
out of all proportion to its original importance. As another 
example we may consider the case of a system acted on by two 
forces of nearly equal period. The resulting vibration, being 
compounded of two nearly in unison, is intermittent, according to 
the principles explained in the last chapter. 

To the motions, which are the immediate effects of the im- 
pressed forces, must always be added the term expressing free 
vibrations, if it be desired to obtain the most general solution. 
Thus in the case of one impressed force, 

u^^^co&(pt^€) + Ae-^(^{'^7^^J?.t-a] (1), ' 

where A and a are arbitrary. 

48. The distinction between /orced and free vibrations is very 
important, and must be clearly understood. The period of the 

1 Airy'B Tide$ and Waves, Art. S2S. 
K. 4 

Digitized by VjOOQIC 


former is determined solely by the force which is supposed to act 
on the system from without ; while that of the latter depends only 
on the constitution of the system itself. Another point of differ- 
ence is that 6o long as the external influence continues to operate, 
a forced vibration is permanent, being represented strictly by a 
harmonic function ; but a free vibration gradually dies away, be- 
coming negligible after a time. Suppose, for example, that the 
system is at rest when the force E cos pt begins to operate. Such 
finite values must be given to the constants A and a in (1) of § 47, 
that both u and u are initially zero. At first then there is a 
free vibration not less important than its rival, but after a time 
friction reduces it to insignificance, and the forced vibration is left 
in complete possession of the field. This condition of things will 
continue so long as the force operatea When the force is removed, 
there is, of course, no discontinuity in the values of u or i, but 
the forced vibration is at once converted into a firee vibration, 
and the period of the force is exchanged for that natural to the 

During the coexistence of the two vibrations in the earlier part 
of the motion, the curious phenomenon of beats may occur, in 
case the two periods differ but slightly. For, n and p being nearly 
equal, and k small, the initial conditions are approximately satis- 
fied by 

w = a cos (p^ — €) — ae~i*^ cos {Vn* — ^/c* . ^ — c}. 
There is thus a rise and fall in the motion, so long as e"**^ remains 
sensible. This intermittence is very conspicuous in the earlier 
stages of the motion of forks driven by electro-magnetism (§ 63), 
[and may be utilized when it is desired to adjust n and p to 
equality. The initial beats are to be made slower and slower, 
until they cease to be perceptible. The vibration then swells 
continuously to a maximum.] 

49. Vibrating systems of one degree of freedom may vary in 
two ways according to the values of the constants n and /e. The 
distinction of pitch is sufficiently intelligible ; but it is worth while 
to examine more closely the consequences of a greater or less 
degree of damping. The most obvious is the more or less rapid 
extinction of a free vibration. The effect in this direction may be 
measured by the number of vibrations which must elapse before 
the amplitude is reduced in a given ratio. Initially the amplitude 
may be taken as unity ; after a time t, let it be 6. Initially = e^K 

Digitized by 




If ^ = a?T, we have a? = log 0, In a system subject to only a 


moderate degree of damping, we may take approximately, 

80 that a? = log^ (1). 


This gives the number of vibrations which are performed, before 
the amplitude falls to 0, 

The influence of damping is also powerfully felt in a forced 
vibration, when there is a near approach to isochronism. In the 
case of an exact equality between p and n, it is the damping alone 
which prevents the motion becoming infinite. We might easily 
anticipate that when the damping is small, a comparatively slight 
deviation from perfect isochronism would cause a large &lling off 
in the magnitude of the vibration, but that with a larger damping 
the same precision of adjustment would not be required. From 
the equations 

r=rosin»€, tan€ = -^, 
w — jr 

^eget __ir = ^__^ (2); 

SO that if /c be small, p must be very nearly equal to n, in order to 
produce a motion not greatly less than the maximum. 

The two principal effects of damping may be compared by 
eliminating /c between (1) and (2). The result is 

-x-'"'\n p)\/t;^:t ^^>' 

where the sign of the square root must be so chosen as to make 
the rigl}t-hand side negative. 

If, when a system vibrates freely, the amplitude be reduced in 
the ratio after x vibrations ; then, when it is acted on by a force 
{p\ the energy of the resulting motion will be less than in the 
case of perfect isochronism in the ratio T i T^, It is a matter of 
indifference whether the forced or the free vibration be the higher; 
all depends on the interval. 

In most cases of interest the interval is small; and then, putting 
p s n + Sn, the formula may be written. 

l9g^_29rSw / T 
X n V T,'T ^*^- 


Digitized by VjOOQIC 




The following table calculated from these formulsB has been 
given by HelmholtzM 

T X 1 J* X J ^' I Number of Tibrations after which the 

Interval oorresponding to a redaotioii ' *^ ***""« 

of the resonance to one-tenth. 


daced to one-tenth. 

1^ tone. 


J tone. 


^ tone. 


f tone. 


Whole tone. 


1^ tone. 


f tone = minor third. 


J tone. 


Two whole tones = major third. 


Formula (4) shews that, when Sn is small, it varies ccsteris 
paribus as -. 

60. From observations of forced vibrations due to known 
forces, the natural period and damping of a system may be deter- 
mined. The formulse are 


w = 


-cos(pf — e), 


tan€ = -r^.. 

On the equilibrium theory we should have 

U = -iCO&pt 

The ratio of the actual amplitude to this is 

^sin€ -£?_n*sin€ 
pK ' n^" pK ' 

If the equilibrium theory be known, the comparison of ampli- 
tudes tells us the value of , say 

px ^ 


= a, 

Tonemj)/S7u2tmj7«n, 8rd edition, p. 221. 

Digitized by 



and € is also known, whence 

, . /^ C08€\ J ©sine .-. 

n* = i)»-5- 1 ), and k--^ (1). 

'^ \ a J a — co8€ ^ ^ 

51. As has been already stated, the distinction of forced and 
free vibrations is important ; but it may be remarked that most of 
the forced vibrations which we shall have to consider as affecting 
a system, take their origin ultimately in the motion of a second 
system, which influences the first, and is influenced by it. A 
vibration may thus have to be reckoned as forced in its relation 
to a system whose limits are fixed arbitrarily, even when that 
system has a share in determining the period of the force which 
acts upon it. On a wider view of the matter embracing both the 
systems, the vibration in question will be recognized as free. An 
example may make this clearer. A tuning-fork vibrating in air 
is part of a compound system including the air and itself, and 
in respect of this compound system the vibration is free. But 
although the fork is influenced by the reaction of the air, yet the 
amount of such influence is small. For practical purposes it is 
convenient to consider the motion of the fork as given, and that of 
the air as forced. No error will be committed if the actual motion 
of the fork (as influenced by its surroundings) be taken as the 
basis of calculation. But the peculiar advantage of this mode of 
conception is manifested in the case of an approximate solution 
being required. It may then suffice to substitute for the actual 
motion, what would be the motion of the fork in the absence of 
air, and afterwards introduce a correction, if necessary. 

52. Illustrations of the principles of this chapter may be 
drawn from all parts of Acoustics. We will give here a few 
applications which deserve an early place on account of their 
simplicity or importance. 

A string or wire ACB is stretched between two fixed points 
A and £, and at its centre carries a mass M, which is supposed to 
be so considerable as to render the mass of the string itself negli- 
gible. When M is pulled aside firom its position of equilibrium, 
and then let go, it executes along the line CM vibrations, which 
are the subject of inquiry. AC^ CB = a. CM = x. The tension 
of the string in the position of equilibrium depends on the amount 
of the stretching to which it has been subjected. In any other 

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position the tension is greater ; but we limit ourselves to the case 
of vibrations so small that the additional stretching is a negligible 
fraction of the whole. On this condition the tension may be 
treated as constant. We denote it by T. 


Thus, kinetic energy « J-Jfo", 


potential energy = 2T { va' + ic* - a} = T -- approximately. 

The equation of motion (which may be derived also inde- 
pendently) is therefore 



from which we infer that the mass M executes harmonic vibra- 
tions, whose period 

^ = 2--V^ (2). 

The amplitude and phase depend of course on the initial cir- 
cumstances, being arbitrary so £BLr as the differential equation is 

Equation (2) expresses the manner in which r varies with each 
of the independent quantities T, M,a: results which may all be 
obtained by consideration of the dimensions (in the technical sense) 
of the quantities involved. The argument from dimensions is so 
often of importance in Acoustics that it may be well to consider 
this first instance at length. 

In the first place we must assure ourselves that of all the 
quantities on which t may depend, the only ones involving a 

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reference to the three fimdamental units— of length, time, and 
mass — are a, M, and T. Let the solution of the problem be 

T=f{fl,M,T) (3). 

This equation must retain its form unchanged, whatever may 
be the fundamental units by means of which the four quantities 
are numerically expressed, as is evident, when it is considered 
that in deriving it no assumptions would be made as to the mag- 
nitudes of those* units. Now of all the quantities on which/' 
depends, T is the only one involving time ; and since its dimen- 
sions are (Mass) (Length) (Time)"*, it follows that when a and M 
are constant, tx T"^; otherwise a change in the unit of time 
would necessarily disturb the equation (3). This being admitted, 
it is easy to see that in order that (3) may be independent of the 
unit of lengtl)^ we must have t x T""* . a*, when M is constant ; and 
finally, in order to secure independence of the unit of mass, 


To determine these indices we might proceed thus : — assume 


then by considering the dimensions in time, space, and mass, we 
obtain respectively 

l = -2a?, = a? + ;8f, = a? + y, 

whence as above ^ = — i, y = i, -s^ = i- 

There must be no mistake as to what this argument does and 
does not prove. We have asmmed that there is a definite 
periodic time depending on no other quantities, having dimen- 
sions in space, time, and mass, than those above mentioned. For 
example, we have not proved that t is independent of the ampli- 
tude of vibration. That, so far as it is true at all, is a consequence 
of the linearity of the approximate differential equation. 

From the necessity of a complete enumeration of all the 
quantities on which the required result may depend, the method 
of dimensions is somewhat dangerous ; but when used with proper 
care it is unquestionably of great power and value. 

53. The solution of the present problem might be made the 
foundation of a method for the absolute measurement of pitch. 
The principal impediment to accuracy would probably be the 

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difficulty of making M sufficiently large in relation to the mass of 
the wire, without at the same time lowering the note too much in 
the musical scale. 






The wire may be stretched by a weight M' attached to its 
further end beyond a bridge or pulley at B. The periodic time 
would be calculated from 




The ratio of if' : Jf is given by the balance. If a be measured 
in feet, and g ~ 32*2, the periodic time is expressed in seconds. 

54 In an ordinary musical string the weight, instead of being 
concentrated in the centre, is uniformly distributed over its length. 
Nevertheless the present problem gives some idea of the nature of 
the gravest vibration of .such a string. Let us compare the two 
cases more closely, supposing the amplitudes of vibration the same 
at the middle point. 

no. II. 

When the uniform string is straight, at the moment of passing 
through the position of equilibrium, its different parts are ani- 
mated with a variable velocity, increasing from either end towards 

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the centre. If we attribute to the whole mass the velocity of the 
centre, it is evident that the kinetic energy will be considerably 
over-estimated. Again, at the moment of maximum excursion, 
the uniform string is more stretched than its substitute, which 
follows the straight courses AM, MB, and accordingly the poten- 
tial energy is diminished by the substitution. The concentration 
of the mass at the middle point at once increases the kinetic 
energy when a? = 0, and decreases the potential energy when i? = 0, 
and therefore, according to the principle explained in § 44, prolongs 
the periodic time. For a string then the period is less than that 
calculated from the formula of the last section, on the supposition 
that M denotes the mass of the string. It will afterwards appear 
that in order to obtain a correct result we should have to take 
instead of M only {ilir^)M. Of the factor 4/7r' by far the more 
important part, viz. ^, is due to the difference of the kinetic 

66. As another example of a system possessing practically but 
one degree of freedom, let us consider the vibration of a spring, one 
end of which is clamped in a vice or otherwise held fast, while the 
other carries a heavy mass; 

In strictness, this system like the last has 
an infinite number of independent modes of vi- C j 

bration; but, when the mass of the spring is ^'""^ 

relatively small, that vibration which is nearly 
independent of its inertia becomes so much the FiOi2. 
most important that the others may be ignored. 
Pushing this idea to its limit, we may regard the 
spring merely as the origin of a force urging the 
attached mass towards the position of equilibrium, 
and, if a certain point be not exceeded, in simple \^ 
proportion to the displacement. The result is a -^ 
harmonic vibration, with a period dependent on 
the stiffiiess of the spring and the mass of the 
load. ' :- 

66. In consequence of the oscillation of the centre of inertia, 
there is a constant tendency towards the communication of motion 
to the supports, to resist which adequately the latter must be 
very firm and massive. In order to obviate this inconvenience. 

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O Q 

two precisely similar springs and loads may be mounted on 

the same framework in a symmetrical manner. 

If the two loads perform vibrations of equal 

amplitude in such a manner that the motions 

are always opposite, or, as it may otherwise be 

expressed, with a phase-difference of half a 

period, the centre of inertia of the whole system 

remains at rest, and there is no tendency to set 

the framework into vibration. We shall see in a 

future chapter that this peculiar relation of phases 

will quickly establish itself, whatever may be the 

original disturbance. In fact, any part of the 

motion which does not conform to the condition 

of leaving the centre of inertia unmoved is soon 

extinguished by damping, unless indeed the 

supports of the system are more than usually 



67. As in our first example we found a rough illustration of 
the fundamental vibration of a musical string, so here with the 
spring and attached load we may compare a uniform slip, or bar, 
of elastic material, one end of which is securely fastened, such for 
instcmce as the tongue of a reed instrument. It is true of course 
that the mass is not concentrated at one end, but distributed 
over the whole length ; yet on account of the smallness of the 
motion near the point of support, the inertia of that part of 
the bar is of but little account. We infer that the fundamental 
vibration of a uniform rod cannot be very different in character 
from that which we have been considering. Of course for pur- 
poses requiring precise calculation, the two systems are suflSciently 
distinct; but where the object is to form clear ideas, precision may 
often be advantageously exchanged for simplicity. 

In the same spirit mt^ may regard the combination of two 
springs and loads shewn in Fig. 13 as a representation of a 
tuning-fork. The instrument, which has been much improved 
of late years, is indispensable to the acoustical investigator. On 
a large scale and for rough purposes it may be made by welding 
a cross piece on the middle of a bar of steel, so as to form a T, and 
then bending the bar into the shape of a horse-shoe. On the 
handle a screw should be cut. But for the better class of tuning- 
forks it is preferable to shape the whole out of one piece of steel. 

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57.] TUNING-FORKS. 59 

A division running from one end down the middle of a bar is first 
made, the two parts opened out to form the prongs of the fork, 
and the whole worked by the hammer and file into the required 
shape. The two prongs must be exactly symmetrical with respect 
to a plane passing through the axis of the handle, in order that 
during the vibration the centre of inertia may remain unmoved, 
— unmoved, that is, in the direction in which the prongs 

The tuning is effected thus. To make the note higher, the 
equivalent inertia of the system must be reduced. This is done 
by 'filing away the ends of the prongs, either diminishing their 
thickness, or actually shortening them. On the other hand, to 
lower the pitch, the substance of the prongs near the bend may 
be reduced, the effect of which is to diminish the force of the 
spring, leaving the inertia practically unchanged ; or the inertia 
may be increased (a method which would be preferable for 
temporary purposes) by loading the ends of the prongs with 
wax, or other material. Large forks are sometimes provided with 
moveable weights, which slide along the prongs, and can be fixed 
in any position by screws. As these approach the ends (where the 
velocity is greatest) the equivalent inertia of the system increases. 
In this way a considerable range of pitch may be obtained from 
one fork. The number of vibrations per second for any position 
of the weights may be marked on the prongs. 

The relation between the pitch and the size of tuning-forks is 
remarkably simple. In a future chapter it will be proved that, 
provided the material remains the same and the shape constant, 
the period of vibration varies directly as the linear dimension. 
Thus, if the linear dimensions of a tuning-fork be doubled, its 
note falls an octave. 

68. The note of a tuning-fork is a nearly pure tone. Imme- 
diately after a fork is struck, high tones may indeed be heard, 
corresponding to modes of vibration, whose nature will be subse- 
quently considered ; but these rapidly die away, and even while 
they exist, they do not blend with the proper tone of the fork, 
partly on account of their very high pitch, and partly because 
they do not belong to its harmonic scale. In the forks examined 
by Helmholtz the first of these overtones had a frequency from 5*8 
to 6*6 times that of the proper tone. 

Tuning-forks are now generally supplied with resonance cases. 

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whose effect is greatly to augment the volume and purity of the 
sound, according to principles to be hereafter developed Id 
order to excite them, a violin or cello bow, well supplied with 
rosin, is drawn across the prongs in the direction of vibration. 
The sound so produced will last a minute or more. 

69. As standards of pitch tuning-forks are invaluable. The 
pitch of organ-pipes rapidly varies with the temperature and with 
the pressure of the wind ; that of strings with the tension, which 
can never be retained constant for long; but a tuning-fork kept 
clean and not subjected to violent changes of temperature or 
magnetization, preservers its pitch with great fidelity. 

[But it must not be supposed that the vibrations of a fork are 
altogether independent of temperature. According to the obser- 
vations of McLeod and Clarke^ the frequency falls by *00011 of its 
value for each degree Cent, of elevation.] 

By means of beats a standard tuning-fork may be copied with 
very great precision. The number of beats heard in a second is 
the difference of the frequencies of the two tones which produce 
them ; so that if the beats can be made so slow as to occupy half 
a minute each, the frequencies differ by only l-30th of a vibra- 
tion. Still greater precision might be obtained by Lissajous' 
optical method. 

Very slow beats being difficult of observation, in consequence 
of the uncertainty whether a falling off in the sound is due to 
interference or to the gradual dying away of the vibrations, 
Scheibler adopted a somewhat modified plan. He took a fork 
slightly different in pitch from the standard — whether higher or 
lower is not material, but we will say, lower, — and counted the 
number of beats, when they were sounded together. About four 
beats a second is the most suitable, and these may be counted for 
perhaps a minute. The fork to be adjusted is then made slightly 
higher than the auxiliary fork, and tuned to give with it precisely 
the same number of beats, as did the standard. In this way a 
copy as exact as possible is secured. To facilitate the counting 
of the beats Scheibler employed pendulums, whose periods of 
vibration could be adjusted. 

[The question between slow and quick beats depends upon the 
circumstances of the case. It seems to be sometimes supposed 
that quick beats have the advantage as admitting of greater 

1 Phil Tram. 18S0, p. 12. 

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59.] scheibler's tonometer. 61 

relative accuracy of counting. But a little consideration shews 
that in a comparison of frequencies we are concerned not with the 
relative, but with the abaolvte accuracy of the counting. If we 
miscount the beats in a minute by one, it makes just the same 
error in the result, whether the whole number of beats be 60 or 

When the sounds are pure tones and are well maintained, it is 
advisable to use beats much slower than four per second. By 
choosing a suitable position it is often possible to make the 
intensities at the ear equal; and then the phase of silence, 
corresponding to antagonism of equal and opposite vibrations, is 
extremely well marked. Taking advantage of this we may deter- 
mine slow beats with very great accuracy by observing the time 
which elapses between recuiTences of silence. In favourable cases 
the whole number of beats in the period of observation may be 
fixed to within one-tenth or one-twentieth of a single beat, a 
degree of accuracy which is out of the question when the beats 
are quick. In this way beats of periods exceeding 30 seconds may 
be utilised with excellent effect ^] 

60. The method of beats was also employed by Scheibler to 
determine the absolute pitch of his standards. Two forks were 
tuned to an octave, and a number of others prepared to bridge 
over the interval by steps so small that each fork gave with its 
immediate neighbours in the series a number of beats that could 
be easily counted. The difference of frequency corresponding to 
each step was observed with all possible accuracy. Their sum, 
being the difference of frequencies for the interval of the octave, 
was equal to the frequency of that fork which formed the starting 
point at the bottom of the series. The pitch of the other forks 
could be deduced. 

If consecutive forks give four beats per second, 65 in all will 
be required to bridge over the interval from c' (256) to c" (512). 
On this account the method is laborious ; but it is probably the 
most accurate for the original determination of pitch, as it is 
liable to no errors but such as care and repetition will eliminate. 
It may be observed that the essential thing is the measurement 
of the difference of frequencies for two notes, whose ratio of 
frequencies is independently known. If we could be sure of its 
accuracy, the interval of the fifth, fourth, or even major third, might 

^ Aooustical Observations, Phil. Mag, May, 1882, p. 342. 

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be substituted for the octave, with the advantage of reducing the 
number of the necessary interpolations. It is probable that with 
the aid of optical methods this course might be successfully 
adopted, as the corresponding Lissajous' figures are easily recog- 
nised, and their steadiness is a very severe test of the accuracy 
with which the ratio is attained. 

[It is essential to the success of this method that the pitch of 
each of the numerous sounds employed should be definite, and in 
particular that the vibrations of any fork should take place at the 
same rate whether that fork be sounding in conjunction with its 
neighbour above or with its neighbour below. There is no reason 
to doubt that this condition is sufficiently satisfied in the case of 
independent tuning-forks; but an attempt to replace forks by a 
set of reeds, mounted side by side on a common wind-chest, has 
led to error, owing to a disturbance of pitch by mutual inter- 
action \] 

The frequency of large tuning-forks may be determined by 
allowing them to trace a harmonic curve on smoked paper, which 
may conveniently be mounted on the circumference of a revolving 
drum. The number of waves executed in a second of time gives 
the frequency. 

In many cases the use of intermittent illumination described 
in § 42 gives a convenient method of determining an unknown 

61. A series of forks ranging at small intervals over an octave 
is very useful for the determination of the frequency of any 
musical note, and is called Scheibler's Tonometer. It may also 
be used for tuning a note to any desired pitch. In either case 
the frequency of the note is determined by the number of beats 
which it gives with the forks, which lie nearest to it (on each 
side) in pitch. 

For tuning pianofortes or organs, a set of twelve forks may be 
used giving the notes of the chromatic scale on the equal tempe- 
rament, or any desired system. The corresponding notes are 
adjusted to unison, and the others tuned by octaves. It is better, 
however, to prepare the forks so as to give four vibrations per 
second less than is above proposed. Each note is then tuned a 
little higher than the corresponding fork, until they give when 
sounded together exactly four beats in the second. It will be 

1 Nature, xyii. pp. 12. 26 ; 1877. 

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61. J scheibler's tonometer. 63 

observed that the addition (or subtraction) of a constant number 
to the frequencies is not the same thing as a mere displacement 
of the scale in absolute pitch. 

In the ordinary practice of tuners a! is taken from a fork, and 
the other notes determined by estimation of fifths. It will be 
remembered that twelve true fifths are slightly in excess of seven 
octaves, so that on the equal temperament system each fifth is a 
little flat. The tuner proceeds upwards from ol by successive 
fifths, coming down an octave after about every alternate step, in 
order to remain in nearly the same part of the scale. Twelve 
fifths should bring him back to a. If this be not the case, the 
work must be readjusted, until all the twelve fifths are too flat by, 
as nearly as can be judged, the same small amount. The in- 
evitable error is then impartially distributed, and rendered as little 
sensible as possible. The octaves, of course, are all tuned true. 
The following numbers indicate the order in which the notes may 
be taken : 

a% b c' c'jf d' d't e' fft g' g't a' a'i V c" c"jt d" d't e" 
13 5 16 8 19 11 3 14 6 17 9 1 12 4 15 7 18 10 2 

In practice the equal temperament is only approximately 
attained; but this is perhaps not of much consequence, considering 
that the system aimed at is itself by no means perfection. 

Violins and other instruments of that class are tuned by true 
fifths from a\ 

62. In illustration of forced vibration let us consider the case 
of a pendulum whose point of support is subject to a small hori- 
zontal harmonic motion. Q is the bob attached by a fine More to 

a moveable point P. OP^x^. g_ 

PQ ss Z, and x is the horizontal 
co-ordinate of Q. Since the 
vibrations are supposed small, 
the vertical motion may be 
neglected, and the tension of 
the wire equated to the weight 
of Q. Hence for the horizontal 

motion * + #«c + y (a? — a?o) = 0. rtci4. 

Now iCp oc cos jp^ ; so that putting g-7-l^n\ our equation takes 
the form already treated of, viz. 

ai + ittP -h n"a? = E cos pt 

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I{ phe equal to n, the motion is limited only by the friction. 
The assumed horizontal harmonic motion for P may be realized by 
means of a second pendulum of massive construction, which carries 
P with it in its motion. An efficient arrangement is shewn ia 
the figure. A, B are iron rings screwed into a beam, or other firm 

Fl Qf6. 

support ; (7, B similar rings attached to a stout bar, which carries 
equal heavy weights E, Fy attached near its ends, and is supported 
in a horizontal position at right angles to the beam by a wire 
passing through the four rings in the manner shewn. When the 
pendulum is made to vibrate, a point in the rod midway between 
C and D executes a harmonic motion in a direction parallel to 
CD, and may be made the point of attachment of another pen- 
dulum PQ. If the weights E and F be very great in relation 
to Q, the upper pendulum swings very nearly in its own proper 
period, and induces in Q a forced vibration of the same period. 
When the length PQ is so adjusted that the natural periods of the 
two pendulums are nearly the same, Q will be thrown into violent 
motion, even though the vibration of P be of but inconsiderable 
amplitude. In this case the difference of phase is about a quarter 
of a period, by which amount the upper pendulum is in advance. 
If the two periods be very different, the vibrations either agree 
or are completely opposed in phase, according to equations (4) 
and (5) of § 46. 

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63. A very good example of a forced vibration is afforded by 
a fork under the influence of an intermittent electric cuirent, 

Fl C. /& 

c ^ '=r3 




whose period is nearly equal to its own. ACB is the fork ; E a 
small electro-magnet, formed by winding insulated wire on an iron 
core of the shape shewn in E (similar to that known as ' Siemens ' 
armature'), and supported between the prongs of the fork. When 
an intermittent current is sent through the wire, a periodic force 
acts upon the fork. This force is not expressible by a simple 
circular function ; but may be expanded by Fourier's theorem in a 
series of such functions, having periods t,\t^\ t, &c. If any of 
these, of not too small amplitude, be nearly isochronous with the 
fork, the latter will be caused to vibrate ; otherwise the effect is 
insignificant In what follows we will suppose that it is the 
complete period t which nearly agrees with that of the fork, and 
consequently regard the series expressing the periodic force as 
reduced to its first term. 

In order to obtain the maximum vibration, the fork must be 
carefully tuned by a small sliding piece or by wax, until its natural 
period (without friction) is equal to that of the force. This is best 
done by actual trial. When the desired equality is approached, 
and the fork is allowed to start from rest, the force and com- 
plementary free vibration are of nearly equal amplitudes and 
frequencies, and therefore (§ 48) in the beginning of the motion 
produce &eato, whose slowness is a measure of the accuracy of 
the adjustment. It is not until after the free vibration has had 
time to subside, that the motion assumes its permanent character. 
The vibrations of a tuning-fork properly constructed and mounted 
are subject to very little damping; consequently a very slight 
deviation from perfect isochronism occasions a marked falling off 
in the intensity of the resonance. 

The amplitude of the forced vibration can be observed with 
sufficient accuracy by the ear or eye; but the experimental 
R. 5 

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verification of the relations pointed out by theory between its 
phase and that of the force which causes it, requires a modified 

Two similar electro-magnets acting on similar forks, and in- 
cluded in the same circuit are excited by the same intermittent 
current. Under these circumstances it is clear that the systems 
will be thrown into similar vibrations, because they are acted on 
by equal forces. This similarity of vibrations refers both to phase 
and amplitude. Let us suppose now that the vibrations are 
effected in perpendicular directions, and by means of one of 
Lissajous' methods are optically compounded. The resulting figure 
is necessarily a straight line. Starting fi-om the case in which the 
amplitudes are a maximum, viz. when the natural periods of both 
forks are the same as that of the force, let one of them be put a 
little out of tune. It must be remembered that whatever their 
natural periods may be, the two forks vibrate in perfect unison 
with the force, and therefore with one another. The principal 
effect of the difference of the natural periods is to destroy the 
synchronism of phase. The straight line, which previously re- 
presented the compound vibration, becomes an ellipse, and this 
remains perfectly steady, so long as the forks are not touched. 
Originally the forks are both a quarter period behind the force. 
When the pitch of one is slightly lowered, it falls still more behind 
the force, and at the same time its amplitude diminishes. Let the 
difference of phase between the two forks be e', and the ratio of 
amplitudes of vibration a : a©. Then by (6) of § 46 

a =« a© cos c'. 

The following table shews the simultaneous values of a : a^ 
and €\ 

a : ao ' €' 



25» 50' 


36» 52' 




53» 7' 




66» 25' 




780 27' 


84» 15'> 

Tonempfiudungen, 3rd edition, p. 190. 

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It appears that a considerable alteration of phase in either 
direction may be obtained without very materially reducing the 
amplitude. When one fork is vibrating at its maximum, the 
other may be made to differ from it on either side by as much as 
60* in phase, without losing more than half its amplitude, or by 
as much as 45^ without losing more than half its energy. By 
allowing one fork to vibrate 45® in advance, and the other 45° 
in arrear of the phase corresponding to the case of maximum 
resonance, we obtain a phase difference of 90® in conjunction with 
an equality of amplitudes. Lissajous' figure then becomes a circle. 
[An intermittent electric current may also be applied to 
regulate the speed of a revolving body. The phonic wheel, in- 
vented independently by M. La Cour and by the author of this 
work^ is of great service in acoustical investigations. It may take 
various forms; but the essential feature is the approximate 
closing of the magnetic circuit of an electro-magnet, fed with an 
intermittent current, by one or more soft iron armatures carried 
by the wheel and disposed symmetrically round the circumference. 
If in the revolution of the wheel the closest passage of the 
armature sjmchronises with the middle of the time of excitation, 
the electro-magnetic forces operating upon the armature during 
its advance and its retreat balance one another. If however the 
wheel be a little in arrear, the forces promoting adv8mce gain an 
advantage over those hindering the retreat of the armature, and 
thus upon the whole the magnetic forces encourage the rotation. 
In like manner if the phase of the wheel be in advance of that 
first specified, forces are called into play which retard the motion. 
By a self-acting adjustment the rotation settles down into such 
a phase that the driving forces exactly balance the resistances. 
When the wheel runs lightly, and the electric appliances are 
moderately powerful, independent driving may not be needed. In 
this case of course the phase of closest passage must follow that 
which marks the middle of the time of magnetisation. If, as is 
sometimes advisable, there be an independent driving power, the 
phase of closest passage may either precede or follow that of 

In some cases the oscillations of the motion about the phase 

into which it should settle down are very persistent and interfere 

with the applications of the instrument. A remedy may be 

found in a ring containing water or mercury, revolving concen- 

1 Nature, May 23, 1878. 


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trically. When the rotation is uniform, the fluid revolves like a 
solid body and then exercises no influence. But when from any 
cause the speed changes, the fluid persists for a time in the former 
motion, and thus brings into play forces tending to damp out 

64. The intermittent current is best obtained by a fork- 
interrupter invented by Helmholtz. This may consist of a fork 
and electro-magnet mounted as before. The wires of the magnet 
are connected, one with one pole of the battery, and the other with 
a mercury cup. The other pole of the battery is connected with 
a second mercury cup. A U-shaped rider of insulated mre is 
carried by the lower prong just over the cups, at such a height 
that during the vibration the circuit is alternately made and 
broken by the passage of one end into and out of the mercury. 
The other end may be kept permanently immersed. By means 
of the periodic force thus obtained, the eflTect of friction is com- 
pensated, and the vibrations of the fork permanently maintained. 
In order to set another fork into forced vibration, its associated 
electro-magnet may be included, either in the same driving-circuit, 
or in a second, whose periodic interruption is effected by another 
rider dipping into mercury cups\ 

The modus operandi of this kind of self-acting instrument is 
often imperfectly apprehended. If the force acting on the fork 
depended only on its position — on whether the circuit were open 
or closed — the work done in passing through any position would 
be undone on the return, so that after a complete period there 
would be nothing outstanding by which the effect of the frictional 
forces could be compensated. Any explanation which does not 
take account of the retardation of the current is wholly beside the 
mark. The causes of retardation are two : irregular contact, and 
self-induction. When the point of the rider first touches the 
mercury, the electric contact is imperfect, probably on account of 

^ I have arranged Beveral interrupters on the above plan, all the component 
parts being of home manufacture. The forks were made by the village blacksmith. 
The onps consisted of iron thimbles, soldered on one end of copper slips, the 
further end being screwed down on the base board of the instrument. Some 
means of adjusting the level of the mercury surface is necessary. In Helmholtz* 
interrupter a horse-shoe electro-magnet embracing the fork is adopted, but I am 
inclined to prefer the present arrangement, at any rate if the pitch be low. In 
some cases a greater motive power is obtained by a horse-shoe magnet acting on a 
soft iron armature carried horizontally by the upper prong and perpendicular to it. 
I have usually found a single Smee cell sufficient battery power. 

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adhering air. On the other hand, in leaving the mercury the 
contact is prolonged by the adhesion of the liquid in the cup to 
the amalgamated wire. On both accounts the current is retarded 
behind what would correspond to the mere position of the fork. 
But, even if the resistance of the circuit depended only on the 
position of the fork, the current would still be retarded by its self- 
induction. However perfect the contact may be, a finite current 
cannot be generated until after the lapse of a finite time, any 
more than in ordinary mechanics a finite velocity can be suddenly 
impressed on an inert body. From whatever causes ari8ing\ the 
effect of the retardation is that more work is gained by the fork 
during the retreat of the rider from the mercury, than is lost 
during its entrance, and thus a balance remains to be set off 
against friction. 

If the magnetic force depended only on the position of the fork, 
the phase of its first harmonic component might be considered to 
be 180* in advance of that of the fork's own vibration. The re- 
tardation spoken of reduces this advance. If the phase-difference 
be reduced to 90^, the force acts in the most favourable manner, 
and the greatest possible vibration is produced. 

It is important to notice that (except in the case just refeired 
to) the actual pitch of the interrupter differs to some extent from 
that natural to the fork according to the law expressed in (5) of 
§ 46, € being in the present case a prescribed phase-difference 
depending on the nature of the contacts and the magnitude of the 
self-induction. If the intermittent current be employed to drive 
a second fork, the maximum vibration is obtained, when the 
frequency of the fork coincides, not with the natural, but with the 
modified frequency of the iuterrupter. 

The deviation of a tuning-fork interrupter from its natural 
pitch is practically very small ; but the fact that such a deviation 
is possible, is at first sight rather surprising. The explanation (in 
the case of a small retardation of current) is, that during that half 
of the motion in which the prongs are the most separated, the 
electro-magnet acts in aid of the proper recovering power due to 
rigidity, and so naturally raises the pitch. Whatever the relation 
of phases may be, the force of the magnet may be divided into 

1 Any desired retardation might be obtained, in default of other means, by 
attaching the rider, not to the prong itself, bat to the farther end of a light 
straight spring carried by the prong and set into forced vibration by the motion of 
its point of attachment. 

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two parts respectively proportional to the velocity and displacement 
(or acceleration). To the first exclusively is due the sustaining 
power of the force, and to the second the alteration of pitch. 

66. The general phenomenon of resonance, though it cannot 
be exhaustively considered under the head of one degree of 
freedom, is in the main referable to the same general principles. 
When a forced vibration is excited in one part of a system, all 
the other parts are also influenced, a vibration of the same period 
being excited, whose amplitude depends on the constitution of the 
system considered as a whole. But it not unfrequently happens 
that interest centres on the vibration of an outlying part whose 
connection with the rest of the system is but loose. In such a case 
the part in question, provided a certain limit of amplitude be 
not exceeded, is very much in the position of a system possessing 
one degree of freedom and acted on by a force, which may be 
regarded as given, independently of the natural period. The 
vibration is accordingly governed by the laws we have already 
investigated. In the case of approximate equality of periods to 
which the name of resonance is generally restricted, the ampli- 
tude may be very considerable, even though in other cases it 
might be so small as to be of little account; and the precision 
required in the adjustment of the periods in order to bring out 
the effect, depends on the degree of damping to which the system 
is subjected. 

Among bodies which resound without an extreme precision of 
tuning, may be mentioned stretched membranes, and strings asso- 
ciated with sounding-boards, as in the pianoforte and the violin. 
When the proper note is sounded in their neighbourhood, these 
bodies are caused to vibrate in a very perceptible manner. The 
experiment may be made by singing into a pianoforte the note 
given by any of its strings, having first raised the corresponding 
damper. Or if one of the strings belonging to any note be plucked 
(like a harp string) with the finger, its fellows will be set into 
vibration, as may immediately be proved by stopping the first. 

The phenomenon of resonance is, however, most striking in 
cases where a very accurate equality of periods is necessary in 
order to elicit the full effect. Of this class tuning-forks, mounted 
on resonance boxes, are a conspicuous example. When the unison 
is perfect the vibration of one fork will be taken up by another 
across the width of a room, but the slightest deviation of pitch 

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is sufficient to render the phenomenon almost insensible. Forks 
of 256 vibrations per second are commonly used for the purpose, 
and it is found that a deviation from unison giving only one beat 
in a second makes all the difference. When the forks ai*e well 
tuned and close together, the vibration may be transferred back- 
wards and forwards between them several times, by damping them 
alternately, with a touch of the finger. 

Illustrations of the powerful effects of isochronism must be 
within the experience of every one. They are often of importance 
in very different fields from any with which acoustics is concerned. 
For example, few things are more dangerous to a ship than to lie 
in the trough of the sea under the influence of waves whose period 
is nearly that of its own natural rolling. 

65 a. It has already (§ 30) been explained how the super- 
position of two vibrations of equal amplitude and of nearly equal 
frequency gives rise to a resultant in which the sound rises and 
falls in beats. If we represent the two components by cos 27mit, 
cos 27r7i^, the resultant is 

2 008^(111— 71^)1, COS w(ni + n^)t (l)j 

and it may be regarded as a vibration of frequency ^ (ui + n^), and 
of amplitude 2 cos tt (rii - n,) t. In passing through zero the 
amplitude changes sign, which is equivalent to a change of phase 
of ISO"", if the amplitude be regarded as always positive. This 
change of phase is readily detected by measurement in drawings 
traced by machines for compounding vibrations, and it is a feature 
of great importance. If a force of this character act upon a system 
whose natural frequency is J (nj + n^), the effect produced is com- 
paratively small. If the system start from rest, the successive 
impulses cooperate at first, but after a time the later impulses 
begin to destroy the effect of former ones. The greatest response 
would be given to forces of frequency Ui and n,, and not to a force 
of frequency i (w^ -f n,). 

If, as in some experiments of Prof. A. M. Mayer \ an otherwise 
steady sound is rendered intermittent by the periodic interposition 
of an obstacle, a very different result is arrived at. In this case 
the phase is resumed after each silence without reversal. If a 
force of this character act upon an isochronous system, the effect 
is indeed less than if there were no intermittence ; but as all the 

* Phil. Mag. May, 1876. 

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impulses operate in the same sense without any antagonism, the 
response is powerful. One kind of intermittent vibration or force 

is represented by 

2(l + cos2'7rmOcos27m^ (2), 

in which n is the frequency of the vibration, and m the frequency 
of intermittence ^ The amplitude is here always positive, and 
varies between the values and 4. By ordinary trigonometrical 
transformation (2) may be put in the form 

2 cos 27rn^ + cos 27r (n + m) ^ + cos 27r(n — m) t (3): 

which shews that the intermittent vibration in question is equiva- 
lent to three simple vibrations of frequencies w, n + m, n — m. 
This is the explanation of the secondary sounds observed by 

The form (2) is of course only a particular case. Another in 
which the intensity of the intermittent sound rises more suddenly 
to its maximum is given by 

^cos^irmtco&iimt (4), 

which may be transformed into 

f COB iimt + cos 27r (n + m) ^ + cos 27r (n — wi) t 

+ icos27r(ri + 2m)^4-icos27r(n- 2m) t (5). 

There are here four secondary sounds, the frequencies of the 
two new ones differing twice as much as before fix)m that of the 
primary sound. 

The theory of intermittent vibrations is well illustrated by 
electrically driven forks. A fork interrupter of frequency 128 
gave a periodic current, by the passage of which through an 
electro-magnet a second fork of like pitch could be excited. The 
action of this current on the second fork could be rendered inter- 
mittent by short-circuiting the electro-magnet. This was effected 
by another interrupter of frequency 4, worked by an independent 
current from a Smee cell. To excite the main cuirent a Grove 
cell was employed. When the contact of the second interrupter 
was permanently broken, so that the main current passed con- 
tinuously through the electro-magnet, the fork was, of course, 
most powerfully affected when tuned to 128. Scarcely any 
response was observable when the pitch was changed to 124 or 
132. But if the second interrupter were allowed to operate, so as 

^ Cram Brown and Tait. Edin. Proe, June, 1S7S. Aooostioal Observations ii. 
Phil Mag. April. 18S0. 

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65 a.] 



to render the periodic current through the electro-magnet inter- 
mittent, then the fork would respond powerfully when tuned to 
124 or 132 as well as when tuned to 128, but not when tuned to 
intermediate pitches, such as 126 or 130. 

The operation of the intermittence in producing a sensitive- 
ness which would not otherwise exist, is easily understood. When 
a fork of frequency 124 starts from rest under the influence of a 
force of frequency 128, the impulses cooperate at first, but after J 
of a second the new impulses begin to oppose the earlier ones. 
After J of a second, another series of impulses begins whose effect 
agrees with that of the first, and so on. Thus if all these impulses 
are allowed to act, the resultant effect is trifling ; but if every 
alternate series is stopped off, a large vibration accumulates. 

Fig. 16 a. 

The most general expression for a vibration of frequency n, 
whose amplitude and phase are slowly variable with a frequency 
m, is 


{Ao-^Ai cos 2'7rmt 4- -4 a cos 47rm^ + A^ cos GTnrU + 
-f- Bi sin 27rmt -h J5, sin 47rwi^ -h B^ sin Qirmt 
f Co 4- Ci cos 27rm^ + Cj cos 4'7rm^ 4- C^ cos 6frmt 4- . . .) 
( -f- Asin 27rm^ 4 J5j sin 47rm^ +2), sin Qwrnt -f- . . . j 

cos 2Tmt 



and this applies both to the case of beats (e.g. if Ai only be finite) 
and to such intermittence as is produced by the interposition of 
an obstacle. The vibration in question is accordingly in all cases 
equivalent to a combination of simple vibrations of frequencies 
n, n + m, n — m, n + 2m, n — 2m, &c. 
It may be well here to emphasise that a simple vibration 
implies infinite continuance, and does not admit of variations of 
phase or amplitude. To suppose, as is sometimes done in optical 
speculations, that a train of simple waves may begin at a given 
epochs continue for a certain time involving it may be a large 
number of periods, and ultimately cease, is a contradiction in terms. 

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66. The solution of the equation for free vibration, viz. 

u4-#ci + n*a«0 (1). 

may be put into another form by expressing the arbitrary con- 
stants of integration A and a in terms of the initial values of u 
and u, which we may denote by Mo and lio- We obtain at once 

u = e"^^ juo ^^ -r- 4 Mo (cos n't + ^ sin n'n \ (2), 

where n' = V/i^ - \k\ 

If there be no friction, /c = 0, and then 

. sinn^ . . xQv 

t^ssUn h^ocosn^ (o). 


These results may be employed to obtain the solution of the 
complete equation 

u4-/«i + n2w= U (4), 

where CT is an explicit function of the time ; for from (2) we see 
that the eflTect at time ^ of a velocity tu communicated at time 

The effect of U is to generate in time dt' a velocity Udt\ whose 
result at time t will therefore be 

u= -, [7a«'e^«(«-«'»sinn'rt-n, 

and thus the solution of (4) will be 

M^^^fT^^^"^^ %vcLri {i^t')JJ di (5). 

If there be no friction, we have simply 

u = ^J*sinn(«-Of^d«' (6)* 

U being the force at time H. 

The lower limit of the integrals is so far arbitrary, but it will 
generally be convenient to make it zero. 

On this supposition u and u as given by (6) vanish, when 
^ = 0, and the complete solution is 

u = e-**^ jUo — 7— + Mo (cos nt + -^,smntj> 

+ i, fe-i^tt-e') sin n' (t - 1') Udt' (7), 

n Jo 

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or if there be no friction 

u = iio hiLoC08nt + - I smnit — tf) Udf (8). 

When t is sufficiently great, the complementary terms tend to 
vanish on account of the factor 6""**^ and may then be omitted. 

66 a. In § 66 we have limited the discussion to the case of 
greatest acoustical importance, that is, we have supposed that nf 
is real, as happens when n^ is positive, and /e not too great. But 
a more general treatment of the problem of free vibrations is not 
without interest. Whatever may be the values of n^ and /c, the 
solution of (1) § 66 may be expressed 

w = ^e'*»* + J5e'*«* (1), 

where /Ai, /i, are the roots of 

/i«4-/c/i + n» = (2). 

The case already discussed is that in which the values of fi are 
imaginary. The motion is then oscillatory, with amplitude which 
decreases if tc be positive, but increases if k be negative. 

But if n\ though positive, be less than J/r*, or if n* be negative, 
n' becomes imaginary, that is /i becomes real. The motion 
expressed by (1) is then non-oscillatory, and it depends upon the 
sign of fi whether it increases or diminishes with the time. From 
the solution of (2), viz. 

M = -i^±iV(«»~4n«) (3), 

it is evident that if w* be positive (and less than J/c*) the two 
values of fi are of the same sign, and that the sign is the opposite 
of that of K. Hence if /c be positive, both terms in (1) diminish 
with the time, so that the system, however disturbed, subsides 
again into a state of rest. If, on the contrary, k be negative, the 
motion increases without limit. ^ 

We have still to consider the case of n^ negative. The real 
values of fi are then of opposite signs. It is possible so to start 
the sjTStem from a displaced position that it shall approach asymp- 
totically the condition of rest in the configuration of equilibrium ; 
but unless a special relation between displacement and velocity is 
satisfied, the motion tends to increase without limit. Under these 
circumstances the equilibrium must be regarded as unstable. In 
this sense stability requires that n* and k be both positive. 

A word may not be out of place as to the eflTect of an im- 

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pressed force upon a statically unstable system. If in § 46 we 
suppose a: = 0, the solution (7) does not change its form merely 
because n^ becomes negative. The fact that a system is suscep- 
tible of purely periodic motion under the operation of an external 
periodic force is therefore no evidence of stability. 

67. For most acoustical purposes it is sufiScient to consider 
the vibrations of the systems, with which we may have to deal, 
as infinitely small, or rather as similar to infinitely small vibra- 
tiona This restriction is the foundation of the important laws 
of isochronism for free vibrations, and of persistence of period 
for forced vibrations. There are, however, phenomena of a sub- 
ordinate but not insignificant character, which depend essentially 
on the square and higher powers of the motion. We will therefore 
devote the remainder of this chapter to the discussion of the 
motion of a system of one degree of freedom, the motion not being 
so small that the squares and higher powers can be altogether 

The approximate expressions for the kinetic and potential 
energies will be of the form 

2" = i (mo + miu) tt«, F= i (/io + f^u) u\ 
If the sum of T and V be difierentiated with respect to the 
time, we find as the equation of motion 

msiU + /i^u + m{(iu + \m{lk^ -h f /Ai^' = Impressed Force, 
which may be treated by the method of successive approximation. 
For the sake of simplicity we will take the case where mi = 0, 
a supposition in no way aflfecting the essence of the question. 
The inertia of the system is thus constant, while the force of 
restitution is a composite function of the displacement, partly pro- 
portional to the displacement itself and partly proportional to 
its square — ^accordingly unsymmetrical with respect to the position 
of equilibrium. Thus for free vibrations our equation is of the 

tt-f-n*i* + aw^ = (1), 

with the approximate solution 

'2* = ^ cosn^ (2), 

where A — ^the amplitude — ^is to be treated as a small quantity. 

Substituting the value of u expressed by (2) in the last 
term, we find 

u + n*M = — a -^ (1 H-cos 2nt), 

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whence for a second approximation to the value of u 

M = ^cosni-2~ + g^^cos2/i^ (3); 

shewing that the proper tone (n) of the system is accompanied 
by its ocUive (2n), whose relative importance increases with the 
amplitude of vibration. A trained ear can generally perceive the 
octave in the sound of a tuning-fork caused to vibrate strongly by 
means of a bow, and with the aid of appliances, to be explained 
later, the existence of the octave may be made manifest to any 
one. By following the same method the approximation can 
be carried further; but we pass on now to the case of a system 
in which the recovering power is symmetrical with respect to 
the position of equilibrium. The equation of motion is then 

u + M«w + /3a» = (4), 

which may be understood to refer to the vibrations of a heavy 
pendulum, or of a load carried at the end of a straight spring. 

If we take as a first approximation t^ = J. cos ni, corresponding 
to y8 = 0, and substitute in the term multiplied by y8, we get 

u + tihi = — -r cos 3n^ i — cos rd. 

4 4 

Corresponding to the la*t term of this equation, we should 
obtain in the solution a term of the form £sin7i^, becoming 
greater without limit with L This, as in a parallel case in the 
Lunar Theory, indicates that our assumed first approximation 
is not really an approximation at all, or at least does not continue 
to be such. If, however, we take as our starting point w = -4 cos mly 
with a suitable value for m, we shall find that the solution may 
be completed with the aid of periodic terms only. In fact it is 
evident beforehand that all we are entitled to assume is that the 
motion is approximately simple harmonic, with a period wp- 
prosdmately the same, as if y3=sO. A very slight examination 
is suflScient to shew that the term varying as it*, not only may, 
but must affect the period. At the same time it is evident 
that a solution, in which the period is assumed wrongly, no 
matter by how little, must at length cease to represent the motion 
with any approach to accuracy. 

We take then for the approximate equation 

.. . , 3/3^' , /3^' o . /^x 

u-^-n^a^^ — —, — cos 771^ r-cos377it (o), 

4 4 ^ 

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of which the solution will be 

u^Aoosmt^ -^ g- -, (6), 

provided that m be taken so as to satisfy 

or m» = n» + — r— (7). 


The term in /) thus produces two effects. It alters the pitch 
of the fundamental vibration, and it introduces the twelfth as 
a necessary accompaniment. The alteration of pitch is in most 
cases exceedingly small — depending on the square of the amplitude, 
but it is not altogether insensible. Tuning-forks generally rise 
a little, though very little, in pitch as the vibration dies away. 
It may be remai'ked that the same slight dependence of pitch 
on amplitude occurs when the force of restitution is of the 
form w'wH-aw', as may be seen by continuing the approximation 
to the solution of (1) one step further than (3). The result in th%t 
case is 

-'=-'-^' (8). 

The difference m* — n' is of the same order in A in both cases ; 
but in one respect there is a distinction worth noting, namely, 
that in (8) m* is always less than n«, while in (7) it depends on 
the sign of )3 whether its effect is to raise or lower the pitch. 
However, in most cases of the unsymmetrical class the change 
of pitch would depend partly on a term of the form ax(} and 
partly on another of the form /8w*, and then 

"^^^^ "6;i« -^-4- (^>- 

[In all cases where the period depends upon amplitude, it is 
necessarily an even function thereof, a change of sign in the ampli- 
tude being merely equivalent to an alteration in phase of 180°.] 

68. We now pass to the consideration of the vibrations 
forced on an unsymmetrical system by two harmonic forces 

Eao^pt, jPcos (j^ — €). 

^ [A oorreetion is here introduced, the necessity for which was pointed oat to me 
by Dr Burton.] 

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The equation of motion is 

it + n*M = - aw» -h -Ecos|)f + -F' 008(9^ -€) (1). 

To find a first approximation we neglect the term containing 
a. Thus 

i^ = ecosp^+/cos(g^--6) (2), 

E F 
where ^= i ^. /=-^ — , (3). 

Substituting this in the term multiplied by a, we get 
t6 4- n*w = J? cos p^ + jP cos (g^ — €) 

- a I ^^ "*■ f ^^® 2pt^^Q0^ 2 {qt - 6)+ e/cos {(p -9) ^ + ej 

+ e/cos{(^ + g)^-€} L 
whence as a second approximation for u 

u = e cos2)« +/C08 {qt - 6) ^^^^ - 2~(n» - V) "^"^ ^^^ 


-^-:p^.<^'>«Kp+9)<-*l (4)- 

The additional terms represent vibrations having firequencies 
which are severally the doubles and the sum and difference of 
those of the primaries. Of the two latter the amplitudes are 
proportional to the product of the original amplitudes, shewing 
that the derived tones increase in relative importance with 
the intensity of their parent tones. 

68a. If an isolated vibrating system be subject to internal 
dissipative influences, the vibrations cannot be permanent, since 
they are dependent upon an initial store of energy which suffers 
gradual exhaustion. In order that the motion may be maintained, 
the vibrating body must be in connection with a source of energy. 
We have already considered cases of this kind under the head of 
forced vibrations, where the system is subject to forces whose 
amplitude and phase are prescribed, independently of the be- 
haviour of the system. Such forces may have their origin in 
revolving mechanism (such as electric alternators) governed so as 
to move at a uniform speed. But more frequently the forces 
under consideration depend upon the vibrations of other systems^ 

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and then the question as to how the vibrations are to be main- 
tained represents itself. A good example is afforded by the case 
already discussed (§§ 63, 65) of a fork maintained in vibration 
electrically by means of currents governed by a fork interrupter. 
It has been pointed out that the performance of the latter 
depends upon the magnetic forces operative upon it differing in 
phase from the vibrations of the fork itself. With the interrupter 
may be classed for the present purpose almost all acoustical and 
musical instruments capable of providing a sustained sound. It 
may suffice to mention vibrations maintained by wind (organ- 
pipes, harmonium reeds, seolian harps, &c.), by heat (singing 
flames, Rijke's tubes, &c.), by friction (violin strings, finger- 
glasses), and the slower vibrations of clock pendulums and watch 

In considering whether proposed forces are of the right kind 
for the maintenance or encouragement of a vibration, it is often 
convenient to regard them as reduced to impulses. Suppose, to 
take a simple case, that a small horizontal positive impulse acts 
upon the bob of a vibrating pendulum. The effect depends, of 
course, upon the phase of the vibration at the instant of the 
impulse. If the bob be moving positively at the instant in 
question the vibration is encouraged, and this effect is a maximum 
when the positive motion is greatest, that is, when the impulse 
occurs at the moment of positive movement through the position 
of equilibrium. This is the condition of things aimed at in 
designing a clock escapement, for the effect of the force is then a 
maximum in encouraging the vibration, and a minimum (zero to 
the first order of approximation) in disturbing the period Of 
course, if the impulse be half a period earlier or later than is 
above supposed, the effect is to discourage the vibration, again 
without altering the period. In like manner we see that if the 
impulse occur at a moment of maximum elongation the effect is 
concentrated upon the period, the vibration being neither en- 
couraged nor discouraged. 

In most cases the force acting upon a vibrating system in 
virtue of its connection with a source of energy may be regarded 
as harmonic. It may then be divided into two parts, one pro- 
portional to the displacement u (or to the acceleration u), the 
second proportional to the velocity ii. The inclusion of such 
forces does not alter the form of the equation of vibration 

u + KU + nhi^O (1). 

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By the first part (proportional to u) the pitch is modified, and by 
the second the coeflScient of decay. If the altered k be still 
positive, vibrations gradually die down ; but if the effect of the 
included forces be to render k negative, vibrations tend on the 
contrary to increase. The only case in which according to (I) a 
steady vibration is possible, is when the complete value of k is 
zero. If this condition be satisfied, a vibration of any amplitude 
is permanently maintained. 

When K is negative, so that small vibrations tend to increase, 
a point is of course soon reached beyond which the approximate 
equations cease to be applicable. We may form an idea of the 
state of things which then arises by adding to equation (1) a 
term proportional to a higher power of the velocity. Let us take 

w+ictt+ic'u» + n»a = (2), 

in which k and k are supposed to be small quantities. The 
approximate solution of (2) is 

u — ABmnt + —So- cos3n^ (3), 

in which A is given by 

A: + |ArV^« = (4). 

From (4) we see that no steady vibration is possible unless k and 
K have opposite signs. If k and k be both positive, the vibration 
in all cases dies down ; while if tc and k be both negative, the 
vibration (according to (2)) increases without limit. It k he 
negative and tc' positive, the vibration becomes steady and 
assumes the amplitude determined by (4). A smaller vibration 
increases up to this point, and a larger vibration falls down to it. 
If on the other hand tc be positive, while k is negative, the steady 
vibration abstractedly possible is unstable, a departure in either 
direction from the amplitude given by (4) tending always to 
increase \ 

68 b. We will now consider briefly another and a very curious 
kind of maintenance, of which the peculiarity is that the maintain- 
ing influence operates with a frequency which is the double of 
that of the vibration maintained. Probably the best known 
example is that form of Melde's experiment, in which a fine string 
is maintained in transverse vibration by connecting one of its 
extremities with the vibrating prong of a massive tuning-fork, 

^ On Maintained Vibrations, Phil, Mag., April, 18S8. 
R. 6 

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the direction of motion of the point of attachment being parallel to 
the lefigth of the string. The effect of the motion is to render 
the tension of the string periodically variable ; and at first sight 
there is nothing to cause the string to depart from its equilibrium 
condition of straightness. It is known, however, that under these 
circumstances the equilibrium may become unstable, and that the 
string may settle down into a state of permanent and vigorous 
vibration, whose period is the doMe of that of the fork. 

As a simpler example, with but one degree of freedom, we 
may take a pendulum, formed of a bar of sofb iron and vibrating 
upon knife-edges. Underneath is placed symmetrically a vertical 
bar electro-magnet, through which is caused to pass an electric 
current rendered intermittent by an interrupter whose frequency 
is twice that of the pendulum. The magnetic force does not tend 
to displace the pendulum from its equilibrium position, but 
produces the same sort of eflTect as if gravity were subject to a 
periodic variation of intensity. 

A similar result is obtained by causing the point of support 
of the pendulum to vibrate in a vertical path. If we denote this 
motion by ^ =/88in 2pt, the effect is as if gravity were variable by 
the term 4p'/8 sin 2pt 

Of the same nature are the crispations observed by Faraday* 
and others upon the surface of water which oscillates vertically, 
Faraday arrived experimentally at the conclusion that there were 
two complete vibrations of the support for each complete vibra- 
tion of the liquid. 

In the following investigation*, relative to the case of one 
degree of freedom, we shall start with the assumption that a 
steady vibration is in progress, and inquire under what conditions 
the assumed state of things is possible. 

If the force of restitution, or " spring," of a body susceptible 
of vibration be subject to an imposed periodic variation, the 
differential equation takes the form 

il + tcU'\-(n*-2asin2pt)u = (1), 

in which k and a are supposed to be small. A similar equation 
would apply approximately to the case of a periodic variation in 
the effective mass of the body. The motion expressed by the 
solution of (1) can be regular only when it keeps perfect time 

I Phil, Traru. 1831, p. 299. 
« Phil. Mag,, April, 1883. 

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with the imposed variations. It will appear that the necessary 
conditions cannot be satisfied rigorously by any simple harmonic 
vibration, but we may assume 

u * ill sinpt + -Bi cosp^ 

•filjsin Spt -hBi cos 3pt+ As 8m bpt-^ (2), 

in which it is not necessary to provide for sines and cosines of even 
multiples of pt If the assumption be justifiable, the solution in 
(2) must be convergent. Substituting in the differential equation, 
and equating to zero the coefficients of sin pt, cos pt, &c we find 

ill (n^ - j[)3) - #cpfi, - olBj 4- olB, = 0, 

5i (n^-p") + KpAj^ - oili - ttils = ; 

il , (n* - V) - 3^i>^J - (lBi + a2^8 = 0, 

JS, (n»- V) + 3/«:pil3 + ttili - ail« = ; 

A, {n^ - 2op^) - oicpB, " aB, + oBj = 0, 

Bi (n* - 2op^) + OKpAji + aiia - ail, « ; 

These equations shew that A^, B^ are of the order a relatively 
to ill, Bi'j that ilj, Ba are of order a relatively to il,, J5„ and 
so on. If we omit A^.B^ in the first pair of equations, we find 
as a first approximation, 

ili(n«-i>')-(/t/>H-a)A = 0, 
4i(^i>-a) + (n>-p»)5i = 0; 

whence ^ - —^ = ^""^/^ = V(«:i^p) /g. 

Whence A,' 'cp + a n^ -^p^ ^/{a^ Kp) ^"^^^ 

and (n^-p'y^a^-Ky (4). 

Thus, if a be given, the value of p necessary for a regular 
motion is definite ; and p having this value, the regular motion is 

u — Psin(pt + €), 

in which €, being equal to tan""^ (BJAi), is also definite. On the 
other hand, as is evident at once from the linearity of the original 
equation, there is nothing to limit the amplitude of vibration. 

These characteristics are preserved however far it may be 
necessary to pursue the approximation. If ilam+i, ^wn+i may be 
neglected, the first m pairs of equations determine the ratios of all 
the coefficients, leaving the absolute magnitude open; and they 
provide further an equation connecting p and a, by which the 
pitch is determined. 

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For the second approximation the second pair of equations 



ti = Psin(p«4-€)+ _^^^cos(3/)^-H€) (5), 

and from the first pair 


1« — ll2 — 

while /) is determined by 

f'-i''-„._-9^)' = «'-*y (7)- 

Returning to the first approximation, we see from (4) that the 
solution is possible only under the condition that a be not less 
than xp. If a = Kp, then p = n; that is, the imposed variation 
in the "spring" must be exactly twice as quick as the natural 
vibration of the body would be in the absence of friction. From 
(3) it appears that in this case € = 0, which indicates that the 
spring is a minimum one-eighth of a period after the body has 
passed its position of equilibrium, and a maximum one-eighth of a 
period before such passage. Under these circumstances the 
greatest possible amount of energy is communicated to the 
system ; and in the case contemplated it is just sufficient to 
balance the loss by dissipation, the adjustment being evidently 
independent of the amplitude. 

I{a<Kp sufficient energy cannot pass to maintain the motion, 
whatever may be the phase-relation ; but if o > ^q^, the balance 
between energy supplied and energy dissipated may be attained 
by such an alteration of phase as shall diminish the former 
quantity to the required amount. The alteration of phase may 
for this purpose be indifferently in either direction ; but if e be 
positive, we must have 

while if 6 be negative 

If a be very much greater than /cp, € = ± Jtt, which indicates 
that when the system passes through its position of equilibrium 
the spring is at its maximum or at its minimum. 

The inference from the equation that the adjustment of pitch 

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68 6.] ABSOLUTE PITCH. 85 

must be ?ibsolutely rigorous for steady vibration will be subject to 
some modification in practice; otherwise the experiment could 
not succeed. In most cases n* is to a certain extent a function of 
amplitude; so that if n* have very nearly the required value, 
complete coincidence is attainable by the assumption of an 
amplitude of large and determinate amount without other 
alterations in the conditions of the system. 

The reader who wishes to pursue this subject is referred to a 
paper by the Author " On the Maintenance of Vibrations by Forces 
of Double Frequency, and on the Propagation of Waves through a 
Medium endowed with a Periodic Structure,"^ in which the analysis 
of Mr Hill" is applied to the present problem. 

68 c. The determination of absolute pitch by means of the 
siren has already been alluded to (§ 17). In all probability first- 
rate results might be got by this method if proper provision, with 
the aid of a phonic wheel for example, were made for uniform 
speed. In recent years several experimenters have obtained excel- 
lent results by various methods ; but a brief notice of these is all 
that our limits will allow. 

One of the most direct determinations is that of Koenig*, to 
whom the scientific world has long been indebted for the construc- 
tion of much excellent apparatus. This depends upon a special 
instrument, consisting of a fork of 64 complete vibrations per 
second, the motion being maintained by a clock movement acting 
upon an escapement. A dial is provided marking ordinary time, 
and serves to record the number of vibrations executed. The 
performance of the fork is tested by a comparison between the 
instrument and any chronometer known to be keeping good time. 
The standard fork of 256 complete vibrations was compared with 
that of the instrument by observing the Lissajous's figure appro- 
priate to the double octave. 

M. Koenig has also investigated the influence of resonators 
upon the pitch of forks. Thus without a resonator a fork of 256 
complete vibrations sounded in a satis&ctory manner for about 90 
seconds. A resonator of adjustable pitch was then brought into 
proximity, and the pitch, originally much graver than that of the 

^ PhiL Mag., Angust, 1887. 

^ On the Part of the Motion of the Lunar Perigree which is a Fnnction of the 
Mean Motions of the Son and Moon, Acta Mathematica 8 ; 1, 1886. Mr Hill's 
work was first published in 1877. 

3 Wied. Ann. n. p. 394, 1880. 

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fork, was gradually raised. Even when the resonator w^ still a 
minor third below the fork, there was observed a slight diminution 
in the duration of the vibratory movement, and at the same time 
an augmentation in the frequency of about '005. As the natural 
note of the resonator approached nearer to that of the fork, this 
diminution in the time and this increase in frequency became 
more pronounced up to the immediate neighbourhood of unison ; 
but at the moment when unison was established, the alteration of 
pitch suddenly disappeared, and the frequency became exactly the 
same as in the absence of the resonator. At the same time the 
sound was powerfully reinforced; but this exaggerated intensity 
fell off rapidly and the vibration died away after 8 or 10 seconds. 
The pitch of the resonator being again raised a little, the sound of 
the fork began to* change in the opposite direction, being now as 
much too grave as before the unison was reached it had been too 
acute. The displacement then fell away by degrees, as the pitch 
of the resonator was fui-ther raised, and the duration of the 
vibrations gradually recovered its original value of about 90 
seconds. The maximum disturbance in the frequency observed 
by Koenig was 035 complete vibrations. For the explanation 
of these effects see § 117. 

The temperature coefficient found by Koenig is '000112, so that 
the pitch of a 256 fork falls '0286 for each degree Cent, by which 
the temperature rises. 

In determinations of absolute pitch' by the Author of this work 
an electrically maintained interrupter fork, whose frequency may 
for example be 32, was employed to drive a dependent fork of 
pitch 128. When the apparatus is in good order, there is a fixed 
relation between the two frequencies, the one being precisely 
four times the other. The higher is of course readily compared 
by beats, or by optical methods, with a standard of 128, whose 
accuracy is to be tested. It remains to determine the frequency 
of the interrupter fork itself. 

For this purpose the intennipter is compared with the pendulum 
of a standard clock whose rate is known. The comparison may be 
direct, or the intervention of a phonic wheel (§ 63) may be invoked. 
In either case the pendulum of the clock is provided with a silvered 
bead upon which is concentrated the light from a lamp. Im- 
mediately in front of the pendulum is placed a screen perforated 
by a somewhat narrow vertical slit. The bright point of light 
1 Nature, zvii. p. 12, 1S77 ; PhiL Tram. 1SS8, Part I. p. 316. 

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reflected by the bead is seen intermittently, either by looking over 
the prong of the interrupter or through a hole in the disc of the 
phonic wheel. In the first case there are 32 views per second, but 
in the latter this number is reduced by the intervention of the 
wheel. In the experiments referred to the wheel was so 
arranged that one revolution corresponded to four complete vibra- 
tions of the interrupter, and there were thus 8 views of the pen- 
dulum per second, instead of 32, Any deviation of the period of 
the pendulum from a precise multiple of the period of intermittence 
shews itself as a cycle of changes in the appearance of the flash 
of light, and an observation of the duration of this cycle gives the 
data for a pi'ecise comparison of frequencies. 

The calculation of the results is very simple. Supposing in 
the first instance that the clock is correct, let a be the number of 
cycles per second (perhaps ^) between the wheel and the clock. 
Since the period of a cycle is the time required for the wheel to 
gain, or lose, one revolution upon the clock, the frequency of revo- 
lution is 8 + a. The frequency of the auxiliary fork is precisely 16 
times as great, i.e. 128 ± 16a. If b be the number of beats per 
second between the auxiliary fork and the standard, the frequency 
of the latter is 

128 ± 16a ± b. 

An error in the mean rate of the clock is readily allowed for ; 
but care is required to ascertain that the actual rate at the time 
of observation does not diflfer appreciably from the mean rate. 
To be quite safe it wouid be necessarj' to repeat the deter- 
minations at intervals over the whole time required to rate the 
clock by observation of the stars. In this case it would probably 
be coDvenient to attach a counting apparatus to the phonic wheel. 

In the method of M'Leod and Clarke^ time, given by a clock, 
is recorded automatically upon the revolving drum of a chrono- 
graph, which is maintained by a suitable governor in uniform 
rotation. The circumference of the drum is marked with a grating 
of equidistant lines parallel to the axis, and the comparison between 
the drum and the standard fork is eflFected by observation of the 
wavy pattern seen when the revolving* grating is looked at past 
the edges of the vibrating prongs. These observers made a special 
investigation as to the effect of bowing a fork upon previously 
existing vibrations. Their conclusion is that in the case of un- 
loaded forks no sensible change of phase occurs. 
1 Phil. Trans, 1880, Part I. p. 1. 

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In the chronographic method of Prof. A. M. Mayer* the fork 
under investigation is armed with a triangular fragment of thin 
sheet metal, one milligram in weight, and actually traces its 
vibrations as a curve of sines upon smoked paper. The time is 
recorded by small electric discharges from an induction apparatus, 
under the control of a clock, and delivered from the same tracing 
point Although the disturbance due to the tracing point appears 
to be very small, it is doubtful whether this method could compete 
in respect of accuracy with those above described where the com- 
parison with the standard is optical or acoustical On the other 
hand, it has the advantage of not requiring a uniform rotation of 
the drum, and the apparatus lends itself with facility to the deter- 
mination of small intervals of time after the manner originally 
proposed by T. Young*. 

68d. The methods hitherto described for the determination of 
absolute pitch, with the exception of that of Scheibler, may be 
regarded as rather mechanical in their character, and they depend 
for the most part upon somewhat special apparatus. It is possible, 
however, to determine pitch with fair accuracy with no other 
appliances than a common harmonium and a watch, and as the 
process is instructive in respect of the theory of overtones, a short 
account will here be given of it*. 

The fimdamental principle is that the absolute frequencies of 
two musical notes can be deduced from the interval between 
them, i.e. the ratio of their frequencies and the number of beats 
which they occasion in a given time when sounded together. 
For example, if x and y denote the frequencies of two notes whose 
interval is an equal temperament major third, we know that 
y = 1*25992 x. At the same time the number of beats heard in a 
second depending upon the deviation of the third from true 
intonation, is 4^ — ox. In the case of the notes of a harmonium, 
which are rich in overtones, these beats are readily counted, and 
thus two equations are obtained from which the values of x and y 
are at once found. 

Of course in practice the truth of an equal temperament third 
could not be taken for granted, but the difficulty thence arising 
would be easily met by including in the counting all the three 

^ National Academy of Sciences, Washington, 3/emoirf , Vol. iii. p. 43, 18S4. 
« Lecturei, Vol. i. p. 191. 
» Nature, Jan. 28, 1S79. 

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major thirds which together make up an octave. Suppose, for 
example, that the frequencies of c, e, ^rjf , c are respectively op, y, Zi 
2a:, and that the beats per second between x and y are a, between 
y and z are 6, and between z and 2a? are c. Then 

4^ ~ 5^' 3s a, 4z — oy^ b, Sx — 5^ =» c, 
from which a- = ^ (25a -f 206 H- 1 6c), 

y = i (32a + 256 + 20c), 
^«i(^W)a + 326 + 25c). 

In the above statements the octave c — c' is for simplicity 
supposed to be true. The actual error could readily be allowed 
for if required ; but in practice it is not necessary to use c at all, 
inasmuch as the third set of beats can be counted equally well 
between ^rf and c. 

The principal objection to the method in the above form is 
that it presupposes the' absolute constancy of the notes, for 
example, that y is the same whether it is being sounded in 
conjunction with x or in conjunction with z. This condition is 
very imperfectly satisfied by the notes of a harmonium. 

In order to apply the fundamental principle with success, it is 
necessary to be able to check the accuracy of the interval which is 
supposed to be known, at the same time that the beats are being 
counted. If the interval be a major tone (9 : 8), its exactness is 
proved by the absence of beats between the ninth component of 
the lower and the eighth of the higher note, and a counting 
of the beats between the tenth component of the lower and the 
ninth of the higher note completes the necessary data for de- 
termining the absolute pitch. 

The equal temperament whole tone (1*12246) is intermediate 
between the minor tone (1*11111) and the major tone (1*12500), 
but lies much nearer to the latter. Regarded as a disturbed 
major tone, it gives slow beats, and regaixied as a disturbed 
minor tone it gives quick ones. Both sets of beats can be heard 
at the same time, and when counted (by two observers) give the 
means of calculating the absolute pitch of both notes. If x and y 
be the frequencies of the two notes, a and 6 the frequencies of the 
slow and quick beats respectively, 
, 9a?— .8y = a, 9y — 10a? = 6, 

whence a? = 9a + 86, y = 10a + 96. 

Theapplication of this method in no way assumes the truth of 

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the equal temperament whole tone, and in fact it is advantageous 
to flatten the interval somewhat, so as to make it lie more nearly 
midway between the major and the minor tone. In this way the 
rapidity of the quicker beats is diminished, which facilitates the 

The course of an experiment is then as follows. The notes C 
and D are sounded together, and at a given signal the observers 
begin counting the beats situated at about d!' and e" on the scale. 
After the expiration of a measured interval of time a second signal 
is given, and the number of both sets of beats is recorded. 

For further details of the method reference must be made to 
the original memoir, but one example of the results may be given 
here. The period being 10 minutes, the number of beats recorded 
were 2392 and 2341, giving x = 6709 as the pitch of C. 

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69. We have now examined in some detail the oscillations 
of a system possessed of one degree of freedom, and the results, 
at which we have arrived, have a very wide application. But 
material systems enjoy in general more than one degree of 
freedom. In order to define their configuration at any moment 
several independent variable quantities must be specified, which, 
by a generalization of language originally employed for a point, 
are called the co-ordinates of the system, the number of indepen* 
dent co-ordinates being the index of freedom. Strictly speaking, 
the displacements possible to a natural system are infinitely 
various, and cannot be represented as made up of a finite number 
of displacements of specified type. To the elementary parts of 
a solid body any arbitrary displacements may be given, subject 
to conditions of continuity. It is only by a process of abstraction 
of the kind so constantly practised in Natural Philosophy, that 
solids are treated as rigid, fluids as incompressible, and other sim- 
plifications introduced so that the position of a system comes to 
depend on a finite number of co-ordinates* It is not, however, 
our intention to exclude the consideration of systems possessing 
infinitely various freedom; on the contrary, some of the most 
interesting applications of the results of this chapter will lie in 
that direction. But such systems are most conveniently conceived 
as limits of others, whose freedom is of a more restricted kind. 
We shall accordingly commence with a system, whose position 
is specified by a finite number of independent co-ordinates ^,, 
^„ ^„ &c. 

70. The main problem of Acoustics consists in the investi- 
gation of the vibrations of a system about a position of stable 
equilibrium, but it will be convenient to commence with the 

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statical part of the subject. By the Principle of Virtual Velocities, 
if we reckon the co-ordinates yp^u ^2, ifec. from the configuration 
of equilibrium, the potential energy of any other configuratioD 
will be a homogeneous quadratic function of the co-ordinates, 
provided thart the displacement be sufficiently small. This quan- 
tity is called F, and represents the work that may be gained in 
passing from the actual to the equilibrium configuration. We may 

F = iCn^i'+iCffl^2'+----^Ci,^iV^, + C^^,^,-h (1). 

Since by supposition the equilibrium is thoroughly stable, the 
quantities Cn, c^, Cii» &c. must be such that V is positive for all 
real values of the co-ordinates. 

71. If the system be displaced from the zero configuration 
by the action of given forces, the new configuration may be 
found from the Principle of Virtual Velocities. If the work done 
by the given forces on the hypothetical displacement S-^i, S^a, 
&c. be 

^iSti + ^2% + (1), 

this expression must be equivalent to SF, so that since Syjr^y S^,, 
&c. are independent, the new position of equilibrium is deter- 
mined by 

'4i"^- ^|-*-«- <«. 

or by (1) of §70, 

. C-nti + C^ir^-^C^ylr^+ =^,l (3), 

where there is no distinction in value between c,., and c,;.. 

From these equations the co-ordinates may be determined in 
terms of the forces. If V be the determinant 

Cii, Cij, Cis, .. 

Ca> ^28* ^23> •• 
C31, Cjftt, Cj3, .. 

the solution of (3) may be written 

dcii ^ dcia 



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These equations determine -^i, yft^, &c. uniquely, since V doea 
not vanish, as appears from the consideration that the equations 
dVjd^^ = 0, &c. could otherwise be satisfied by finite values of the 
co-ordinates, provided only that the ratios were suitable, which is 
contrary to the hypothesis that the system is thoroughly stable in 
the zero configuration. 

72. If Vrj, ... ^1, ... and ^/, ... ^/, ... be two sets of dis- 
placements and corresponding forces, we have the following re- 
ciprocal relation, 

^i^/+.^«^/ + ...=^i>i + ^a't.-f (1), 

as may be seen by substituting the values of the forces, when each 
side of (1) takes the form, 

Suppose in (1) that all the forces vanish except "9^ and '*'/; 

^,V^/ = ^i'>^i (2). 

If the forces ^j and '*'/ be of the same kind, we may suppose 
them equal, and we then recognise that a force of any type acting 
alone produces a displacement of a second type equal to the 
displacement of the first type due to the action of an equal force 
of the second type. For example, if A and B be two points 
of a rod supported horizontally in any manner, the vertical de- 
flection at A, when a weight W is attached at B, is the same as 
the deflection at B, when W is applied at A *. 

73. Since F is a homogeneous quadratic function of the co- 

^•--iK+'+lf.*-^ (')• 

or, if "^i, '^'a, &c. be the forces necessary to maintain the dis- 
placement represented by V^ij-^sj&c., 

2F=^,^, + >Fa^.-h (2). 

If ^^i + A-^i, '^2-|-A'^2, &0. represent another displacement, 
for which the necessary forces are ^i-H A^i, %-|- A%, &c., the 

1 On this sabjeot, see PhiU Mag,, Deo., 1S74, and Maroh, 1875. 

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corresponding potential energy is given by 

+ A^i.^i + A>Fa.>/^a+... 

+ A^i.A^i + A^a.A^,+ ..., 
80 that we may write 

2A7=2^.A>^ + 2A^.i|r + SA>F.A^ (3), 

where AF is the difference of the potential energies in the two 
cases, and we must particularly notice that by the reciprocal 
relation, § 72 (1), 

S^.A^r^SANl^.^r (4). 

From (3) and (4) we may deduce two important theorems, 
relating to the value of F for a system subjected t6 given dis- 
placements, and to given forces respectively. 

74. The first theorem is to the effect that, if given displace- 
ments (not sufficient by themselves to determine the configuration) 
be produced in a system by forces of corresponding types, the re- 
sulting value of Ffor the system so displaced, and in equilibrium, 
is as small as it can be under the given displacement conditions ; 
and that the value of F for any other configuration exceeds this 
by the potential energy of the configuration which is the difference 
of the two. The only difficulty in the above statement consists 
in understanding what is meant by * forces of corresponding types.* 
Suppose, for example, that the system is a stretched string, of 
which a given point P is to be subject to an obligatory displace- 
ment; the force of corresponding type is here a force applied 
at the point P itself. And generally, the forces, by which the 
proposed displacement is to be made, must be such as would do 
no work on the system, provided^nly that that displacement were 
710^ made. 

By a suitable choice of co-ordinates, the given displacement 
conditions may be expressed by ascribing given values to the first 
r co-ordinates ^i, '^a* ••• '^r, and the conditions as to the forces 
will then be represented by making the forces of the i^emaining 
types '^'r+n '*'r+si &c. vanish. If -^ -h A-^/r refer to any other con- 
figuration of the system, and N?" -H A^ be the corresponding forces, 
we are to suppose that A*^,, A*^], &c. as far as A^r c^U vanish. 
Thus for the first r suffixes A-^ vanishes, and for the remaining 

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suffixes ^ vanishes. Accordingly SNlT.A^ is zero, and therefore 
SA'*'.'^ is also zero. Hence 

2AF=2A^.AVr (1), 

which proves that if the given displacements be made in any 
other than the prescribed way, the potential energy is increased 
by the energy of the diflference of the configurations. 

By means of this theorem we may trace the effect on F of any 
relaxation in the stiffness of a system, subject to given displacement 
conditions. For, if after the alteration in stiffness the original equi- 
librium configuration be considered, the value of V corresponding 
thereto is by supposition less than before ; and, as we have just 
seen, there will be a still further diminution in the value of V 
when the system passes to equilibrium under the altered con- 
ditions. Hence we conclude that a diminution in F as a function 
of the co-ordinates entails also a diminution in the actual value of 
V when a system is subjected to given displacements. It will 
be understood that in particular cases the diminution spoken of 
may vanish ^ 

For example, if a point P of a bar clamped at both ends be 
displaced laterally to a given small amount by a force there ap- 
plied, the potential energy of the deformation will be diminished 
by any relaxation (however local) in the stifihess of the bar. 

76. The second theorem relates to a system displaced by given 
forces, and asserts that in this case the value of F in equilibrium 
is greater than it would be in any other configuration in which 
the system could be maintained at rest under the given forces, by 
the operation of mere constraints. We will shew that the removal 
of constraints increases the value of F. 

The co-ordinates may be so chosen that the conditions of con- 
straint are expressed by 

^, = 0, V^, = 0, yJTr^O (1). 

We have then to prove that when ^r+n ^r+a» &c. are given, the 
value of F is least when the conditions (1) hold. The second 
configuration being denoted as before by •^i + A'^i &c., we see 
that for suffixes up to r inclusive -^ vanishes, and for higher 
suffixes A'4^ vanishes. Hence 

2V^.A^ = 2A^.^ = 0, 

^ See a paper on Geneial Theorems relating to Equilibrium and Initial and 
Steady Motions. Phil, Mag., March, 1875. 

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and therefore 

2AF = 2A^.iX^ (2), 

shewing that the increase in V due to the removal of the con- 
straints is equal to the potential energy of the difference of the two 

76. We now pass to the investigation of the initial motion of 
a system which starts from rest under the operation of given 
impulses. The motion thus acquired is independent of any 
potential energy which the system may possess when actually 
displaced, since by the nature of impulses we have to do only 
with the initial configuration itself. The initial motion is also 
independent of any forces of a finite kind, whether impressed on 
the system from without, or of the nature of viscosity. 

If P, Q, R be the component impulses, parallel to the axes, on 
a particle m whose rectangular co-ordinates are x, y, z, we have by 
D'Alembert's Principle 

Sm(^&r + ySy + iS-^) = 2(P&r + Q% + iJS^) (1), 

where x, y, i denote the velocities acquired by the particle in virtue 
of the impulses, and Bx, Sy, Sz correspond to any arbitrary dis- 
placement of the system which does not violate the connection of 
its parts. It is required to transform (1) into an equation expressed 
by the independent generalized co-ordinates. 

For the first side, 

(dx dx d i \ 

, J , _ ( . dx , . dv , . dz\ 
+ dir,lm(.^+y^ + .^J^ 

-, . « / , dx . djf dz \ 
= «^j.i2m-^-(;r« + y« + i»)+ 

= st,|f + a^,jf+ (2). 

where T, the kinetic energy of the system is supposed to be 
expressed as a function of -^j, -^g, &c. 

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76.] IMPULSES. 97 

On the second side, 
MP^ + Qh + RBz) = Sf.tm(p^+Q^ + R^) + 

= f,S^i + f,S^.+ (3), 

The transformed equation is therefore 

(j|-f')«*'+(kl-f-)'*-+-=» <*>• 

where S-^i.-S-^^a* &c. are now completely independent. Hence to 
determine the motion we have 

yr = fi» ,r = f9,&c (5), 

where fi, f„ &c. may be considered as the generalized components 
of impulse. 

77. Since T is a homogeneous quadratic function of the gene- 
ralized co-ordinates, we may take 

T=-^(hiiri^-^ia^^^+ + 012^1^1^2 + aa'^2>^.+ (1), 





where there is no distinction in value between Ors and a„^ 
Again, by the nature of T, 

27=1^.1^+^,1^^+ = fttx + f,^.+ (3). 

The theory of initial motion is closely analogous to that of the 
displacement of a system from a configuration of stable equilibrium 
by steadily applied forces. In the present theory the initial kinetic 
energy T bears to the velocities and impulses the same relations 
as in the former V bears to the displacements and forces respect- 
ively. In one respect the theory of initial motions is the more 
complete, inasmuch as T is exactly, while V is in general only 
approximately, a homogeneous quadratic function of the variable& 

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If '^i, '^ai . . .i f i» f a » • • • denote one set of velocities and impulses 
for a system started from rest, and -^Z, -^a', ..., f/, f,', ... a second 
set, we may prove, as in § 72, the following reciprocal relation : 

fi'^i+f.'^a+...=fi^/+fa^a'-f (4)^ 

This theorem admits of interesting application to fluid motion. 
It is known, and will be proved later in the course of this work, 
that the motion of a frictionless incompressible liquid, which 
starts from rest, is of such a kind that its component velocities 
at any point are the corresponding differential coefficients of a 
certain function, called the velocity-potential. Let the fluid be 
set in motion by a prescribed arbitrary deformation of the surface 
S of a closed space described within it. The resulting motion is 
determined by the normal velocities of the elements of S, which, 
being shared by the fluid in contact with them, are denoted by 
du/dn, if u be the velocity-potential, which interpreted physically 
denotes the impulsive pressure. Hence by the theorem, if v be 
the velocity-potential of a second motion, corresponding to 
another set of arbitrary surface velocities dv/dn, 

. \\^>-\\'> ■■ <«■ 

— ^an equation immediately following from Green's theorem, if 
besides S there be only fixed solids immersed in the fluid. The 
present method enables us to attribute to it a much higher gene- 
rality. For example, the immersed solids, instead of being fixed> 
may be free, altogether or in part, to take the motion imposed 
upon them by the fluid pressures. 

78. A particular case of the general theorem is worthy of 
special notice. In the first motion let 

^i=il, ^a = 0, f8 = f4 = f« =0; 

and in the second. 

Then f/ = f, (1). 

In words, if, by means of a suitable impulse of the correspond- 
ing type, a given arbitrary velocity of one co-ordinate be impressed 
on a system, the impulse corresponding to a second co-ordinate 
necessary in order to prevent it from changing, is the same as 
would be required for the first co-ordinate, if the given velocity- 
were impressed on the second. 

^ Thomson and Tait, § 313 (/). 

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78.] Kelvin's theorem. 99 

As a simple example, take the case of two spheres A and B •- 
immersed in a liquid, whose centres are free to move along certain 
lines. If ^ be set in motion with a given velocity, B will 
naturally begin to move also. The theorem asserts that the 
impulse required to prevent the motion of B, is the same as if 
the functions of A and B were exchanged : and this even though 
there be other rigid bodies, C, D, &c., in the fluid, either fixed, or 
free in whole or in part. 

The case of electric currents mutually influencing each other by 
induction is precisely similar. Let there be two circuits A and B, 
in the neighbourhood of which there may be any number of other 
wire circuits or solid conductors. If a unit current be suddenly 
developed in the circuit A, the electromotive impulse induced in 
B is the same as there would have been in A, had the current been 
forcibly developed in B, 

79. The motion of a system, on which given arbitrary velocities 
are impressed by means of the necessary impulses of the corre- 
sponding t)rpes, possesses a remarkable property discovered by 
Thomson. The conditions are that -^i, yjr^, '^s, ...'^r are given, 
while fr+i» fr+2, ••• vanish. Let yjti, -^a, •••?!, fa, &c. correspond to 
the actual motion ; and 

to another motion satisf}dng the same velocity conditions. For 
each suffix either A*^ or f vanishes. Now for the kinetic energy 
of the supposed motion, 

2(r+Ar)=(f,+Af,)(^i + A^0 + ... 

= 2T+f,A>^, + f,A^,+ ... 
+ Afi.i^i + Afj.i^j+... + AfiAi|rj + Af,A>^a+.... 
But by the reciprocal relation (4) of § 77 

faAi|ri-h...=Afa.'^i + ..., 

of which the former by hypothesis is zero ; so that 

2Ar=Af,Ai^i + Af,A^,+ (1), 

shewing that the energy of the supposed motion exceeds that of 
the actual motion by the energy of that motion which would have 
to be compounded with the latter to produce the former. The 
motion actually induced in the system has thus less energy than 
any other satisfying the same velocity conditions. In a subsequent 
chapter we shall make use of this property to find a superior limit 
to the energy of a system set in motion with prescribed velocities. 

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If any diminution be made in the inertia of any of the parte 
of a system, the motion corresponding to prescribed velocity 
conditions will in general undergo a change. The value of T will 
necessarily be less than before ; for there would be a decrease even 
if the motion remained unchanged, and therefore a fortiori when 
the motion is such as to make T an absolute minimum. Con- 
versely any increase in the inertia increases the initial value of T, 

This theorem is analogous to that of § 74. The analogue for 
initial motions of the theorem of § 75, relating to the potential 
energy of a system displaced by given forces, is that of Bertrand, 
and may be thus stated : — If a system start from rest under the 
operation of given impulses, the kinetic energy of the actual motion 
exceeds that of any other motion which the system might have 
been guided to take with the assistance of mere constraints, by the 
kinetic energy of the difference of the motions^ 

[The theorems of Kelvin and Bertrand represent different 
aspects of the same truth. Let us suppose that the prescribed 
impulse is entirely of the first type fi. Then r = ifi^i, whether 
the motion be free or be subjected to any constraint. Further, 
under any given circumstances as to constraint, -^i is proportional 
to fi, and the ratio fi : -^j may be regarded as the moment of 
inertia ; so that 

Kelvin's theorem asserts that the introduction of a consti^aint 
can only increase the value of T when -^i is given. Hence whether 
•^1 be given or not, the constraint can only increase the ratio of 
27 to -^i' or of fi to -^i. Both theorems are included in the 
statement that the moment of inertia is increased by the intro- 
duction of a constraint.] 

80. We will not dwell at any greater length on the mechanics 
of a system subject to impulses, but pass on to investigate 
Lagrange's equations for continuous motion. We shall suppose 
that the connections binding together the parts of the system 
are not explicit fiinctions of the time; such cases of forced 
motion as we shall have to consider will be specially shewn to 
be within the scope of the investigation. 

By D'Alembert's Principle in combination with that of Virtual 

2m Qthx + yhy + zhz) = 2 {Xhx + Yhy + Zhz) (1), 

^ Thomson and Tait, § 811. Phil, Mag. March, 1875. 

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80.] Lagrange's equations. 101 

where Sx, Sy, Sz denote a displacement of the system of the most 
general kind possible without violating the connections of its 
parts. Since the displacements of the individual particles of 
the system are mutually related, Sa;, ... are not independent. The 
object now is to transform to other variables -^i, -^j,..., w^hich 
shall be independent. We have 

so that 

xBx = -J- (xhx) — ^Sd^ , 

lm{xSx + ySy + zSz) = ^. 2m (xSx + y Sy + iS^) - ST, 
But (§ 76) we have already found that 

while ST^^B^, + ^^^,+ ..., 

if r be expressed as a quadratic function of -^i, ^j, ..., whose 
coeflScients are in general functions of V^u'^j,.... Also 

d (dT ..\ d (dT\ ., dT ^.. 


inasmuch as -^ S>^i ^B-rr-^i, 


^SQ-f}^-* <^^ 

Thus, if the transformation of the second side of (1) be 

2(X&c+y«y + ZS^) = ^iS^i + ^a8V^, + (3), 

we have equations of motion of the form 

if^).^^ = ^ (4). 

dVdyjr' dy^ ^ 

Since '^'S^ denotes the work done on the system during a 
displacement S^, "9 may be regarded as the generalized com- 
ponent of force. 

In the case of a conservative system it is convenient to 
separate &om '^ those parts which depend only on the configura- 

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tion of the system. Thus, if V denote the potential energy, we 
may write 

dt\d'^) dit dyjr ^ ^' 

where 'V is now limited to the forces acting on the system which 
are not already taken account of in the term dV/d'^. 

81. There is also another group of forces whose existence 
it is often advantageous to recognize specially, namely those 
arising from friction or viscosity. If we suppose that each 
particle of the system is retarded by forces proportional to its 
component velocities, the effect will be shewn in the fundamental 
equation (1) § 80 by the addition to the left-hand member of 
the terms 

2 {kJcZx -f Kyi/hy H- Kg^ Bz\ 

where Kx, /Cy, Kg are coefficients independent of the velocities, 
but possibly dependent on the configuration of the system. The 
transformation to the independent co-ordinates -^i, y^^, &c. is 
effected in a similar manner to that of 

Sy/t {xSw + yBy + zSz) 
considered above (§ 80), and gives 

dF c , dF ^ , ,- . 

^a^.-H^-^^sv^.-H (1). 

where i" = ^2 (xg^ + Kyy^ + kJ;^) 

= i6u^i' + i6«^2" + ... + 6i2^it« + b^yjr.yjt, + (2). 

Fy it will be observed, is like T a homogeneous quadratic 
function of the velocities, positive for all real values of the 
variables. It represents half the rate at which energy is dissipated. 

The above investigation refers to retarding forces proportional 
to the absolute velocities ; but it is equally important to consider 
such as depend on the relative velocities of the parts of the 
system, and fortunately this can be done without any increase 
of complication. For example, if a force act on the particle Xi 
proportional to (d^ — ij), there will be at the same moment an 
equal and opposite force acting on the particle x^. The additional 
terms in the fundamental equation will be of the form 

fC» (Xj — X2) BXi + Kx (Xt — Xi) &Cj, 

which may be written 

tCx (iJi - 4) B(Xi - ^j) = S^i -y- [^Kx (Xi - X^y] + 

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and 80 on for any number of pairs of mutually influencing 
particles. The only eflfect is the addition of new terms to F, 
which still appears in the form (2)\ We shall see presently that 
the existence of the function F, which may be called the Dis- 
sipation Function, implies certain relations among the coefficients 
of the generalized equations of vibration, which carry with them 
important consequences^ 

The equations of motion may now be written in the form 


dtKd'f) df d^ df 

82. We may now introduce the condition that the motion 
takes place in the immediate neighbourhood of a configuration 
of thoroughly stable equilibrium ; T and F are then homogeneous 
quadratic functions of the velocities with coefficients which are 
to be treated as constant, and F is a similar function of the 
co-ordinates themselves, provided that (as we suppose to be 
the case) the origin of each co-ordinate is taken to correspond 
with the configuration of equilibrium. Moreover all three 
functions are essentially positive. Since terms of the form dT/dyfr 
are of the second order of small quantities, the equations of motion 
become linear, assuming the form 

dAdylrJ^d^jr^dyk'^ ^^^' 

dt\d^J dyjt ' d'sjt 

where under ^ are to be included all forces acting on the system 
not already provided for by the differential coefficients of F and V. 
The three quadratic functions will be expressed as follows : — 

-P = i6nti»+i6a^,*+ ... +6i2^i^,-H ... ■ (2), 

where the coefficients a, b, c are constants. 

From equation (1) we may of course fall back on previous 
results by supposing F and F, or F and T, to vanish. 

A third set of theorems of interest in the application to Elec- 

^ The differences referred to in the text may of coarse pass into differential 
coefficients in the case of a body continuously deformed. 

> The Dissipation Function appears for the first time, so far as I am aware, in 
a paper on General Theorems relating to Vibrations, published in the Proeeedingi 
of the Mathematical Society for June, 1873. 

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tricity may be obtained by omitting T €uid F, while F is retained, 
but it is unnecessary to pursue the subject here. 

If we substitute the values of T, F and F, and write D for djdt, 
we obtain a system of equations which may be put into the form 

^ii-^i + ^ij-^a + e^-^t + ... = ^1 ' 



where en denotes the quadratic operator 

e« = a«i)» + 6rJ> + Cr, (4). 

It must be particularly remarked that since 

art = ^try ^ri — ^trt <^r9 = ^tn 

it follows that €„^etr (5). 

[The theory of motional forces, i.e. forces proportional to the 
velocities, has been further developed in the second edition of 
Thomson and Tait's Natural Philosophy (1879). In the most 
general case the equations may be written 

where bn^btr, ^rf = Ar (7). 

Of these the terms with the coefficients b can be derived from 
the dissipation function 

The terms in ^ on the other hand do not represent dissipation, 
and are called the gyrostatic terms. 

If we multiply the first of equations (6) by -^i, the second by 
-^j, &c., and then add, we obtain 

^^l^ + 2F^^,ir, + ^,yfr,-\- (8). 

In this the first term represents the rate at which energy is 
being stored in the system ; 2^ is the rate of dissipation ; and the 
two together account for the work done upon the system by the 
external forces.] 

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83. Before proceeding further, we may draw an important 
inference from the linearity of our equations. If corresponding 
respectively to the two sets of forces ^j, ^j,..., ^/, ^a', ... two 
motions denoted by -^i, >^j, ..., i^/, i^,', ... be possible, then must 
also be possible the motion '^i + >f^/, -^a + V^a'i • • • in conjunction 
with the forces "5^1 + '*'i', '^'a + '*'«'» .••• Or, as a particular case, 
when there are no impressed forces, the superposition of any two 
natural vibrations constitutes also a natural vibration. This is the 
celebrated principle of the Coexistence of Small Motions, first 
clearly enunciated by Daniel Bernoulli. It will be understood 
that its truth depends in general on the justice of the assumption 
that the motion is so small that its square may be neglected. 

[Again, if a system be under the influence of constant forces 
"^1, &c., which displace it into a new position of equilibrium, the 
vibrations which may occur about the new position are the same 
as those which might before have occurred about the old position.] 

84. To investigate the free vibrations, we must put '*'i, ^a, ... 
equal to zero ; and we will commence with a system on which no 
fiictional forces act, for which therefore the coefficients e^i* &c. are 
even functions of the sjrmbol D, We have 

eai-^i + ea^^sH- ....= \ (!)• 

From these equations, of which there are as many (m) as the 
system possesses degrees of liberty, let all but one of the valuables 
be eliminated. The result, which is of the same form whichever 
be the co-ordinate retained, may be written 

Vt = (2), 

where V denotes the determinant 


! ^u> ^ia> ^is> ••• 
^Ji> ^a2» ^as> ••• 

and is (if there be no friction) an even function of D of degree 2m. 
I^t +X,, iXa, ..., ±\to be the roots of V=0 considered as an 
equation in D, Then by the theory of differential equations the 
most general value of '^ is 

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where the 2m quantities A, A\ B, B\ &c. are arbitrary constants. 
This form holds good for each of the co-ordinates, but the constants 
in the diflferent expressions are not independent. In fact if a 
particular solution be 

the ratios -4^ : -4, : -4, ... are completely determined by the 


6ii-4i + eMilaH-^i8^i + =0 \ 

en-4iH-Cail,-|-6a^8+ =0 > (5)i 

where in each of the coefficients such as ^„» ^ is substituted for i). 
Equations (5) are necessarily compatible, by the condition that Xi 
is a root of V=0. The ratios A^ :Ai\At ... corresponding to 
the root — Xj are the same as the ratios Ax'.A^iA^..., but for 
the other pairs of roots Xj, - X^, &c. there are distinct systems of 

86. The nature of the system with which we are dealing 
imposes an important restriction on the possible values of X, If Xi 
were real, either \ or — Xi would be real and positive, and we 
should obtain a particular solution for which the co-ordinates, and 
with them the kinetic energy denoted by 

increase without limit. Such a motion is obviously impossible for 
a conservative system, whose whole energy can never differ from 
the sum of the potential and kinetic energies with which it was 
animated at starting. This conclusion is not evaded by taking Xi 
negative ; because we are as much at liberty to trace the motion 
backwards as forwards. It is as certain that the motion never was 
infinite, as that it never will he. The same argument excludes the 
possibility of a complex value of X. 

We infer that all the values of X are purely imaginary, cor- 
responding to real negative values of W Analytically, the fact 
that the roots of V = 0, considered as an equation in i)*, are 
all real and negative, must be a consequence of the relations 
subsisting between the coefficients Ou, Oia, ..., Cu, Cu, ... in virtue of 
the fact that for all real values of the variables T and V are 
positive. The case of two degrees of liberty will be afterwards 
worked out in full. 

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86. The form of the solution may now be advantageously 
changed by writing irii for \i, &c. (where i= V — 1), and taking 
new arbitrary constants. Thus 

-1^1 = Ai cos (lilt - a) + -Bi cos {nj; - ^8) + Ci cos (n^t - 7) + ... ' 

-^2 = ila cos (ni^ — a) + jB, cos (wj^ — /8) + Ca cos (n,^ — 7) + ... ..,,(i) 

-^/r, = ^, cos (nj; - a) + 5, cos (nj; — I3) + Ct cos (n^t - 7) + . . 

where ni\ n,*, &c. are the m roots of the equation of m^ degree 
in 71* found by writing — n^ for D* in V = 0. For each value of n 
the ratios A^iAiiAt,.. are determinate and real. 

This is the complete solution of the problem of the free 
vibrations of a conservative system. We see that the whole 
motion may be resolved into vi normal harmonic vibrations of 
(in general) different periods, each of which is entirely indepen- 
dent ef the others. If the motion, depending on the original 
disturbance, be such as to reduce itself to one of these (rii) 
we have 

y^i^Ai cos {riit — a), y^^^^i cos {nj; - a), &c (2), 

where the ratios -4^:^.2:^43 ...depend on the constitution of the 
system, and only the absolute amplitude and phase are arbitrary. 
The several co-ordinates are always in similar (or opposite) phases 
of vibration, and the whole system is to be found in the configura- 
tion of equilibrium at the same moment. 

We perceive here the mechanical foundation of the supremacy 
of harmonic vibrations. If the motion be sufficiently small, the 
differential equations become linear with constant coefficients; 
while circular (and exponential) functions are the only ones which 
retain their type on differentiation. 

87. The m periods of vibration, determined by the equation 
V =0, are quantities intrinsic to the system, and must come out 
the same whatever co-ordinates may be chosen to define the con- 
figuration. But there is one system of co-ordinates, which is 
especially suitable, that namely in which the normal types of 
vibration are defined by the vanishing of all the co-ordinates but 
one. In the first type the original co-ordinates '^u'^j, &c. have 
given ratios; let the quantity fixing the absolute values be ^, so 
that in this t3rpe each co-ordinate is a known multiple of 0,. So 
in the second type each co-ordinate may be regarded as a known 
multiple of a second quantity <^2i &nd so on. By a suitable deter- 

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mination of the m quantities ^, ^s> &c., any configuration of the 
system may be represented as compounded of the m configurations 
of these tjrpes, and thus the quantities ^ themselves may be looked 
upon as co-ordinates defining the configuration of the system. 
They are called the normal co-ordinates \ 

When expressed in terms of the normal co-ordinates, T and V 
are reduced to sums of squares ; for it is easily seen that if the 
products also appeared, the resulting equations of vibration would 
not be satisfied by putting any m — 1 of the co-ordinates equal to 
zero, while the remaining one was finite. 

We might have commenced with this transformation, assuming- 
from Algebra that any two homogeneous quadratic functions can 
be reduced by linear transformations to sums of squares. Thus 

where the coefficients (in which the double suffixes are no longer 
required) are necessarily positive. 
Lagrange's equations now become 

ai^ + Ci<^i = 0, a,$, + Cj<^ = 0, &c (2), 

of which the solution is 

4>i = A cos(riit — a), 0, = £ cos (ti^ — /8), &c (3), 

where A, 5..., a, /8... are arbitrary constants, and 

ni»=Ci-rai, n^^c^-^a^, &c (4). 

[The vibrations expressed by the various normal co-ordinates 
are completely independent of one another, and the energy of the 
whole motion is the simple sum of the parts corresponding to the 
several normal vibrations taken separately. In fact by (1) 

r+F=icx^« + iM,« + (3). 

By the nature of the case the coefficients a are necessarily 
positive. But if the equilibrium be unstable, some of the 
coefficients c may be negative. Corresponding to any negative 
c, n becomes imaginary and the circular functions of the time are 
replaced by exponentials. 

In any motion proportional to e^ the disturbance is equally 
multiplied in equal times, and the degree of instability may be 
considered to be measured by X. If there be more than one 

^ Thomson and Tait's Natural Philoiophy, first edition 1867, § 337. 

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unstable mode, the relative importance is largely determined by 
the corresponding values of X. Thus, if 

in which Xj > Xj, then whatever may be the finite ratio o{ A : B, 
the first term ultimately acquires the preponderance, inasmuch as 

In general, unstable equilibrium when disturbed infinitesimally 
will be departed from according to that mode which is most 
unstable^ viz. for which X is greatest. In a later chapter we shall 
meet with interesting applications of this principle. 

The reduction to normal co-ordinates allows us readily to trace 
what occurs when two of the values of n* become equal. It is 
evident that there is no change of form. The spherical pendulum 
may be referred to as a simple example of equal roots. It is 
remarkable that both Lagrange and Laplace fell into the error of 
supposing that equality among roots necessarily implies terms 
containing ^ as a factor^ The analytical theory of the general 
case (where the co-ordinates are not normal) has been discussed by 
SomoP and by Routh'.] 

88. The interpretation of the equations of motion leads to a 
theorem of considerable importance, which may be thus stated*. 
The period of a conservative system vibrating in a constrained type 
about a position of stable equilibrium is stationarj- in value when 
the type is normal. We might prove this from the original 
equations of vibration, but it will be more convenient to employ 
the normal co-ordinates. The constraint, which may be supposed 
to be of such a character as to leave only one degree of freedom, is 
represented by taking the quantities in gfven ratios. 

If we put 

i>,^A,0, <^, = il,^,&c (1), 

d is a variable quantity, and Ai, A^, &c. are given for a given con- 

The expressions for T and V become 

r={K^i«+iMa»+ }^^ 

Vr={^c^Ai^ + ^cM+ }^, 

1 Thomson and Tait, 2nd edition, § 343 7;i. 
3 St Petenb, Acad, Sci, M6m. x. 1859. 

' Stability of Motion (Adams Prize Essay for 1877). See also Bouth*8 Rigid 
Dyfiamiet, 5th edition, 1892. 

* Proceedingt of the Mathematical Society, June, 1873. 

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whence, if 6 varies as cos pt, 

This gives the period of the vibration of the constrained type ; 
and it is evident that the period is stationary, when all but one of 
the coefficients -4i,ilj, ... vanish, that is to say, when the tj'pe 
coincides with one of those natural to the system, and no constraint 
is needed. 

[In the foregoing statement the equilibrium is supposed to be 
thoroughly stable, so that all the quantities c are positive. But 
the theorem applies equally even though any or all of the c*s be 
negative. Only if j^ itself be negative, the period becomes 
imaginary. In this case the stationary character attaches to the 
coefficients of ^ in the exponential terms, quantities which measure 
the degree of instability. 

Corresponding theorems, of importance in other branches of 
science, may be stated for systems such that only T and -P, or only 
Fand Fy are sensible ^ 

The stationary property of the roots of Lagrange's determinant 
(3) § 84, suggests a general method of approximating to their 
values. Beginning with assumed rough approximations to the 

ratios A^-.A^iA^ we may calculate a first approximation to 

jf from 

^^iaii^i' + iaa^»+... + aiA^,+ ... ^^' 

With this value of p* we may recalculate the ratios A^xA^.,. from 
any (m — 1) of equations (5) § 84, then again by application of (3) 
determine an improved value of p', and so on.] 

By means of the same theorem we may prove that an increase 
in the mass of any part of a vibrating system is attended by a 
prolongation of all the natural periods, or at any rate that no 
period can be diminished. Suppose the increment of mass to be 
infinitesimal. After the alteration, the types of free vibration will 
in general be changed ; but, by a suitable constraint, the system 
may be made to retain any one of the former types. If this be 
done, it is certain that any vibration which involves a motion of 
the part whose mass has been increased will have its period 
prolonged. Only as a particular case (as, for example, when a 
load is placed at the node of a vibrating string) can the period 

^ Brit. Asi. Rep. for 1S85, p. 911. 

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remain unchanged. The theorem now allows us to sissert that 
the removal of the constraint, and the consequent change of type, 
can only affect the period by a quantity of the second order ; and 
that therefore in the limit the &ee period cannot be less than 
before the change. By integration we infer that a finite increase 
of mass must prolong the period of every vibration which involves 
a motion of the part affected, and that in no case can the period 
be diminished ; but in order to see the correspondence of the two 
sets of periods, it may be necessary to suppose the alterations 
made by steps. Conversely, the effect of a removal of part of 
the mass of a vibrating system must be to shorten the periods 
of all the free vibrations. 

In like manner we may prove that if the system undergo such 
a change that the potential energy of a given configuration is 
diminished, while the kinetic energy of a given motion is unaltered, 
the periods of the free vibrations ai*e all increased, and conversely. 
This proposition may sometimes be used for tracing the effects of 
a constraint; for if we suppose that the potential energy of 
any configuration violating the condition of constraint gradually 
increases, we shall approach a state of things in which the 
condition is observed with any desired degree of completeness. 
During each step of the process every free vibration becomes 
(in general) more rapid, and a number of the free periods (equal 
to the degrees of liberty lost) become infinitely small. The 
same practical result may be reached without altering the po* 
tential energy by supposing the kinetic energy of any motion 
violating the condition to increase without limit. In this case 
one or more periods become infinitely large, but the finite 
periods are ultimately the same as those arrived at when the 
potential energy is increased, although in one case the periods 
have been throughout increasing, and in the other diminishing. 
This example shews the necessity of making the alterations by 
steps; otherwise we should not understand the correspondence 
of the two sets of periods. Further illustrations will be given 
under the head of two degrees of freedom. 

By means of the principle that the value of the free periods 
is stationary, we may easily calculate corrections due to any 
deviation in the system from theoretical simplicity. If we take 
as a hypothetical type of vibration that proper to the simple 
system, the period so found will differ fi'om the truth by quan- 
tities depending on the squares of the irregularities. Several 

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examples of such calculations will be given in the course of 
this work. 

89. Another point of importance relating to the period of a 
system vibrating in an arbitrary type remains to be noticed. 
It appears from (2) § 88, that the period of the vibration cor- 
responding to any hypothetical type is included between the 
greatest and least of those natural to the system. In the case 
of systems like strings and plates which are treated as capable 
of continuous deformation, there is no least natural period; 
but we may still assert that the period calculated from any hypo- 
thetical type cannot exceed that belonging to the gravest normal 
type. When therefore the object is to estimate the longest 
proper period of a system by means of calculations founded 
on an assumed t3rpe, we know a priori that the result will come 
out too small. 

In the choice of a hypothetical type judgment must be 
used, the object being to approach the truth as nearly as can 
be done without too great a sacrifice of simplicity. Thus the 
type for a string heavily weighted at one point might suitably 
be taken from the extreme case of an infinite load, when the 
two parts of the string would be straight. As an example of 
a calculation of this kind, of which the result is known, we 
will take the case of a uniform string of length I, stretched 
with tension Ti, and inquire what the period would be on 
certain suppositions as to the type of vibration. 

Taking the origin of a at the middle of the string, let the 
curve of vibration on the positive side be 

y = co8p<|l-(^)"| (1). 

and on the negative side the image of this in the axis of y, 
* n being not less than unity. This form satisfies the conditioa 
that y vanishes when a? = ± JZ. We have now to form the ex- 
pressions for T and V, and it will be sufficient to consider the 
positive half of the string only. Thus, p being the longitudinal 

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2(n+l)(2n+l) 2\ 
2n-l 'pi*' 


If n = 1, the string vibrates as if the mass were concentrated 
in its middle point, and 


If n = 2, the form is parabolic, and 

The true value of p^ for the gravest type is — j^ , so that 

the assumption of a parabolic form gives a period which is too 
small in the ratio ir : »J 10 or '9936 : 1. The minimum of p*, 
as given by (2), occurs when n = J (V6 + 1) = 1*72474, and gives 

©« = 9-8990^,. 

The period is now too small in the ratio 

TT : >/9^8990 = '99851 : 1. 

It will be seen that there is considerable latitude in the 
choice of a type, even the violent supposition that the string 
vibrates as two straight pieces giving a period less than ten 
per cent, in error. And whatever type we choose to take, the 
period calculated from it cannot be greater than the truth. 

[In the above applications it is assumed that there are no 
unstable modes. When unstable modes exist, the statement is 
that a constrained mode if stable possesses a frequency of vibra- 
tion less than that of the highest normal mode, and if unstable 
has a degree of instability less than that of the most unstable 
normal mode] 

90. The rigorous determination of the periods and types of 
vibration of a given system is usually a matter of great diflSculty, 
arising from the fact that the functions necessary to express the 
modes of vibration of most continuous bodies are not as yet recog- 
nised in analysis. It is therefore often necessary to fall back on 
methods of approximation, refening the proposed system to some 
other of a character more amenable to analysis, and calculating 
corrections depending on the supposition that the difference be- 
tween the two systems is small. The problem of approximately 
R. 8 

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••} (1), 


simple systems is thus one of great importance, more especially 
as it is impossible in practice actually to realise the simple forms 
about which we can most easily reason. 

Let us suppose then that the vibrations of a simple system are 
thoroughly known, and that it is required to investigate those 
of a system derived from it by introducing small variations in 
the mechanical functions. If ^, <^3, &c. be the normal co-ordi- 
nates of the original system, 

and for the varied system, referred to the same co-ordinates, 
which are now only approximately normal, 

F+SF=i (ci + Scn) <^»+ ... + Sc,0,<^+ . 
in which Sa^, Soi,, Scu, Scia, &c. are to be regarded as small 
quantities. In certain cases new co-ordinates may appear, but 
if so their coefficients must be small. From (1) we obtain for the 
Lagrangian equations of motion, 

(ar+~Sa„ Z)« + Ci + Scn) (fh + (Ba^.2l> + Sc„) ^2 ' 

(&Zai)« + &M)<^ + (a, + Saa2)* + c, + Sc^)02 )- (2)- 

In the original system the fundamental .types of vibration 
are those which correspond to the variation of but a single co- 
ordinate at a time. Let us fix our attention on one of them, 
involving say a variation of <j>r, while all the remaining co- 
ordinates vanish. The change in the system will in general 
entail an alteration in the fundamental or normal types; but 
under the circumstances contemplated the alteration is small. 
The new normal type is expressed by the synchronous variation 
of the other co-ordinates in addition to 0^ ; but the ratio of any 
other <f)g to <f>r is small. When these ratios are known, the normal 
mode of the altered system will be determined. 

Since the whole motion is simple harmonic, we may suppose 
that each co-ordinate varies as cosjOr^, and substitute in the 
differential equations —pr^ for i>*. In the «'** equation 0^ occurs 
with the finite coefficient 

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The coefficient of ^^ is 

The other terms are to be neglected in a first approximation, 
since both the co-ordinate (relatively to 0r) and its coefficient are 
small quantities. Hence 

*-*-- cr-^.«a. (^>- 

Now - a,p,* + c, = 0, 

and thus 0, : ^ ^ P^'f^""^ ^ (4) 

the required result. 

If the kinetic energy alone undergo variation, 

*' = '^'"^7^'-^~ ^'^ 

The corrected value of the period is determined by the rth 
equation of (2), not hitherto used. We may write it, 

Substituting for ^, : (f>r from (4), we get 

a ^ Cr + 8Crr y (^Crg -pr^'JarMy rr.. 

P' Or + SOrr a^(p,'^Pr') ^''^• 

The first term gives the value of pr^ calculated without allow- 
ance for the change of type, and is sufficient, as we have already 
proved, when the square of the alteration in the system may 
be neglected. The terms included under the symbol 2, in 
which the summation extends to all values of 8 other than r, 
give the correction due to the change of type and are of the 
second order. Since a, and Or are positive, the sign of any term 
depends upon that oi p^—pr^ If pg^>pr^, that is, if the mode 
s be more acute than the mode r, the correction is negative, 
and makes the calculated note graver than before; but if the 
mode 8 be the graver, the correction raises the note. If r refer 
to the gravest mode of the system, the whole correction is 
negative ; and if r refer to the acutest mode, the whole correction 
is positive, as we have already seen by another method. 

91. As an example of the use of these formula, we may 
take the case of a stretched string, whose longitudinal density p 
is not quite constant. If x be measured from one end, and y 


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be the transverse displacement, the configuration at any time t 
will be expressed by 

y = <^8iny 4-<^8in-j-+<^3 8xn y + (1), 

I being the length of the string. ^, 02,*.. are the normal 
co-ordinates for /9 = constant, and though here p is not strictly 
constant, the configuration of the system may still be expressed 
by means of the same quantities. Since the potential energy 
of any configuration is the same as if p = constant, SV==^0, For 
the kinetic energy we have 

T + Sr = ijV(*i8in^ + <^,sin?p' + ...yAr 

a=4<^i" I psin"-=-da7 + i<^j* I psin'-v dx+... 
Jo ^ .' ^ 

, 1 1 [^ . Tra? . 2irx , . 
+ <pi9a I psin-T-sm— p cw? + .... 

If p were constant, the products of the velocities would 
disappear, since <^, ^, &c. are, on that supposition, the normal 
co-ordinates. As it is, the integral coefficients, though not actually 
evanescent, are small quantities. Let p = po-^- Bp] then in our 
previous notation 

«r = JVo> oarr= / op sui* — p cwj, oa„ = I Op sm -r- sm -y- rfd:. 

Thus the type of vibration is expressed by 

or, since pr' - P8^ = i^ i ^, 

. . r* f^2Sp . rTra? . sirx , .^. 

<>' •■ -^"^^ Jol^"'°-2 ^^°— '^ <2>- 

Let us apply this result to calculate the displacement of the 
nodal point of the second mode (r = 2), which would be in the 
middle, if the string were uniform. In the neighbourhood of 
this point, if x — ^l-hBx, the approximate value of y is 

y^^^ism^ +<^,8m-2- + <^s8m-2-+... 
7^ . TT 27r , 27r . ) 

TT , 


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91.] EXAMPLES. 117 

Hence when y = 0, 

^'=^J4>i-'h+ <!>.-- ] (3) 

approximately, where 

To shew the application of these formulae, we may suppose 
the irregularity to consist in a small load of mass p^ situated 
B,t x^H, though the result might be obtained much more easily 
directly. We have 

e. _ 2X f 2 2 2_ 2_ \ 

7rV2|P-4 8»-4 5«-4"^7«-4"^ J' 

from which the value of Sx may be calculated by approximation. 
The real value of Bx is, however, very simple. The series within 
brackets may be written 

which is equal to 




ol + x* 
The value of the definite integral is 

TT -f- 4 sm J *, 

J *!. t 2X 7rV2 X 

as may also be readily proved by equating the periods of vibra- 
tion of the two parts of the string, that of the loaded part being 
calculated approximately on the assumption of unchanged type. 

As an example of the formula (6) § 90 for the period, we 
may take the case of a striug carrying a small load p^ at its 
middle point. We have 

ar = i/p», Sa^ = poXsin«-2-, &v, = poX sin -g- 81^-2"' 

and thus, if P^ be the value corresponding to \ = 0, we get when 
r is even, pr — Pr, and when r is odd, 

1 Todhnnter'8 Int, Calc, § 255. 

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where the summation is to be extended to all the odd values 
of 8 other than r. If r = 1, 

Now 22--!— = 2 ^,-2 ^ 

V-1 8-1 8+V 

in which the values of » are 3, 5, 7, 9.... Accordingly 

v_L -1 

and p,. = P..|i_^ + ^V I (6). 

giving the pitch of the gravest tone accurately as far as the 
square of the ratio X : l. 

In the general case the value of p^, correct as far as the first 
order in 8p, will be 


92. The theory of Vibrations throws great light on expansions 
of arbitrary functions in series of other functions of specified 
typea The best known example of such expansions is that 
generally called after Fourier, in which an arbitrary periodic 
function is resolved into a series of harmonics, whose periods 
are submultiples of that of the given function. It is well known 
that the difficulty of the question is confined to the proof of the 
possibility of the expansion ; if this be assumed, the determination 
of the coefficients is easy enough. What I wish now to draw 
attention to is, that in this, and an immense variety of similar 
cases, the possibility of the expansion may be inferred fix>m 
physical considerations. 

To fix our ideas, let us consider the small vibrations of a 
uniform string stretched between fixed points. We know fix>m' 
the general theory that the whole motion, whatever it may 
be, can be analysed into a series of component motions, each 
represented by a harmonic function of the time, and capable 
of existing by itself. If we can discover these normal types, 
we shall be in a position to represent the most general vibration 
possible by combining them, assigning to each an arbitrary 
amplitude and phase. 

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Assuming that a motion is harmonic with respect to time^ 
we get to determine the type an equation of the form 

whence it appears that the normal functions are 

. irx 
y = sm-^, 


y = 8in 


, &c. 

We infer that the most general position which the string can 
assume is capable of representation by a series of the foim 

. . irx . . 27rx . . Zirx 
Ai sm -J- + Ai sm —j— + -4, sm -j — h 

which is a particular case of Fourier's theorem. There would 
be no diflSculty in proving the theorem in its most general form. 

So far the string has been supposed uniform. But we have 
only to introduce a variable density, or even a single load at 
any point of the string, in order to alter completely the ex- 
pansion whose possibility may be inferred from the dynamical 
theory. It is unnecessary to dwell here on this subject, as 
we shall have further examples in the chapters on the vibrations 
of particuhu* systems, such as bars, membranes, and confined 
masses of air. 

92 a. In § 88 we have a formula for the frequency of vibration 
applicable when by the imposition of given constraints the original 
system is left with only one degree of freedom. It is of interest 
to trace also the effect of less complete constraints, such as may 
be expressed by linear relations among the normal co-ordinates of 
number less by at least two than that of the (original) degrees of 
freedom. Thus we may suppose that 

9i<t>i+92<t>i-^g3<l>s + ... = 

Ai^i + Aa<^a + ^8^8 + ... = 


If the number of equations (r) fall short of the number of the 
degrees of freedom by unity, the ratios ^i:^s:^8... are fully 
determined, and the case is that of but one outstanding degree of 
freedom discussed in § 88. 

This problem may be treated in more than one way, but the 

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most instructive procedure is to trace the effect of additions to T 
and F. We will suppose that equations (1) § 87 are altered to 

r=K<^* + ia,<^a» + ...+ia(/,<^4./.(^,+ ...)* (2), 

7 = icA* + ic^.' + ... + i7(/A+/.^ + ...)" (3), 

and that F, not previously existent, is now 

F^1ifi{A<k+M.+ '")'-' (4). 

The connection with the proposed problem will be understood 
by supposing for instance that a = 0, )8 = 0, while 7 = oo . By (3) 
the potential energy of any displacement violating the condition 

/A+/A+...=0 (5) 

is then infinite, and this is tantamount to the imposition of the 
constraint represented by (5). 

Lagrange's equations with X written for D now become 


If we multiply the first of these by/i/(aiX"+ c^), the second by 

/^(OjX* -t- Ca), and so on, and add the results together, the factor 

(fi<i>i-^fi<f>i+ '*-) will divide out, and the determinant takes the 


f^ J. f^ 4. _i_ z = n\ 

(hX'-^C a^\^ + c^^ ^aX» + /3X + 7 ^ ^' 

If any one of the quantities a, )8, 7 become infinite while the 
others remain finite, the effect is equivalent to the imposition of the 
constraint (5), and the result may be written 

2/V(aX« + c) = (8V. 

When multiplied out this equation is of degree (m— 1) in X*, one 
degree of freedom having been lost. 

If we put J3 = 0y (7) is an equation of the mth degree in X', and 
the coefficients a, 7 enter in the same way as do Oi, Cj; a„ c,; &c. 

In order to refer more directly to the case of vibrations about 
stable equilibrium, we will write p* for — XI The values of p* 
belonging to the unaltered system, viz. n^^ Wj',..., are given as 
before by 

Ci — air?^*=0, Cs — as722* = 0, &c., (9); 

and we will also write 

7-ai/« = (10), 

1 Bouth'B Rigid Dynamics, 5th edition, 1892, § 67. 

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92 a.] ONE CX)NSTRAINT. 121 

where i/* relates to the supposed additions to T and V considered 
as belonging to an independent vibrator. Let the order of magni- 
tude of these quantities be 

^*.W,«, nr\t^y7ir+i\ ^* (11). 

We shall see that there is a root of (7) between each consecutive 
pair of the quantities (11). 

Our equation may be written 




+ (Ci — OiP") (Ca — OaP') = (12). 

When p^ coincides with any of the quantities (11), all but one 
of the terms in (12) vanish, and the sign of the expression is the 
same as that of the term which remains over. When p* < w,*, all 
the terms are positive, so that there is no root less than ni\ 
When p^ = V, the expression (12) reduces to the positive quantity 

/i« (7 - aV) (c - Ojni^) (Cs - ajTii') 

When p^ rises to Wj', (12) becomes 

/,«(7~ aw,«) (Ci- aiw,0(ca-a,72,«) ; 

and this is negative, since the factor (ci — OiW,*) is now negative. 
Hence there is a root of (12) between %" and n,*. When jp«= Wj«, 
the expression is again positive, and thus there is a root between 
n,* and n,* This argument may be continued, and it proves that 
there is a root of (12) between any consecutive two of the (m + 1) 
quantities (11). The m roots of (12) are now accounted for, and 
there is none greater than rim^. If we compare the values of the 
roots before and after the change, we see that the effect is to 
cause a movement which is in every case towards 1^.^ Considered 
absolutely the movement is in one direction for those roots that 
are greater than v^ and in the opposite direction for those that 
are less than 1^. Accordingly the interval from n^ to Wr+i', in 
which v^ lies, contains after the change two roots, one on either 
side of 1^. 

If 1^ be less than any of the quantities n*, as happens when 
7 = 0, one root lies between 1^ and Wj*, one between n^ and r^*, and 
so on. Thus every root is depressed. On the other hand if 
v" > n^, every root is increased. This happens if a = 0. (§ 88.) 

^ It will be understood that in particular cases the movement may vanish. 

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The results now arrived at are of course independent of the 
special machinery of normal co-ordinates used in the investigation* 

If to any part of a system (wi', n^ ) be attached a vibrator 

(v*) having a single degree of freedom, the eflFect is to displace all 
the quantities nl^ ... in the direction of i^. Let us now suppose 
that a second change is made in the vibrator whereby a becomes 
a + a^ and 7 becomes 7 + 7'. Every root of the determinantal 
equation moves towards l/'^ where 7' — aV = 0. If we suppose 
that v^ = V*, the movements are in all cases in the same directions 
as before. Going back now to the original system, and supposing 
that a, 7 grow from zero to their actual values in such a manner 
that 1^ remains constant, wet see that during this process the roots 
move without regression in the direction of closer agreement 
with I/*. 

As a and 7 become infinite, one root of (12) moves to coinci- 
dence with I/", while the remaining (m— 1) roots, corresponding to 
the constrained system, are given by 

2/V(c-a;)0 = (13), 

and are independent of the value of i/*. 

Particular cases are obtained by supposing either i/* = 0, or 
j;» = 00 . Whether the constraint is eflFected by making infinite 
the kinetic energy of any motion, or the potential energy of 
any displacement, which violates it, makes no diflference to the 
vibrations which remain. In the first case one vibration becomes 
infinitely slow, and in the second case one becomes infinitely quick. 
However the constraint be arrived at, the (m— 1) frequencies of 
vibration of the constrained system sefparate^ the m frequencies 
of the original system. 

Any number of examples of this theorem may be invented 
without diflBculty. Consider the case of a uniform stretched 
string, held at both ends and vibrating transversely. This is the 
original system. Now introduce a constraint by holding at rest a 
point which divides the length in the proportion (say) of 3 : 2. 
The two parts vibrate independently, and the frequencies for each 
part form an arithmetical progression. If the frequencies proper 
to the undivided string be 1, 2, 3, 4 ; those for the parts are 

^ But in particular cases the " separation " may vanish. The theorem in the 
text was proved for two degrees of freedom in the first edition of this work. In 
its generality it appears to be due to Bouth. 

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92 a.] ONE CONSTRAINT. 123 

f (1, 2, 3, ...) and f (1, 2, 3, ...). The beginning of each series is 
shewn in the accompanying scheme ; 

and it will be seen that between any consecutive numbers in 
the first row there is a number to be found either in the second 
or in the third row. In the case of 5 and 10 we have an extreme 
condition of things ; but the slightest displacement of the point 
at which the constraint is applied will displace one of the fives, 
tens &c. to the left And the other to the right. 

The coincidences may be avoided by dividing the string 
incommensurably. Thus, if x be an incommensurable number 
less than unity, one of the series of quantities m/x, m/(l — a?), where 
m is a whole number, can be found which shall lie between any 
given consecutive integers, and but one such quantity can be found. 

Again, let us suppose that a system is referred to co-ordinates 
which are not normal (§ 84), and let the constraint represented by 
-^1=8 be imposed. The determinant of the altered system is 
formed from that of 'the original system by erasing the first row 
and the first column. It may be called Vj, and from this again 
may be formed in like manner a new determinant V,, and so on. 
These determinants form a series of functions of p*, regularly 
decreasing in degree; and we conclude that the roots of each 
separate the roots of that immediately preceding^ 

It may be remarked that while for the sake of simplicity of 
statement we have supposed that the equilibrium of the original 
system was thoroughly stable, as also that of the vibration brought 
into connection therewith, these restrictions may easily be 
dispensed with. In any case the series of positive and negative 

quantities, Wi*, n,", and i^, may be arranged in algebraic order, 

and the effect of the vibrator is to cause a movement of every 
value of jp* in the direction of i/*. 

In order to extend the above theory we will now suppose that 
the addition to 7 is 

+ iaA(Ai<*>i + Ma+...)'+ (14) 

^ Boath*B Rigid Dynamics, 5th edition, Part ii. § 58. 

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.) + ... = 0...(17). 


and the addition to V 

H (/i<th +M, + ...)» + H (S-.^ + <7W>. + •••)• + 
If we set 

a/V + 7/=-f", a,V+7„=<?', 

and so on, Lagrange's equations become 

(oiX.' + c.) ^ + F'f, if, in +/.^ + . 
+ O'gi (g'i«^ + ^.<^ + -.) + S% (hi<fh + A^ + 

(a,\» + c) ^ + F% {/^ +/,^ + . . .) 
+ <?'<7.(5'i^ +5'*^+ ...) + H% (A.<^, + A,^ + ...) + ... = 0...(18), 
and 80 on, the number of equations being equal to the number 
(m) of co-ordinates ^, ^ .... The number of additions (r), corre- 
sponding to the letters/, g,h,...,ia supposed to be less than m. 

From the above m equations let r new ones be formed, as 
follows. For the first multiply (17) by /,/(o,X' + c,), (18) by 
/,/(a^' + c), and so on, and add the results together. For the 
second proceed in the same manner, using the multipliers 
giKih^* + <h), ffi/(<h^* + Ct), &c. In like manner for the third 
equation use h instead of g, and so on. In this way we obtain r 
equations which may be written 

F' {fA +/A + • • •) IV-f" + F^' + ^.' + ^.' +• . .} 

+ 0' ($i<f>i +g.<t>»+ ...) {F^Gr + F,G, + ...} 

+ H'(lH<l>,-i-h,ip,+ ...){F,H^ + FJI,+ ...} + =0...(19), 

F'(fr<k-^f^ + ...){G,F^ + GJ',+ ...} 
4 G' ig,4>, -h <7,^ + . . .) {1/G' + G,» +(?,» + .. .} 

+ fr'(A,^-t-A,^ + ...){(?,ff,-l-(?.ff. + ...}-l- =0...(20). 

and so on, where for brevity 

F,' = /.V(axX' -I- c,). Fi =UI{ais? + c,), Ac, «| 

F,Gr=f^gJ{a,\' + c,). &c. J 

The determinantal equation, of the rth order, is thus 
l/F' + tF*, ^FG. tFH,. 

1FG,1/G' + 2G', tGH, 

1.FH, IGH, 1/H' + 1H\ . 

= 0. 


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92 a.] 



If, for example, there be two additions to T and V of the kind 
prescribed, the equation is 

js^ + ^ + -^+2i*.2(?«-{2i'^}» = (23), 

and herein 

(i\» + j;'+ ...) (Gx» +(?,»+...)- (^i(?i + ^.<?. + ...)' 

= -2,l.{F,G,-F,G,y ^24). 

Equation (23) is in general of the mth degree in X*, and 
determines the frequencies of vibration. In the extreme case 
where F' and 0' are made infinite, the system is subject to the 
two constraints 

/.^+/,^+ ... = 0) , 

«7x<^ + «ir.*,+ "=0j ^^*'''' 

and the equation ' giving the (m — 2) outstanding roots is 
(/ig«-/«yi)' (/ig»-/«gi)* 

= 0. 


(a,X» + <h) (a,V + c) "^ (oiX' + c,) (a,X» + c.) 

In general if the system be subject to the r constraints (1), the 
determinantal equation is 

IFF, IFO, -ZFH,... 
1.F0, IGG, 20H.... 
IFH, I.OH. IHH,... 



If r be less than m, this determinant can be resolved* into a 
sum of squares of determinants of the same order (r). Thus if there 
be three constraints, the first of these squares is 

F^ F^ F^ » 

ffi G, (?, (28), 

Hi H^ Hi 

and the others are to be found by including every combination of 
the m suffixes taken three together. To fall back upon the original 
notation we have merely in (28) to replace the capital letters 
F, 0,... by/, g,..., and to introduce the denominator 

(oiX* + Ci) (OaX' + c,) (a,X> + C3). 

The determinantal equation for a system originally of m degrees 
of freedom and subjected to r constraints is thus found. Its form 

1 Thils result is due to Bouth, loe, cit, § 67. 
* Salmon, Lessons on HigJier Algebra^ § 24. 

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[92 a. 

is largely determined by the consideration that it must remain un- 
affected by. interchanges either of the letters or of the suffixes. 
That it would become nugatory if two of the conditions of con- 
straint coincided, could also have been foreseen. If r = m — 1, 
the system is reduced to one degree of freedom, and the equation 

g% g» 94'" 

A, A, A4... 



9i 9* 9i"* 
hi As A4... 

.(o^' + c)- 


in agreement with § (88). 

There are theories, parallel to the foregoing, for systems in 
which T and jP, or V and P, are alone sensible. In these cases, if 
the functions be intrinsically positive, the normal motions are 
proportional to exponential functions of the time such as er*^\ 
The quantities Tj, t,,... are called the time-constants, or persis- 
tences, of the motions, being the times occupied by the motions in 
subsiding in the ratio of e : 1. The new persistences, after the 
introduction of a constraint, will separate the original values. ^ 

The best illustrations of this theory are electrical, where the 
motions are not restricted to be small. Suppose (to take an 
electro-magnetic example) that in one branch of a net-work of 
conductors there is introduced a coil of persistence (when closed 
upon itself) equal to •/, the original persistences being Ti, Tj,.... 
Then the new persistences lie in all cases nearer to r, and they 
separate the quantities t\ Ti, T3.... If t' be made infinite as by 
increasing the self-induction of the additional coil without limit, 
or be made to vanish as by breaking the contact in the branch, 
the result is a constraint, and the new values of the persistences 
separate the former onea 

93. The determination of the coefficients to suit arbitrar}' 
initial conditions may always be readily effected by the funda- 
mental property of the normal functions, and it may be convenient 
to sketch the process here for systems like strings, bars, mem- 
branes, plates, &c. in which there is only one dependent variable 
(I* to be considered. If 1^1,1^^... be the normal functions, and 
■^, ^ ... the corresponding co-ordinates. 

f=<^it*i + <^l«s-f <^,M,+ . 


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The equations of free motion are 

^ + wi'^ = 0, ^, + n,»<^, = 0,&c. 
of which the solutions are 

<l>i = Ai sin flit + B1CO8 flit 
^ = 4a sin n,^ + -Bj cos nj; 




The initial values of f and ^ are therefore 

C = Biu, + 5jw, + 5,^, + ... I 


and the problem is to determine Ai, A^,... Bi, ^, ... so as to 
correspond with arbitrary values of (fo c^nd ^o- 

It pdxhe the mass of the element dw, we have from (1) 

= ^4>i^lptii*dx + ^^2^jpu^^dx + ... + ^^il 

But the expression for T in terms of ^, <^j, &c. cannot contain 
the products of the normal generalized velocities, and therefore 
every integral of the form 




Hence to determine Br we have only to multiple the first 
of equations (4) by pUr and integrate over the system. We thus 

BrjpUr^dx^ jpUr^ifiUc (6). 

Similarl}', nrArlpUr*dx=: jpii,t4^ 0)- 

The process is just the same whether the element dx he bl line, 
area, or volume. 

The conjugate property, expressed by (5), depends upon the 
fact that the functions u are normal. As soon as this is known 
by the solution of a differential equation or otherwise, we may 
infer the conjugate property without further proof, but the pro- 
perty itself is most intimately connected with the fundamental 
variational equation of motion § 94. 

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I V 


94 If 7 be the potential energy of deformation, f the 
displacement, and p the density of the (line, area, or volume) 
element dx, the equation of virtual velocities gives immediately 


jp'tS^dx^O (1), 

In this equation 87 is a symmetrical function of ^ and B^, 
as may be readily proved from the expression for V in terms 
of generalized co-ordinates. In fact if 

Suppose now that f refers to the motion corresponding to 
a normal function t^, so that tJ + Wr*f=0, while Sf is identified 
with another normal function u, ; then 

SK=n^* iplLrU^, 

Again, if we suppose, as we are equally entitled to do, that f 
varies as a, and Sf as i/r, we get for the same quantity 87, 

and therefore 

(nr^-n,^)jpurv^ = (2), 

from which the conjugate property follows, if the motions re- 
presented respectively by t*r ai^d Ug have different periods. 

A good example of the connection of the two methods of 
treatment will be found in the chapter on the transverse vibrations 
of bars. 

96. Professor Stokes^ has drawn attention to a very general 
law connecting those parts of the free motion which depend 
on the initial displacements of a system not subject to frictional 
forces, with those which depend on the initial velocities. If 
a velocity of any type be communicated to a system at rest, 
and then after a small interval of time the opposite velocity 
be communicated, the effect in the limit will be to start the 
system without velocity, but with a displacement of the corre- 
sponding type. We may readily prove from this that in order 

1 Dynamical Theory of Diffraction, Cambridge Trans, Vol. «. p. 1, 1866. 


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to deduce the motion depending on initial displacements from 
that depending on the initial velocities, it is only necessary to 
diflFerentiate with respect to the time, and to replace the arbitrary 
constants (or functions) which express the initial velocities by 
those which express the corresponding initial displacements. 
Thus, if <f> be any normal co-ordinate satisfying the equation 

the solution in terms of the initial values of <f> and ^ is 

^ ^ <f>ocos nt + - ^oBin nt (1), 


of which the first term may be obtained from the second by 
Stokes' rule. 


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96. When dissipative forces act upon a system, the character 
of the motion is in general more complicated. If two only of the 
functions T, F, and V be finite, we may by a suitable linear trans- 
formation rid ourselves of the products of the co-ordinates, and 
obtain the normal types of motion. In the preceding chapter we 
have considered the case of ^= 0. The same theory with obvious 
modifications will apply when 7 = 0, or F = 0, but these cases 
though of importance in other parts of Physics, such as Heat and 
Electricity, scarcely belong to our present subject. 

The presence of Motion will not interfere with the reduction of 
T and V to sums of squares ; but the transformation proper for 
them will not in general suit also the requirements of F, The 
general equation can then only be reduced to the form 

ai$i + 6u<^i + 6i2<^2 + ... +Ci<^i = <!>!, &c (1), 

and not to the simpler form applicable to a system of one degree 
of freedom, viz. 

ai<^i + &i^ + c,<^ = *i. &c (2). 

We may, however, choose which pair of functions we shall 
reduce, though in Acoustics the choice would almost always fall 
on T and V. 

97. There is, however, a not unimportant class of cases in 
which the reduction of all three functions may be effected; and 
the theory then assumes an exceptional simplicity. Under this head 
the most important are probably those when ^ is of the same form 
as T or F. The first case occurs fi-equently, in books at any rate, 
when the motion of each part of the sjrstem is resisted by a re- 
tarding force, proportional both to the mass and velocity of the 

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part. The same exceptional reduction is possible when ^ is a 
linear function of T and F, or when T is itself of the same form as 
y. In any of these cases, the equations of motion are of the same 
form as for a system of one degree of freedom, and the theory 
possesses certain peculiarities which make it worthy of separate 

The equations of motion are obtained at once from T, F 
and F:— 

aifiH-6i<^i + Ci<^i = *i, ) 

o^ + h^^ + c,^, = <E>„ &c. j 

in which the co-ordinates are separated. 

For the free vibrations we have only to put O^ = 0, &c., and 
the solution is of the form 

^ = e-^ |<^, ^^* + 4>, (co8«'« + ^, sin n'«)| (2), 

where K — hja, n*=^c/a, n' =^»J{n^-'\Kp), 

and ^0 aiid ^q are the initial values of 4> and (^. 

The whole motion may therefore be analysed into component 
motions, each of which corresponds to the variation of but one 
normal co-ordinate at a time. And the vibration in each of these 
modes is altogether similar to that of a system with only one 
degree of liberty. After a certain time, greater or less according 
to the amount of dissipation, the free vibrations become insignifi- 
cant, and the system returns sensibly to rest. 

[If F be of the same form as T, all the values of k are equal, 
viz. all vibrations die out at the same rate.] 

Simultaneously with the free vibrations, but in perfect inde- 
pendence of them, there may exist forced vibrations depending on 
the quantities 4>. Precisely as in the case of one degree of free- 
dom, the solution of 

a^ + 6<^ + c<^ = <l> (3) 

may be written 

<^ = i /"%-**<'-«') sin n'(«-0<I>d«' (4X 

where as above 

K = 6/a, n* = cja, n' == tj(n^ — i /c"). 
To obtain the complete expression for <\> we must add to the 
right-hand member of (4), which makes the initial values of <f> 
and ^ vanish, the terms given in (2) which represent the residue 


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at time t of the initial values ^o and <^o* If there be no frictioo, 
the value of <f> in (4) reduces to 

<f> = ^j\inn(t-r)<S>df (5). 

98. The complete independence of the normal co-ordinates 
leads to an interesting theorem concerning the relation of the 
subsequent motion to the initial disturbance. For if the forces 
which act upon the sjrstem be of such a character that they do no 
work on the displacement indicated by S<^, then <I>i = 0. No such 
forces, however long continued, can produce any effect on the 
motion ^. If it exist, they cannot destroy it ; if it do not exist, 
they cannot generate it. The most important application of the 
theorem is when the forces applied to the system act at a node of 
the normal component <t>i, that is, at a point which the component 
vibration in question does not tend to set in motion. Two extreme 
cases of such forces may be specially noted, (1) when the force is 
an impulse, starting the system from rest, (2) when it has acted so 
long that the system is again at rest under its influence in a dis- 
turbed position. So soon as the force ceases, natural vibrations 
set in, and in the absence of friction would continue for an in- 
definite time. We infer that whatever in other respects their 
character may be, they contain no component of the type ^. This 
conclusion is limited to cases where T, F, V admit of simultaneous 
reduction, including of course the case of no friction. 

99. The formulae quoted in § 97 are applicable to any kind of 
force, but it will often happen that we have to deal only with the 
effects of impressed forces of the harmonic type, and we may then 
advantageously employ the more special formulae applicable to such 
forces. In using normal co-ordinates, we have first to calculate the 
forces ^1, *j, &c. corresponding to each period, and thence deduce 
the values of the co-ordinates themselves. If among the natural 
periods (calculated without allowance for friction) there be any 
nearly agreeing in magnitude with the period of an impressed 
force, the corresponding component vibrations will be abnormally 
large, unless indeed the force itself be greatly attenuated in the 
preliminary resolution. Suppose, for example, that a transverse 
force of harmonic type and given period acts at a single point of 
a stretched string. All the normal modes of vibration will, in 
general, be excited, not however in their own proper periods, but 

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in the period of the impressed force ; but any normal component, 
which has a node at the point of application, will not be excited. 
The magnitude of each component thus depends on two things : 
(1) on the situation of its nodes with respect to the point at which 
the force is applied, and (2) on the degree of agreement between 
its own proper period and that of the force. It is important to 
remember that in response to a simple harmonic force, the system 
will vibrate in general in all its modes, although in particular 
cases it may sometimes be sufficient to attend to only one of them 
as being of paramount importance. 

100. When the periods of the forces operating are very long 
relatively to the free periods of the system, an equilibrium theory 
is sometimes adequate, but in such a case the solution could 
generally be found more easily without the use of the normal 
co-ordinates. Bernoulli's theory of the Tides is of this class, and 
proceeds on the assumption that the free periods of the masses of 
water found on the globe are small relatively to the periods of the 
operative forces, in which case the inertia of the water might be 
left out of account. As a matter of fact this supposition is only 
very roughly and partially applicable, and we are consequently 
still in the dark on many important points relating to the tides. 
The principal forces have a semi-diurnal period, which is not suffi- 
ciently long in relation to the natural periods concerned, to allow 
of the inertia of the water being neglected. But if the rotation of 
the earth had been much slower, the equilibrium theory of the 
tides might have been adequate. 

A corrected equilibrium theory is sometimes useful, when the 
period of the impressed force is sufficiently long in comparison 
with most of the natural periods of a system, but not so in the 
case of one or two of them. It will be sufficient to take the case 
where there is no friction. In the equation 

a^-hc(^ = 4>, or ^ + w'<^ = 4>/a, 

suppose that the impressed force varies as cos pt Then 

<^ = 4>-ra(n»-p») (1). 

The equilibrium theory neglects jo» in comparison with n\ 
and takes 

t^ = <l)~an« (2). 

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Suppose now that this course is justifiable, except in respect 
of the single normal co-ordinate ^. We have then only to add 
to the result of the equilibrium theory, the difference between 
the true and the there assumed value of ^, viz. 

A ==__*!_ *L=^ *^ n\ 

The other extreme case ought also to be noticed. If the 
forced vibrations be extremely rapid, they may become nearly 
independent of the potential energy of the s}rstem. Instead 
of neglecting p" in comparison with n', we have then to neglect 
w" in comparison with p^, which gives 

^ = — <I>-4-ap* (4). 

If there be one or two co-ordinates to which this treatment 
is not applicable, we may supplement the result, calculated on 
the hypothesis that V is altogether negligible, with corrections 
for these particular co-ordinates. 

101. Before passing on to the general theory of the vibrations 
of systems subject to dissipation, it may be well to point out 
some peculiarities of the free vibrations of continuous systems, 
started by a force applied at a single point. On the suppositions 
and notations of § 93, the configuration at any time is deter- 
mined by 

?=<^i^ + ^2Wa+<^^+ (1), 

where the normal co-ordinates satisfy equations of the form 

aJi>r-^Cr^r^^r (2). 

Suppose now that the system is held at rest by a force applied 
at the point Q. The value of <I>r is determined by the considera- 
tion that ^f£<l>r represents the work done upon the system by the 
impressed forces during a hypothetical displacement S^^B<f>r'Ur, 
that is 

thus ^r^lZUrdx^UriQ)jZdx; 

80 that initially by (2) 

c^^Vr{Q)fzdx (3). 

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If the system be let go from this configuration at ^=^0, we 
have at any subsequent time t, 

Ur{Q)jZdx Ur{Q)jZdx 

<^^=cosr^i =cosM v. (*), 

*" n/ jp Ur^dx 

and at the point P 

f^ScosM . (5). 


At particular points v>r(P) and %'{Q) vanish, but on the 


neither converges, nor diverges, with r. The series for f therefore 
converges with 71^""'. 

Again, suppose that the system is started by an impulse 
from the configuration of equilibrium. In this case initially 

a^r^j^fdt = Ur (Q)jz,da:, 

whence at time t 

This gives 

<l>r=--—'Ur(Q)'\Zidx^ ^'IZ^dx (6), 


f =2sinn,i 

nr jpUr^dx 

shewing that in this case the series converges with Wr~^ that 
is more slowly than in the previous case. 

In both cases it may be observed that the value of ^ is 
symmetrical with respect to P and Q, proving that the displace- 
ment at time t for the point P when the force or impulse is ap- 
plied at Q, is the same as it would be at Q if the force or impulse 
had been applied at P. This is an example of a very general 
reciprocal theorem, which we shall consider at length presently. 

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As a third case we may suppose the body to start from rest 
as deformed by a force uniformly distributed, over its length, 
area, or volume. We readily find 

?=ScosM T-^ (8). 

V IpUr^dx 

The series for f will be more convergent than when the force 
is concentrated in a single point. 

In exactly the same way we may treat the case of a con- 
tinuous body whose motion is subject to dissipation, provided 
that the three functions T, F, V be simultaneously reducible, 
but it is not necessary to write down the formulae. 

102. If the three mechanical functions T, F and V of any 
system be not simultaneously reducible, the natural vibrations 
(as has already been observed) are more complicated in their 
character. When, however, the dissipation is small, the method 
of reduction is still useful ; and this class of cases besides being 
of some importance in itself will form a good introduction to 
the more general theory. We suppose then that T and V are 
expressed as sums of squares 

F = ic,^» + ic.0,« + ...J ^ ^' 

while F still appears in the more general form 

i^''=i6n<^i' + i6«<^,^ + ...+Mi*a+ (2). 

The equations of motion are accordingly 

Oi^i + bu^ 4- ftis^j + 6is<^3 + ... + Ci<l>i = I 

a,^8 + iii<^i + i«<^2 + 6a<^s+-.. +Ca(^2 = > (3), 

in which the coeflScients 6u, 6ia, &c. are to be treated as small. 
If there were no friction, the above system of equations would 
be satisfied by supposing one co-ordinate ^^ to vary suitably, 
while the other co-ordinates vanish. In the actual case there 
will be a corresponding solution in which the value of any other 
co-ordinate (f>g will be small relatively to <^y. 

Hence, if we omit terms of the second order, the r^ equation 

ar$r+6rr<^r+Cr<^r = (4), 

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from which we infer that <f>r varies approximately as if there 
-were no change due to friction in the type of vibration. If ^r 
vary as e*^, we obtain to determine pr 

arPr^-^brrPr + Cr^O (6). 

The roots of this equation are complex, but the real part 
is small in comparison with the imaginary part. [The character 
of the motion represented by (5) has already been discussed 
(§ 45). The rate at which the vibrations die down is proportional 
to brr, and the period, if the term be still admitted, is approxi- 
mately the same as if there were no dissipation.] 

From the sf"^ equation, if we introduce the supposition that 
all the co-ordinates vary as e^, we get 

(Pr'a. + Ct) <l>g + brsPr^r = 0, 

terms of the second order being omitted ; whence 

<^. : ^, b^^pr_^_br^pr_ ,g. 

This equation determines approximately the altered type 
of vibration. Since the chief part of pr is imaginary, we see 
that the co-ordinates <f>g are approximately in the same phase, 
but that that phase differs by a quarter period from the phase 
of ^r- Hence when the function F does not reduce to a sum 
of squares, the character of the elementary modes of vibration 
is less simple than otherwise, and the various parts of the system 
are no longer simultaneously in the same phase. 

We proved above that, when the friction is small, the value 
of Pr may be calculated approximately without allowance for 
the change of type ; but by means of (6) we may obtain a still 
closer approximation, in which the squares of the small quantities 
are retained. The r^^ equation (3) gives 

<^Pr'+Cr+b„Pr + t-^;^^^^0 '..... (7). 

The leading part of the terms included under 2 being real, 
the correction has no effect on the real paiij of pr on which 
the rate of decay c|iepends. 

102 a. Following the electrical analogy we may conveniently 
describe the forces expressed by jP as forces of resistance. In 
§ 102 we have seen that if the resistances be small, the periods 
are independent of them. We may therefore extend to this case 

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the application of the theorems with regard to the effect upon 
the periods of additions to T and F, which have been already 
proved when there are no resistances. 

By (5) § 102, if the forces of resistance be increased, the rates 
of subsidence of all the normal motions are in general increased 
with them; but in particular cases it may happen that there 
is no change in a rate of subsidence. 

It is natural to inquire whether this conclusion is limited to 
BmaJl resistances, for at first sight it would appear likely to hold 
good generally. An argument sufficient to decide this question 
may be founded upon a particular case. Consider a system formed 
by attaching two loads at any points of a stretched string vibrating 
transversely. If the mass of the string itself be neglected, there 
are two degrees of freedom and two periods of vibration corre- 
sponding to two normal modes. In each of these modes both loads 
in general vibrate. Now suppose that a force of resistance is 
introduced retarding the motion of one of the loads, and that this 
force gradually increases. At first the effect is to cause both kinds 
of vibration to die out and that at an increasing rate, but after- 
wards the law changes. For when the resistance becomes infinite, 
it is equivalent to a constraint, holding at rest the load upon which 
it acts. The remaining vibration is then unaffected by resistance, 
and maintains itself indefinitely. Thus the rate of subsidence of 
one of the normal modes has decreased to evanescence in spite of a 
continual increase in the forces of resistance F, This case is of 
course sufficient to disprove the suggested general theorem. 

108. We now return to the consideration of the general 
equations of § 84. 

If '^i* '^a* &C. be the co-ordinates and ^i, ^a, &c. the forces, 
we have 

where e^ = ar,l> + KsD + c„ (2). 

For the free vibrations ^i, &c. vanish. If V be the de- 

^1 , ^2 > • • • 

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the result of eliminating from (1) all the co-ordinates but one, is 

V^ = (4). 

Since V now contains odd powers of D, the 2m roots of the 
equation V=0 no longer occur in equal positive and negative 
pairs, but contain a real as well as an imaginary part. The 
complete integral may however still be written 

^ = -de^i« + ^>i'« + J5fl^« + 5'e^'« + (5), 

where the pcdrs of conjugate roots are /*!, An' ; /^, /^' ; &c. Corre- 
sponding to each root, there is a particular solution such as 

in which the ratios A^ : A^ : -4,... are determined by the equa- 
tions of motion, and only the absolute value remains arbitrary. 
In the present case however (where V contains odd powers of D) 
these ratios are not in general real, and therefore the variations 
of the co-ordinates -^i, yjr^y &c. are not synchronous in phase. If 
we put fh — ^i + i/^u /*i' = ai-*A, &c., we see that none of the 
quantities a can be positive, since in that case the energy of 
the motion would increase with the time, as we know it cannot 

103 a. The general argument (§§ 85, 103) from considerations 
of energy as to the nature of the roots of the determinantal 
equation (Thomson and Tait's Natural Philosophy, 1st edition 1867) 
has been put into a more mathematical form by Routh\ His 
investigation relates to the most general form of the equation in 
which the relations § 82 

Ort-a^y 6r»=6»r, C„ = C«. (1), 

are not assumed. But for the sake of brevity and as sufficient 
for almost all acoustical problems, these relations vdll here be 
supposed to hold. 

We shall have occasion to consider two solutions corresponding 
to two roots fly V of the equation. ITor the first we have 

^, = M,e^y ir,^M,e^', ^,^M,^\kc (2), 

and for the second 

^^^N.i^y ^,^N,^y ^, = i<r,e^,&c (3). 

In either of these solutions, for example (2), the ratios 

^ Rigid DynamieSf 5th edition, Ch. vii. 

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are determinate when /a has been chosen. They are real when 
fi is real ; and when fi is complex (a ± t^S), they take the fonD 


If now we substitute the values of '^ from (2) in the equations 
of motion, we get 

(OiiM" + 6iiA* + Cii) if, + (a,^* + 6wfA + Ci2)ifj+ =0 

{a^ + 6ij/A 4- Cu) JJfi + (a«i/Lt» H- 6a/* + CM)ifj+ =0 r-'-W- 



.=0 p--( 

The first result is' obtained by multiplying these equations in 
order by ifj, ifj, &c, and adding. It may be written 

^/A» + J5^+a = 0, (5), 


-4=Jai,Jlf,« + Jaaif,» + auJfiif,+ (6), 

J5 = \huM^^ + i6„ilf,» + 6«ilfiJlf,+ (7). 

0=iCn^i' + iCaJf,» + Ci^iif,+ (8). 

The functions -4, jB, (7, are, it will be seen, the same as we have 
already denoted by T, F, and V respectively; but the varied 
notation may be useful as reminding us that there is as yet no 
limitation upon the nature of these quadratic functions. 

The following inferences from (6) are drawn by Bouth : — 

(a) If AyByC either be zero, or be one-signed functions of 
the same sign, the fundamental determinant cannot have a real 

positive root. For if fi were real, the coefficients M^, JIT,, 

would be real. We should thus have the sum of three positive 
quantities equal to zero. 

(^) If there be no forces of resistance, i.e. if the term B be 
absent, and if A and G be one-signed and have the same sign, 
the fundamental determinant cannot have a real root, positive or 

(7) If -4, J5, (7 be one-signed functions, but if the sign of 
B be opposite to that of A and (7, the fundamental determinant 
cannot have a real negative root. 

The second equation is obtained as before from (4), except that 
now the multipliers are iVj, N^,.,. appropriate to the root v. The 
result may be written 

A(ji,v)ii^-\'B{,jL,v)lx + G{^,v)^0 (9), 


2A (fA, v) = OiiMiNi + aj\/fj^2 + 

+ a,,(M,N,+ M^,)+ (10), 

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103 a.] ROUTH's THEOREMS. 141 

with similar suppositions for B(fi,v) and C(fi,v). A(fi,v) is 
thus a symmetrical function of the Jtf s and N% so that 

A<ji,v)=A(v,^) (11). 

It will be observed that according to this notation A (fi, fi) is 
the same as ^ in (6). 
In like manner 

A(ji,v)i^ + B(pL,v)v+C(jjL,p)^0 (12), 

shewing that fi, v are both roots of the quadratic, whose co- 
efficients are A (fi, v\ B (/Lt, v), C (fi, v). Accordingly 

B(fi,v) P(M.y) n^^ 

A(fi,v) '^ A(/A,v) 

We will now suppose that fA, v are two conjugate complex 
roots, so that 

where a, yS are real. Under these circumstances if ifj, Jfa> ••• be 
A + tQi, Ps + iQa,..., then N^,N,,... will be Pi-iQj, P^-iQ,, 
, the P's and 0*8 being real. Thus by (10) 

2A(ji,v)^a,,{Pi^-{-Q,') + a^{P^+Q^) + 

+ 2a,,(P,P, + Q,(2,)+ 

^2A{P) + 2A(Q) (14). 

In (14) A(P), A(Q) are functions, such as (6), of real variables. 
From (13) we now find 

^—A-(pyfA(Q) <!«)' 

"+'^-Z(P)TX(Q) <^^)- 

From these Routh deduces the following conclusions : — 

(S) If A and B be one-signed and have the same sign 
(whether (7 be a one-signed function or not), then the real part a 
of every imaginary root must be negative and not zero. But if B 
be absent, then the real part of every imaginary root is zero. 

(e) If A and C be one-signed and have opposite signs, then 
whatever may be the character of B, there can be no imaginary 

It may be remarked that if B do not occur, and if fi^ and j^ 
be different roots of the determinant, it follows from (9), (12) that 

A(jjL,v)^C(ji,yp)^0 (17). 

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When the number of degrees of freedom is finite, the ftinda- 
mental determinant may be expanded in powers of fi, giving' 
an equation / (/a) =0 of degree 2m. The condition of stability 
is that all the real roots and the real parts of all the complex 
roots should be negative. If, as usual, complex quantities a? + »y 
be represented by points whose co-ordinates are x, y, the condition 
is that all points representing roots should lie to the left of the 
axis of y. The application of Cauchy's rule relative to the 
number of roots within any contour, by taking as the contour the 
infinite semi-circle on the positive side of the axis of y, is veiy 
fully discussed by RouthS who has thrown the results into forms 
convenient for practical application to particular casea 

108 6. The theorems of § 103 a do not exhaust all that general 
mechanical principles would lead us to expect as to the character 
of the roots of the fundamental determinant, and it may be well 
to pursue the question a little further. We will suppose through- 
out that A is one-signed and positive. 

If B and G be both one-signed and positive, we see that the 
equilibrium is thoroughly stable ; for from (a) it follows that there 
can be no positive root, and from (S) that no complex root can have 
its real part positive. 

In like manner the equations of § 103 a suffice for the case 
where C is one-signed and positive, B one-signed and negative. 
By (5) every real root is positive, and by (15) the real part 
of every complex root. Hence the equilibrium is unstable in 
every mode. 

When C is one-signed and negative, all the roots are real (S) ; 
but (5) does not tell us whether they are positive or negative. 
When J? = 0, we know (§ 87) that the roots occur in pairs of equal 
numerical value and of opposite sign. In this case therefore 
there are m positive and m negative roots. We will prove that 
this state of things cannot be disturbed by B, For if the determi- 
nant be expanded, the coefficient of /x*^ is the discriminant of J, 
and the coefficient of ij!^ is the discriminant of 0. By supposition 
neither of these quantities is zero, and thus no root of the equation 
can be other than finite. Hence as B increases from zero to its 
actual magnitude as a function of the variables, no root of the 
equation can change sign, and accordingly there remain m 

1 Adams Prize Essay 1877 ; Rigid Dynamics § 290. 

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103 6.] INSTABILITY. 143 

positive and m negative roots. It should be noticed that in this 
ai^ument there is no restriction upon the character of B. 

In the case of a real root the values of Mi, ifj, ... are real, and 
thus the motion is such as might take place under a constraint 
reducing the system to one degree of freedom. But if this con- 
straint were actually imposed, there would be two corresponding 
values of fi, being the values given by (5). In general only one of 
these is applicable to the question in hand. Othenvise it would 
be possible to define m kinds of constraint, one or other of which 
would be consistent with any of the 2m roots. But this could 
only happen when the three functions -4, jB, C are simultaneously 
reducible to sums of squares (§ 97). 

When jB = 0, there are m modes of motion, and two roots for 
each mode. In the present application to the case where C is 
one-signed and negative, each of the m modes for J3 » gives 
one positive and one negative root. The positive root denotes 
instability, and although the negative root gives a motion which 
diminishes without limit, the character of instability is considered 
to attach to the mode as a whole, and all the m modes are said 
to be unstable. But when B is finite, there are in general 2m 
distinct modes with one root corresponding to each. Of the 
2m modes m are unstable, but the remaining m modes must be 
reckoned as stable. On the whole, however, the equilibrium is 
unstable, so that the influence of B, even when positive, is in- 
sufficient to obviate the instability due to the character of C, 

We must not prolong much further our discussion of unstable 
systems, but there is one theorem respecting real roots too 
fundamental to be passed over. It may be regarded as an ex- 
tension of that of § 88. 

The value of fi corresponding to a given constraint ifi : if, : ... 
is one of the roots of (5) : and it follows from (4) that the value of 
fi is stationary when the imposed constraint coincides with one of 
the modes of free motion. The effect of small changes in A, By C 
may thus be calculated from (5) without allowance for the 
accompan}ring change of type. 

Let C, being negative for the mode under consideration, 
undergo numerical increase, while A and B remain unchanged as 
functions of the co-ordinates. The latter condition requires that 
the roots of (5), one of which is positive and one negative, should 
move either both towards zero or both away from zero ; and the 
first condition excludes the former alternative. Whether it be 

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the positive or the negative root of (5) which is the root of the 
determinant, we infer that the change in question causes the 
latter to move away from zero. 

In like manner if A increase, while B and C remain unchanged, 
the movement of the root, whether positive or negative, is 
necessarily towards zero. 

Again, if A and C be given, while B increases algebraically 
as a function of the variables, the movement of the root of the 
determinant must be in the positive direction. 

Ad algebraic increase in B thus increases the stability, or 
decreases the instability, in every mode. A numerical increase 
in C or decrease in A on the other hand promotes the stability 
of the stable modes and the instability of the unstable modes. 

We can do little more than allude to the theorem relating to 
the effect of a single constraint upon a system for which G is 
one-signed and negative. Whatever be the nature of B, the 
(m— 1) positive roots of the determinant, appropriate to the 
system after the constraint has been applied, will separate the m 
positive roots of the original determinant, and a like proposition 
will hold for the negative roots. Upon this we may found a 
generalization of the foregoing conclusions analogous to that 
of § 92 a. Consider an independent vibrator of one degree of 
freedom for which C is positive, and let the roots of the frequency 
equation be Vi, I'a, one negative and one positive. If we regard 
this as forming part of the system, we have in all (2m + 2) roots. 
The effect of a constraint by which the two parts of the system 
are connected will be to reduce the (2m + 2) back to ^m. Of 
these the m positive will separate the (m + 1) quantities formed 
of the m positive roots of the original equation together with (the 
positive) 1/2, and a similar proposition will hold for the negative 
roots. The effect of the vibrator upon the original system is thus 
to cause a movement of the positive roots towards v^y and a 
movement of the negative roots towards Vj. This conclusion 
covers all the previous statements as to the effect of changes in 
Ay B, C upon the values of the roots. 

Enough has now been said on the subject of the free vibra- 
tions of a system in general. » Any further illustration that it 
may require will be afforded by the discussion of the case of two 
degrees of freedom, § 112, and by the vibrations of strings and other 
special bodies with which we shall soon be occupied. We resume 

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the equations (1) § 103, with the view of investigating further the 
nature oi forced vSmxtions, 

104. In order to eliminate irom the equations all the co- 
ordinates but one ('^i), operate on them in succession with the 
minor determinants 

dV dV dV ^ 

and add the results together; and in like manner for the other 
oo-ordinate& We thus obtain as the equivalent of the original 
system of equations 


in which the differentiations of V are to be made without re- 
cognition of the equality subsisting between ert and e^. 

The forces '^^i, ^9^, &c. are any whatever, subject, of course, 
to the condition of not producing so great a displacement or 
motion that the squares of the small quantities become sensible. 
If, as is often the case, the forces operating be made up of two 
parts, one constant with respect to time, and the other periodic, 
it is convenient to separate in imagination the two classes of 
effects produced. The effect due to the constant forces is exactly 
the same as if they acted alone, and is found by the solution 
of a statical problem. It will therefore generally be sufficient 
to suppose the forces periodic, the effects of any constant forces, 
such as gravity, being merely to alter the configuration about 
which the vibrations proper are executed. We may thus without 
any real loss of generality confine ourselves to periodic, and 
therefore by Fourier's theorem to harmonic forces. 

We might therefore assume as expressions for ^^^ &c. circular 
functions of the time; but, as we shall have frequent occasion 
to recognise in the course of this work, it is usually more con- 
venient to employ an imaginary exponential function, such as 
E^p\ where ^ is a constant which may be complex. When the 
R. 10 

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corresponding symbolical solution is obtained, its real and 
imaginary parts may be separated, and belong respectively to 
the real and imaginary parts of the data. In this way the 
analysis gains considerably in brevity, inasmuch as differentiations 
and alterations of phase are expressed by merely modifying^ the 
complex coefficient without changing the form of the function. 
We therefore write 

^1 = ^,^1^, "ir^^E^e^^ &c, 


The minor determinants of the type -p- are rational integral 

functions of the symbol D, and operate on ^], &c. according to 

f{D)^=f(ip)^'^ (2). 

Our equations therefore assume the form 

V^, = i4,en V^, = ^e**, &c (3), 

where Ai, A^, &c. are certain complex constants. And the sym- 
bolical solutions are 

or by (2), ^, = ^,-^, &c (4), 

where V (ip) denotes the result of substituting ip for D in V. 

Consider first the case of a system exempt from friction. 

V and its differential coefficients are then even functions of 
D, so that V(ip) is real. Throwing away the imaginary part 
of the solution, writing -Bie**» for Ai, &c., we have 


^i = y^C0S(p« + tfi)> &C (5). 

If we suppose that the forces "^^i, &c. (in the case of more 
than one generalized component) have all the same phase, they 
may be expressed by 

EiCos(pt-\-a\ EiCosipt + a), &c. ; 

and then, as is easily seen, the co-ordinates themselves agree 
in phase with the forces: 

t> = V^co8(l>« + a) (6). 

The amplitudes of the vibrations depend among other things 
on the magnitude of ^ (ip). Now, if the period of the forces 

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be the same as one of those belonging to the free vibrations, 
V (%p) = 0, and the amplitude becomes infinite. This is, of 
<x>urse, just the case in which it is essential to introduce the 
consideration of friction, from which no natural system is really 

If there be friction, V (ip) is complex ; but it may be divided 
into two pai-ts — one real and the other purely imaginary, of which 
the latter depends entirely on the friction. Thus, if we put 

V(ip) = Vi(i/)) + i>V,(ip) (7), 

Vi, Vj are even functions of ip, and therefore real. If as before 
Ai = i2i6^', our solution takes the form 

or, on throwing away the imaginary part, 

{V,(ip)|»+J)»V.7yS)l»}i ^ ^' 

where tan7 = ~^,^^^ (9). 

We have said that V, (ip) depends entirely on the friction ; but 
it is not true, on the other hand, that V^ (ip) is exactly the same, 
as if there had been no friction. However, this is approximately 
the case, if the friction be small ; because any part of V (ip), which 
depends on the first power of the coefficients of friction, is neces- 
-sarily imaginary. Whenever there is a coincidence between the 
period of the force and that of one of the free vibrations, V^ (ip) 
vanishes, and we have tan 7 = — oo , and therefore 

It,sm(pt + 0^) 

indicating a vibration of large amplitude, only limited by the 

On the hypothesis of small firiction, is in general small, and 
so also is 7, except in case of approximate equality of periods. 
With certain exceptions, therefore, the motion has nearly the 
same (or opposite) phase with the force that excites it. 

When a force expressed by a harmonic term acts on a system, 
the resulting motion is everywhere harmonic, and retains the 
original period, provided always that the squares of the displace- 


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meats and velocities may be neglected. This important principle 
^as enunciated by Laplace and applied by him to the theory of 
the tides. Its great generality was also recognised by Sir John 
Herschel, to whom we owe a formal demonstration of its truths 

If the force be not a harmonic function of the time, the types 
of vibration in different parts of the system are in general different^ 
from each other and from that of the force. The harmonic 
functions are thus the only ones which preserve their type un- 
changed, which, as was remarked in the Introduction, is a strong 
reason for anticipating that they correspond to simple tones. 

106. We now turn to a somewhat different kind of forced 
vibration, where, instead of given /orce« as hitherto, given inexora- 
ble motions are prescribed. 

If we suppose that the co-ordinates -^i, -^a, ••• V^r *re given 
functions of the time, while the forces of the remaining types 
•^y+i, '*',.+„ ... '*'»» vanish, the equations of motion divide them- 
selves into two groups, viz. 


er+1,1 ^1 + «r+l,i >/^2 + ... + ^r+l.m '^m = ) 


emi '^1 + ^ms '^s+.-.+^mw '^m = J 

In each of the m — r equations of the latter group, the first r 
terms are known explicit functions of the time, and have the same 
effect as known forces acting on the system. The equations of 
this group are therefore sufficient to determine the unknown 
quantities ; after which, if required, the forces necessary to main- 
tain the prescribed motion may be determined from the liret 
group. It is obvious that there is no essential difference between 
the two classes of problems of forced vibrations. 

106. The motion of a system devoid of friction and executing 
simple harmonic vibrations in consequence of prescribed variations 
of some of the co-ordinates, possesses a peculiarity parallel to those 
considered in §§ 74, 79. Let 

'^i = -4iCosp<, •^, = -4jCosp^, &c., 
^ Encyc. Metrop. art. 823. Also Outlinei of Astronomy , § 650. 

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in which the cjuantities Ai..,Ar are regarded as given, while the 
remaining ones are arbitrary. We have from the expressions for 
Tand 7, § 82, 

+ {i(^i-p"^)-^i'+ ••• +(^-"l>'^«)-4i-4j+ •••} cos 2p<, 
from which we see that the equations of motion express the con- 
dition that E, the variable part of T + F, which is proportional to 

i(^-l>"flbi)^i' + ...+(Ci2-l>*a»)ili^, + (1), 

shall be stationary in value, for all variations of the quantities 
Ar+i . . . Am' Let p'* be the value of p* natural to the system when 
vibrating under the restraint defined by the ratios 

Ai : A^.,,Ar : Ar+i l ...^my 

8o that 

J?=r(p'«-jp«){iauili« + ...+au4i^ + ...} (2). 

From this we see that if p* be certainly less than p'* ; that is, 
if the prescribed period be greater than any of those natural to 
the system under the partial constraint represented by 

Ai : ^a*" Arj 

then E is necessarily positive, and the stationary value — ^there can 
be but one — ^is an absolute minimum. For a similar reasoD, if the 
prescribed period be less than any of those natural to the partially 
constrained system, £ is an absolute maximum algebraically, but 
arithmetically an absolute minimum. But when p* lies within the 
range of possible values of p'*, E may be positive or negative, and 
the actual value is not the greatest or least possible. Whenever 
a natural vibration is consistent with the imposed conditions, that 
will be the vibration assumed. The variable part of 74- F is then 

For convenience of treatment we have considered apart the 
two great classes of forced vibrations and free vibrations; but there 
is, of course, nothing to prevent their coexistence. After the lapse 
of a sufficient interval of time, the free vibrations always dis- 
appear, however small the friction may be. The case of abso- 
lutely no friction is purely ideal. 

There is one caution, however, which may not be superfluous 
in respect to the case where given motions are forced on the 
system. Suppose, as before, that the co-ordinates -^i, '^a,...'^^ are 
given. Then the free vibrations, whose existence or non-existence 

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is a matter of indifference so far as the forced motion is concemed, 
must be understood to be such as the system is capable of, when 
the co-ordinates V^i.-.-^r <^'^^ w)f allowed to vary from zero. Ln 
order to prevent their varjdng, forces of the corresponding types 
must be introduced ; so that from one point of view the motion in 
question may be regarded as forced. But the applied forces are 
merely of the nature of a constraint ; and their effect is the same 
as a limitation on the freedom of the motion. 

106 a. The principles of the last sections shew that if 
V^ii '^f-'^r be given harmonic functions of the time AiCoaptj 
A2 cos pt,..,, the forces of the other types vanishing, then the 
motion is determinate, unless p is so chosen as to coincide with 
one of the values proper to the system when -^i, '^^...^r are 
maintained at zero. As an example, consider the case of a 
membrane capable of vibrating transversely. If the displacement 
y^ at every point of the contour be given (proportional to cos pt), 
then in general the value in the interior is determinate ; but an 
exception occurs if p have one of the values proper to the 
membrane when vibrating with the contour held at rest. This 
problem is considered by M. Duhem^ on the basis of a special 
analytical investigation by Schwartz. It will be seen that it may 
be regarded as a particular case of a vastly more general theorem. 

A like result may be stated for an elastic solid of which the 
surface motion (proportional to cos pt) is given at every point. Of 
course, the motion at the boundary need not be more than partially 
given. Thus for a mass of air we may suppose given the motion 
normal to a closed surface. The internal motion is then deter- 
minate, unless the frequency chosen is one of those proper to the 
mass, when the surface is made unyielding. 

107. Very remarkable reciprocal relations exist between the 
forces and motions of different types, which may be regarded as 
extensions of the corresponding theorems for systems in which 
only F or r has to be considered (§ 72 and §§ 77, 78). If we sup- 
pose that all the component forces, except two — '^'i and '*', — are 
zero, we obtain from § 104, 


1 Cours de Phyiique Math€matiqu€, Tome Second, p. 190, Paris, 1S91. 

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We now consider two cases of motion for the same system ; first 
when ^s vanishes, and secondly (with dashed letters) when '9i 
vanishes. If ^, = 0, 

^-^-'£^^ (^>- 

Similarly, if ^,' = 0, 

^''=^-'£^'' <^)- 

In these equations V and its differential coefficients are rational 
integral functions of the symbol D; and since in every case 
^r« = «#r, ^ is a symmetrical determinant, and therefore 

^^^^^ (4) 

den deg, 

zfft u^ir 

Hence we see that if a force '*'i act on the system, the co- 
ordinate '^^ is related to it in the same way as the co-ordinate '^Z 
is related to the force '9^, when this latter force is supposed to act 

In addition to the motion here contemplated, there may be 
free vibrations dependent on a disturbance already existing at the 
moment subsequent to which all new sources of disturbance are 
included in '9 ; but these vibrations are themselves the effect of 
forces which acted previously. However small the dissipation 
may be, there must be an interval of time after which free vibra- 
tions die out, and beyond which it is unnecessary to go in taking 
account of the forces which have acted on a system. If therefore 
we include under "V forces of sufficient remoteness, there are no 
independent vibrations to be considered, and in this way the 
theorem may be extended to cases which would not at first sight 
appear to come within its scope. Suppose, for example, that the 
system is at rest in its position of equilibrium, and then begins to 
be acted on by a force of the first type, gradually increasing in 
magnitude from zero to a finite value ^i, at which point it ceases 
to increase. If now at a given epoch of time the force be sud- 
denly destroyed and remain zero ever afterwards, free vibrations of 
the system will set in, and continue until destroyed by friction. 
At any time t subsequent to the given epoch, the co-ordinate yfr^ 
has a value dependent upon t proportional to '*'i. The theorem 
allows us to assert that this value yfr^ beai*s the same relation to '9i 
as yJTi would at the same moment have borne to '^/, if the original 
cause of the vibrations had been a force of the second type in- 

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creasing gradually from zero to '^/, and then suddenly vaniBhing^ 
at the given epoch of time. We have already had an example of 
this in § 101, and a like result obtains when the cause of the 
original disturbance is an impulse, or, as in the problem of the 
pianoforte-string, a variable force of finite though short duration^ 
In these applications of our theorem we obtain results relating to 
free vibrations, considered as the residual effect of forces whose 
actual operation may have been long before. 

108. In an important class of cases the forces ^i and '9^ are 
harmonic, and -of the same period. We may represent them by 
Aie^^^, ilaV^*, where Ai and A^ may be assumed to be recdf if the 
forces be in the same phase at the moments compared. The 
results may then be written 

^■.^,i}s^^l ™- 

where ip is written for D. Thus, 

^V« = ilit/.... (2). . 

Since the ratio ^^i : il,' is by hypothesis real, the same is 

true of the ratio -^Z : -^s; which signifies that the motions 

represented by those symbols are in the same phase. Passing 
to real quantities we may state the theorem thus: — 

If a force ^i = AiC08pt, aoting on the system give rise to 
the motion '^j = dAiCOs(pt — e); then will a force 'S^a' == A,' cos pt 
produce the motion -^Z = dk^ cos (pt — c). 

If there be no friction, e will be zero. 

If ^1 = -4j', then >fr/ = -^j. But it must be remembered that 
the forces "^i and 'V^ are not necessarily comparable, any more 
than the co-ordinates of corresponding t)rpes, one of which for 
example may represent a linear and another an angular dis- 

The reciprocal theorem may be stated in several ways, but 
before proceeding to these we will give another investigation, 
not requiring a knowledge of determinants. 

If ^1,^,,... -^tu V^,,... and ^/, ^/,... i|r/, -^Z,... be two sets 

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of forces and corresponding displacements, the equations of 
motion, § 103, give 

+ ^/r/(e^i|ri + eM'^2 + ««V^.+ ...) + ••• • 

Now, if all the forces vary as ^^^ the effect of a symbolic 
operator such as en on any of the quantities -^ is merely to 
multiply that quantity by the constant found by substituting 
ip for D in €„. Supposing this substitution made, and having 
regard to the relations «« = ««•, we may write 

+ ^.(V^i>, + V^,>i) + (3). 

Hence by the symmetry 

which is the expression of the reciprocal relation. 

109. In the applications that we are about to make it 

will be supposed throughout that the forces of all tjrpes but 

two (which we may as well take as the first and second) are 

zero. Thus 

^i^i' + >i^,l|r/«^/V^,+^,>, (1). 

The consequences of this equation may be exhibited in three 
different ways. In the first we suppose that 

whence V^, : ^, = if-/ : ^/ (2), 

shewing, as before, that the relation of '^^ to "9^ in the first 
case when "9^^^ is the same as the relation of '^Z to ^,' in 
the second case, when '*'i = 0, the identity of relationship ex- 
tending to phase as well as amplitude. 

A few examples may promote the comprehension of a law, 
whose extreme generality is not unlikely to convey an impression 
of vagueness. 

If P and Q be two points of a horizontal bar supported in 
any manner (e.g. with one end clamped and the other free), a 
given harmonic transverse force applied at P will give at any 
moment the same vertical deflection at Q as would have been 
found at P, had the force acted at Q. 

If we take angular instead of linear displacements, the 

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Google -^ 


theorem will run: — A given harmonic couple at P will give the 
same rotation at Q as the couple at Q would give at P. 

Or if one displacement be linear and the other angular, the 
result may be stated thus: Suppose for the first case that a 
harmonic couple acts at P, and for the second that a vertical 
force of the same period and phase acts at Q, then the linear 
displacement at Q in the first case has at every moment the 
same phase as the rotatory displacement at P in the second, 
and the amplitudes of the tiro displacements are so related that 
the maximum couple at P would do the same work in acting 
over the maximum rotation at P due to the force at Q, as the 
maximum force at Q would do in acting through the maximum 
displacement at Q due to the couple at P. In this case the 
statement is more complicated, as the forces, being of different 
kinds, cannot be taken equal. 

If we suppose the period of the forces to be excessively long, 
the momentary position of the system tends to coincide with 
that in which it would be maintained at rest by the then acting 
forces, and the equilibrium theory becomes applicable. Our 
theorem then reduces to the statical one proved in § 72. 

As a second example, suppose that in a space occupied by 
air, and either wholly, or partly, confined by solid boundaries, 
there are two spheres A and B, whose centres have one degree 
of freedom. Then a periodic force acting on A will produce 
the same motion in B, as if the parts were interchanged; and 
this, whatever membranes, strings, forks on resonance cases, or 
other bodies capable of being set into vibration, may be present in 
their neighbourhood. 

Or, if A and B denote two points of a solid elastic body 
of any shape, a force parallel to OX, acting at A, will produce 
the same motion of the point B parallel to OF as an equal force 
parallel to OY acting at B would produce in the point A, 
parallel to OX. 

Or again, let A and B be two points of a space occupied by 
air, between which are situated obstacles of any kind. Then a 
sound originating at A is perceived at B with the same intensity 
as that with which an equal sound originating at B would be per- 
ceived at ^.^ The obstacle, for instance, might consist of a rigid 

^ Helmholtz, CreUe, Bd. lvii., 1859. The soands must be such as in the absenoe 
of obstacles would diffuse themselves equally in aU directions. 

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wall pierced with one or more holes. This example corresponds 
to the optical law that if by any combination of reflecting or 
refracting surfaces one point can be seen from a second, the second 
can also be seen from the first. In Acoustics the sound shadows 
are usually only partial in consequence of the not insignificant 
value of the wave-length in comparison with the dimensions of 
ordinary obstacles: and the reciprocal relation is of considerable 

A frirther example may be taken from electricity. Let there 
be two circuits of insulated wire A and B, and in their neigh- 
bourhood any combination of wire-circuits or solid conductors 
in communication with condensers. A periodic electro-motive 
force in the circuit A will give rise to the same current in B 
as would be excited in A if the electro-motive force operated 
in B. 

Our last example will be taken from the theory of conduction 
and radiation of heat, Newton's law of cooling being assumed 
as a basi& The temperature at any point A of sl conducting and 
radiating system due to a steady (or harmonic) source of heat 
at ^ is the same as the temperature at B due to an equal source 
at A. Moreover, if at any time the source at B be removed, the 
whole subsequent course of temperature at A will be the same as 
it would be at fi if the parts of B and A were interchanged. 

110. The second way of stating the reciprocal theorem is 
arrived at by taking in (1) of § 109, 

V^i = 0, i|r; = 0; 

whence ^iV^/ = ^V^2 (1). 

or ^, : ifr. = ^/ : ^/ (2), 

shewing that the relation of ^j to yfr^ in the first case, when -^i = 0, 
is the same as the relation of ^,' to yjti in the second case, when 


Thus in the example of the rod, if the point P be held at 
rest while a given vibration is imposed upon Q (by a force there 
applied), the reaction at P is the same both in amplitude and 
phase as it would be at Q if that point were held at rest and 
the given vibration were imposed upon P. 

So if A and B be two electric circuits in the neighbourhood 
of any number of others, C, D,,.. whether closed or terminating 

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in condensers, and a given periodic current be excited in A by 
the necessary electro-motive force, the induced electro-motive 
force in B is the same as it would be in ^, if the parts of A 
and B were interchanged. 

The third form of statement is obtained by putting in (1) 
of § 109, 

%=o. v^;=o; 

whence ^i>i + ^2>2 = (3), 

or ^1 : V^, = -^/ :>/ (4), 

proving that the ratio of -^i to yjr^ in the first case, when '9^ acts 
alone, is the negative of the ratio of '9^' to '9i in the second case, 
when the forces are so related as to keep -^Z equal to zero. 

Thus if the point P of the rod be held at rest while a periodic 
force acts at Q, the reaction at P bears the same numerical ratio 
to the force at Q as the displacement at Q would bear to the 
displacement at P, if the rod were caused to vibrate by a force 
applied at P. 

111. The reciprocal theorem has been proved for all systems 
in which the frictional forces can be represented by the function F, 
but it is susceptible of a further and an important generalization. 
We have indeed proved the existence . of the function F for 
a large class of cases where the motion is resisted by forces 
proportional to the absolute or relative velocities, but there are 
other sources of dissipation not to be brought under this head, 
whose effects it is equally important to include ; for example, the 
dissipation due to the conduction or radiation of heat. Now 
although it be true that the forces in these cases are not for aU 
possible motions in a constant ratio to the velocities or displace- 
ments, yet in any actual case of periodic motion (t) they are 
necesseuily periodic, and therefore, whatever their phase, ex- 
pressible by a sura of two terms, oue proportional to the dis- 
placement (absolute or relative) and the other proportional to the 
velocity of the part of the system affected. If the coefficients 
be the same, not necessarily for all motions whatever, hut for all 
motions of the period r, the function F exists in the only sense 
required for our present purpose. In fact since it is exclusively 
with motions of period r that the theorem is concerned, it is 
plainly a matter of indifference whether the functions T, F, V 
are dependent upon r or not. Thus extended, the theorem is 

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perhaps sufficiently general to cover the whole field of dissipative 

It is important to remember that the Principle of Reciprocity- 
is limited to systems which vibrate about a configuration of equi- 
librium, and is therefore not to be applied without reservation to 
such a problem as that presented by the transmission of sonorous 
waves through the atmosphere when disturbed by wind. The 
vibrations must also be of such a character that the square of the 
motion can be neglected throughout; otherwise our demonstra- 
tion would not hold good. Other apparent exceptions depend on 
a misunderstanding of the principle itself. Care must he taken 
to observe a proper correspondence between the forces and dis- 
placements, the rule being that the action of the force over the 
displacement is to represent work done. Thus couples correspond 
to rotations, pressures to increments of volume, and so on. 

Ill a. The substance of the preceding sections is taken £rom 
a paper by the Author*, in which the action of dissipative forces 
appears first to have been included. Reciprocal theorems of a 
special character, and with exclusion of dissipation, had been 
previously given by other writers. One, due to von Helmholtz, 
has already been quoted. Reference may also be made to the 
reciprocal theorem of Betti*, relating to a uniform isotropic elastic 
solid, upon which bodily and surface forces act. Lamb* has shewn 
that these results and more recent ones of von Helmholtz^ may 
be deduced from a very general equation established by Lagrange 
in the Mdcanique Analytique, 

111 6. In many cases of practical interest the external force, 
in response to which a system vibrates harmonically, is applied at a 
single point. This may be called the driving-point, and it becomes 
important to estimate the reaction of the sjrstem upon it. When 
T and F only are sensible, or F and V only, certain general 
conclusions may be stated, of which a specimen will here be given. 
For further details reference must be made to a paper by the 
Author •. 

1 ** Some General Theorems relating to Vibrations," Froe, Math, Soc., 1878. 
» II Nuovo Cimento, 1872. 

» Proc. Math. Soc., Vol. xix., p. 144, Jan. 1888. 
* CreUe, t. 100, pp. 137, 213. 1886. 

B '*The Beaction upon the Driving-point of a System ezecnting Forced Harmonic 
' Oscillations of various Periods." Phil. Mag., May, 1886. 

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Consider a system, devoid of potential energy, in which the 
co-ordinate yfri is made to vary by the operation of the harmonic 
force '9i, proportional to e*^. The other co-ordinates may be chosen 
arbitrarily, and it will be very convenient to choose them so that 
no product of them enters into the expressions for Tand F, They 
would be in fact the normal co-ordinates of the system on the 
supposition that yfr^ is constrained (by a suitable force of its own 
type) to remain zero. The expressions for T and F thus take the 
following forms : — 

+ <hlt^lit^ + (hz^l^Z + (h4^l4'4'^ ...(1). 

The equations for a force '*'i, proportional to e*^, are accordingly 

(tpOii -I- bn) ^1 + (tpOia + 6is) ^s + (tpo^ + ^w) ^s + . . . = ^i, 

(ipoi^ + 6,a) ^^1 + (ipa„ -H b„) i/r, = 0, 
(ipoi, + 6„) ^i -H (ipon + 63s) ^s = 0, 

By means of the second and following equations -^j^ '^s ... are 
expressed in terms of yjri. Introducing these values into the first 
equation, we get 

%l^^-ip<^r + K-^?^^-^^^^- (3). 

The ratio '^^i/'^i is a complex quantity, of which the real part 
corresponds to the work done by the force in a complete period 
and dissipated in the system. By an extension of electrical 
language we may call it the resistance of the system and denote it 
by the letter R'. The other part of the ratio is imaginary. If we 
denote it by ipL'^i^ or Z'-^i, L' will be the moment of inertia, or 
self-induction of electrical theory. We write therefore 

^, = (iJ'4-tpi0^i (4); 

and the values of R and L are to be deduced by separation of the 
real and the imaginary parts of the right-hand member of (3). In 
this way we get 

^-^--^h^^p^b^i^^Tp^) ^^>- 

This is the value of the resistance as determined by the 
constitution of the system, and by the frequency of the imposed 

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vibration. Each component of the latter series (which alone 
involves p) is of the form <iji^l{P + yp^)\ where a, /9, 7 are all positive, 
and (as may be seen most easily by considering its reciprocal) 
increases continually as jp* increases from zero to infinity. We 
conclude that as the frequency of vibration increases, the value of 
R increases continuously with it. At the lower limit the motion 
is determined sensibly by the quantities h (the resistances) only, and 
the corresponding resultant resistance R is an absolute minimum, 
whose value is 

&u-S(6„V6«) (6). 

At the upper limit the motion is determined by the ineiiiia of 
the component parts without regard to resistances, and the value 

T V iha* . < (gi«&« - <hi>uy 



6„ + S(6«^|-26„^) (7). 

When p is either very large or very small, all the co-ordinates 
are in the same phase, and (6), (7) may be identified with 

Also i'»a,-2^V2^^^^f4x (8). 

In the latter series every term is positive, and continually 
diminishes as p^ increases. Hence every increase of frequency is 
attended by a diminution of the moment of inertia, which tends 
ultimately to the minimum corresponding to the disappearance of 
the dissipative terms. 

If p be either very large or very small, (8) identifies itself 
with 2TI^^\ 

As a simple example take the problem of the reaction upon 
the primary circuit of the electric currents generated in a neigh- 
bouring secondary circuit. In this case the co-ordinates (or rather 
their rates of increase) ai-e naturally taken to be the currents 
themselves, so that '^i is the primary, and -^3 the secondary 
current. In usual electrical notation we represent the coefficients 
of self-induction by i, N, and of mutual induction by M, so that 

and the resistances by R and 8. Thus 

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and (5) and (8) become at once 

^ -^-^¥+^* ^^^' 

^-■^-S'-'+w ^ ^' 

These formulae were given originally by Maxwell, who remarked 
that the reaction of the currents in the secondary has the effect 
of increasing the effective resistance and diminishing the effective 
self-induction of the primaiy circuit. 

If the rate of alternation be very slow, the secondary circuit is 
without influence. If, on the other hand, the rate be very rapid, 

iJ' = iZ -h M'SjN^ i' =Z - M'IN. 

112. In Chapter ill. we considered the vibrations of a system 
with one degree of freedom. The remainder of the present Chapter 
will be devoted to some details of the case where the degrees of 
freedom are two. 

If w and y denote the two co-ordinates, the expressions for T 
and V are of the form 

2V==Aid' + 2Bxy + Cy*\ ^^' 

so that, in the absence of friction, the equations of motion are 

Lx-\-My-\-Ax-^By = X\ . 

Mx-^Ny + Bx+Cy=Y] ^^^• 

When there are no impressed forces, we have for the natural 


(LI> +A)x^{M]>-\-B)y^O\ 
(MD^ + B)x+{ND^-{'C)y = 0' 

D being the symbol of differentiation with respect to time. 

If a solution of (3) be x — le^, y = me**, X' is one of the 
roots of 

{L>}'\-A){N\^ + C)-{M\* + By = Q (4), 


\'{LN^M^)^X^{LG'\-NA'-2MB) + AG^»^0 (5). 

The constants L, M, N\ A, B, (7, are not entirely arbitrary. 
Since T and V are essentially positive, the following inequalities 
must be satisfied : — 

LN>M\ AC>B' (6). 

Moreover, L, N, A^ C must themselves be positive. 


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We proceed to examine the effect of these restrictions on the 
roots of (5). 

In the first place the three coefficients in the equation are 
positive. For the first and third, this is obvious £rom (6). The 

ii^ which, as is seen from (6), JLNAG is necessarily greater than 
MB, We conclude that the values of \*, if real, are both 

It remains to prove that the roots are in fact real The 
ition to be satisfied is that the following quantity be not 
neglative : — 

After reduction this may be brought into the form 
+ (^/I0 - jNly {{JLC - jNlr + 4 {JLNAG - MB)\ 

which shews that the condition is satisfied, since JLNAG --MB 
is positive. This is the analytical proof that the values of X' are 
both real and negative ; a fact that might have been anticipated 
without any analysis from the physical constitution of the system, 
whose vibrations they serve to express. 

The two values of X' are different, unless both 


which require that 

L : M : N^A : B : G (7), 

The common spherical pendulum is an example of this case. 

By means of a suitable force Y the co-ordinate y may be 
prevented from varying. The system then loses one degree of 
freedom, and the period corresponding to the remaining one is in 
general different from either of those possible before the introduc- 
tion of F. Suppose that the types of the motions obtained by 
thus preventing in turn the variation of y and x are respectively 
e^^, e^. Then /Lti', ftj* are the roots of the equation 

(L\' + A)(N\' + G) = 0, 

R. 11 

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162 VIBRATING SYsWeMS^*^^ ^ ^^^^^^ [ll2. 

being that obtained from (4) b)\ ' suppressing if and B. Hence 
(4) may itself be put into the form^ ^p>J| 

ZiV^(X«-/iiO(V-/^Y^*-^ = ^^^^ (^X 

which shews at once that neither Vw^f the roots of V can be 
intermediate in value between fj^^ aS^ id /*,* A Etle funiiS ^ 
examination will prove that one of the ro^Mal^ ^ grwiter tHi both, 
the quantities /ii', /Xj', and the other less thaiSr^V^!.?o/if we pu^ 

/( V) = ZJV^ (V - /i,0 (V - Ata^) - (ilf V + 5)^ 
we see that when X* is very small, / is positive (AC-B^); whj 
V decreases (algebraically) to fii\ f changes sign and becomes 
negative. Between and /ii* there is therefore a root ; and 
by similar reasoning between fta* and — x . We conclude thatSfche 
tones obtained by subjecting the system to the two kinds of con- 
straint in question are both intermediate in pitch between 4he 
tones given by the natural vibrations of the system. In particu] 
cases fii\ fi^ may be equal, and then 

This proposition may be generalized Any kind of constraint 
which leaves the system still in possession of one degree of free- 
dom may be regarded as the imposition of a forced relation 
between the co-ordinates, such as 

aa?-|-^y = (10). 

Now if cue + ^y, and any other homogeneous linear func- 
tion of X and y, be taken as new variables, the same argument 
proves that the single period possible to the system after the 
introduction of the constraint, is intermediate in value between 
those two in which the natural vibrations were previously per- 
formed. Conversely, the two periods which become possible 
when a constraint is removed, lie one on each side of the original 

If the values of X* be equal, which can only happen when 
L : M : N=A : B : C, 
the introduction of a constraint has no effect on the period ; for 
instance, the limitation of a spherical pendulum to one vertical 

113. As a simple example of a system with two degrees of 
freedom, we may take a stretched string of length I, itself without 


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inertia, but carrying two equal masses m at distances a and b from 
one end (Fig. 17). Tension = 2',. 

Fig. 17. 

K a and y denote the displacements, 
2T = m(£* + y'), 


a b — a I — b) ' 

Since T and V are not of the same form, it follows that the 
two periods of vibration are in every case unequal. 

If the loads be symmetrically attached, the character of the 
two component vibrations is evident. In the first, which will have 
the longer period, the two weights move together, so that x and y 
remain equal throughout the vibration. In the second x and y are 
numerically equal, but opposed in sign. The middle point of the 
string then remains at rest, and the two masses are always to 
be found on a straight line passing through it. In the first case 
a; — y = 0, and in the second j;H-y = 0; so that a; — y and a? + y 
are the new variables which must be assumed in order to reduce 
the functions T and V simultaneously to a sum of squares. 

For example, if the masses be so attached as to divide the 
string into three equal parts. 


from which we obtain as the complete solution, 
x + y = Acosy^.t + ay 


.-y^Bcos{^.t + ^)^ 


where, as usual, the constants A, a, B, jS are to be determined by 
the initial circumstances. 

114. When the two natural periods of a system are nearly 
equal, the phenomenon of intermittent vibration sometimes pre- 
sents itself in a very curious manner. In order to illustrate this, 


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we may recur to the string loaded, we will now suppose, with two 
equal masses at distances from its ends equal to one-fourth of the 
length. If the middle point of the string were absolutely fixed, 
the two similar systems on either side of it would be completely 
independent, or, if the whole be considered as one system, the two 
periods of vibration would be equal. We now suppose that 
instead of being absolutely fixed, the middle point is attached to 
springs, or other machinery, destitute of inertia, so that it is 
capable of yielding slightly. The reservation as to inertia is to 
avoid the introduction of a third degree of freedom. 

From the symmetry it is evident that the fundamental vibra- 
tions of the system are those represented by a?H-y and x — y. 
Their periods are slightly different, because, on account of the 
yielding of the centre, the potential energy of a displacement 
when X and y are equal, is less than that of a displacement 
when X and y are opposite; whereas the kinetic energies are 
the same for the two kinds of vibration. In the solution 

a? + y = -4cos(ni« + a) | 

we are therefore to regard n^ and n, as nearly, but not quite, equal. 
Now let us suppose that initially x and x vanish. The conditions 

-4 cos a -h -Bcos^ = 
UiA sin a + n^B sin /8 = 

which give approximately 

^+-8 = 0, a = ^. 

Thus x = A%m ^ ^ ^ t smf ^^"<H-aj 

y = Acos -g— t cos f g ^ 4- a 1 

The value of the co-ordinate x is here approximately ex- 
pressed by a harmonic term, whose amplitude, being proportional 
to sin J (n^ - Wi) *. is a slowly varying harmonic function of the 
time. The vibrations of the co-ordinates are therefore intermittent, 
and so adjusted that each amplitude vanishes at the moment that 
the other is at its maximum. 

This phenomenon may be prettily shewn by a tuning fork of 
very low pitch, heavily weighted at the ends, and firmly held by 


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screwing the stalk into a massive support. When the fork vibrates 
in the normal manner, the rigidity^ or want of rigidity, of the 
stalk does not come into play ; bat if the displacements of the two 
prongs be in the same direction, the slight yielding of the stalk 
entails a small change of period. If the fork be excited by striking 
one prong, the vibrations are intermittent, and appear to transfer 
themselves bcu^kwards and forwards between the prongs. Unless, 
however, the support be very firm, the abnormal vibration, which 
involves a motion of the centre of inertia, is soon dissipated ; and 
then, of course, the vibration appears to become steady. If the 
fork be merely held in the hand, the phenomenon of intermittence 
cannot be obtained at all. 

116. The stretched string with two attached masses may be 
used to illustrate some general principles. For example, the period 
of the vibration which remains possible when one mass is held 
at rest, is intermediate between the two free periods. Any in- 
crease in either load depresses the pitch of both the natural 
vibrations, and conversely. If the new load be situated at a point 
of the string not coinciding with the places where the other loads 
are attached, nor with the node of one of the two previously 
possible free vibrations (the other has no node), the effect is still 
to prolong both the periods already present. With regard to the 
third finite period, which becomes possible for the first time after 
the addition of the new load, it must be regarded as derived from 
one of infinitely small magnitude, of which an indefinite number 
may be supposed to form part of the system. It is instructive 
to trace the effect of the introduction of a new load and its gradual 
increase from zero to infinity, but for this purpose it will be 
simpler to take the case where there is but one other. At the 
commencement there is one finite period Ti, and another of in- 
finitesimal magnitude r,. As the load increases r, becomes finite, 
and both Ti and Tg continually increase. Let us now consider 
what happens when the load becomes very great. One of the 
periods is necessarily large and capable of growing beyond all 
limit The other must approach a fixed finite limit. The first 
belongs to a motion in which the larger mass vibrates nearly as 
if the other were absent ; the second is the period of the vibration 
of the smaller mass, taking place much as if the larger were fixed. 
Now since Tj and r, can never be equal, Ti must be always the 
greater ; and we infer, that as the load becomes continually larger, 

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it is Ti that increases indefinitely, and r, that approaches a finite 

We now pass to the consideration of forced vibrations. 

116. The general equations for a system of two degrees of 
freedom including friction are 

{MD'+l3D-hB)x + {ND' + yD-hC)y^Y] ^ ^• 

In what follows we shall suppose that F = 0, and that X — ^. 
The solution for y is 

^ {A-p'L + iap)(G''P'N + iyp)^(B'-p'M + tfipy'"^^^' 

If the connection between x and y be of a loose character, the 
constants Jf, /8, B are small, so that the term (B — p^M + ifipY 
in the denominator may in general be neglected. When this 
is permissible, the co-ordinate y is the same as if a; had been pre- 
vented firom varying, and a force Y had been introduced whose 
magnitude is independent of N, 7, and C, But if, in consequence 
of an approximate isochronism between the force and one of the 
motions which become possible when ar or y is constrained to be 
zero, either A—p^L-^tap or C—p^N'\-iyp be small^ then the 
term in the denominator containing the coefficients of mutual 
influence must be retained^ being no longer relatively unimportant ; 
and the solution is accordingly of a more complicated character. 

Symmetry shews that if we had assumed X = 0, F = 6*^, we 
should have found the same value for x as now obtains for y. This 
is the Reciprocal Theorem of § 108 applied to a system capable 
of two independent motions. The string and two loads may again 
be referred to as an example. 

117. So far for an imposed force. We shall next suppose 
that it is a motion of one co-ordinate (x = ^p*) that is prescribed, 
while F=0; and for greater simplicity we shall confine ourselves 
to the case where ^ = 0. The value of y is 

y c-Np*+iyp ^^''• 

Let as now inquire into the reaction of this motion on x. 
We have 

^-"^'^^'-'^m^ <^> 


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If the real and imaginary parts of the coefficient of e^ be re- 
spectively A' and la'p, we may put 

{MB'^B)y^A'x^tix (3), 

^(G^Np^y+rfp^ ^ ^' 

It appears that the effect of the reaction of y (over and above 
what would be caused by holding y = 0) is represented by changing 
A into A + A\ and a into a + a', where A' and a' have the above 
values, and is therefore equivalent to the effect of an alteration in 
the coefficients of spring and friction. These alterations, however, 
are not constants, but functions of the period of the motion con- 
templated, whose character we now proceed to consider. 

Let n be the value otp corresponding to the natural frictionless 
period of y {x being maintained at zero); so that (7 — n*iV = 0. 

A' = (B--MT^y A^(;>--nO ] 

--iB^Mj^f ^^^^Jl^,^^^ ] 


In most cases with which we are practically concerned 7 is 
small, and interest centres mainly on values of p not much differ- 
ing from n. We shall accordingly leave out of account the 
variations of the positive factor {B — Jfjp*)*, and in the small term 
7^, substitute for p its approximate value n. When p is not 
nearly equal to n, the term in question is of no importance. 

As might be anticipated from the general principle of work, 
a' is alwajrs positive. Its maximum value occurs when jp = n 
nearly, and is then proportional to l/7n», which varies inversely 
with 7. This might not have been expected on a superficial view 
of the matter, for it seems rather a paradox that, the greater the 
friction, the less should be its result. But it must be remembered 
that 7 is only the coefficient of friction, and that when 7 is small 
the maximum motion is so much increased that the whole work 
spent against friction is greater than if 7 were more considerable. 

But the point of most interest is the dependence of A' on p, 
lip be less than n. A' is negative. As p passes through the value 

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n. A' vanishes, and changes sign. When A' is negative, the in- 
fluence of y is to diminish the recovering power of the vibration «, 
and we see that this happens when the forced vibration is slower 
than that natural to y. The tendency of the vibration y is thus 
to retard the vibration x, if the latter be already the slower, but 
to accelerate it, if it be already the more rapid, only vanishing in 
the critical case of perfect isochronism. The attempt to make x 
vibrate at the rate determined by w is beset with a peculiar 
difficulty, analogous to that met with in balancing a heavy 
body with the centre of gravity above the support. On which- 
ever side a slight departure from precision of adjustment may 
occur the influence of the dependent vibration is always to increase 
the error. Examples of the instability of pitch accompanying a 
strong resonance will come across us hereafter ; but undoubtedly 
the most interesting application of the results of this section is to 
the explanation of the anomalous refraction, by substances possess- 
ing a very marked selective absorption, of the two kinds of light 
situated (in a normal spectrum) immediately on either side of the 
absorption band^ It was observed by Christiansen and Eundt, 
the discoverers of this remarkable phenomenon, that media of the 
kind in question (for example, ^t^oA^ne in alcoholic solution) refract 
the ray immediately below the absorption-band abnormally in 
excess, and that above it in defect If we suppose, as on other 
grounds it would be natural to do, that the intense absorption is 
the result of an agreement between the vibrations of the kind of 
light affected, and some vibration proper to the molecules of the 
absorbing agent, our theory would indicate that for light of some- 
what greater period the effect must be the same as a relaxation of 
the natural elasticity of the ether, manifesting itself by a slower 
propagation and increased refraction. On the other side of the 
absorption-band its influence must be in the opposite direc- 

In order to trace the law of connection between A' and p, take, 
for brevity, 7 n = a, Nijj^ — n") = x, so that 

When the sign of a? is changed. A' is reversed with it, but pre- 
serves its numerical value. When a; = 0, or ±00 , A^ vanishes. 

1 Phil Mag,, May, 1872. Also Sellmeier, Pogg, Arm, t oxliii. p. 272, 1871. 

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Hence the origin is on the representative curve (Fig. 18), and the 
axis of a? is an asymptote. The maximum and minimum values of 
A' occur when x is respectively equal to + a, or — a ; and then 



:.= ± 


The corresponding values of p are given by 



Hence, the smaller the value of a or 7, the greater will be the 
maximum alteration of A, and the corresponding value of p wilt 
approach nearer and nearer to n. It may be well to repeat, that in 
the optical application a diminished 7 is attended by an increased 
maximum absorption. When the adjustment of periods is such as 
to fevour A' as much as possible, the corresponding value of a m 
one half of its maximum. 

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118. Among vibrating bodies there are none that occupy a 
more prominent position than Stretched Strings. From the 
earliest times they have been employed for musical purposes, 
and in the present day they still form the essential parts of such 
important instruments as the pianoforte and the violin. To the 
mathematician they must always possess a peculiar interest as the 
battle-field on which were fought out the controversies of D'Alem- 
bert, Euler, Bernoulli and Lagrange, relating to the nature of the 
solutions of partial differential equations. To the student of 
Acoustics they are doubly important. In consequence of the com- 
parative simplicity of their theory, they are the ground on which 
difficult or doubtful questions, such as those relating to the nature 
of simple tones, can be most advantageously faced ; while in the 
form of a Monochord or Sonometer, they aflFord the most generally 
available means for the comparison of pitch. 

The ' string ' of Acoustics is a perfectly uniform and flexible 
filament of solid matter stretched between two fixed points — ^in 
fact an ideal body, never actually realized in practice, though 
closely approximated to by most of the strings employed in music. 
We shall afterwards see how to take account of any small devia- 
tions from complete flexibility and uniformity. 

The vibrations of a string may be divided into two distinct 
classes, which are practically independent of one another, if the 
amplitudes do not exceed certain limits. In the first class the 
displacements and motions of the particles are longittAdinal, so 
that the string always retains its straightness. The potential 
energy of a displacement depends, not on the whole tension, but 
on the changes of tension which occur in the various parts of the 
string, due to the increased or diminished extension. In order to 

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calculate it we must koow the relation between the extension of 
a string and the stretching force. The approximate law (given by 
Hooke) may be expressed by saying that the extension varies 
as the tension, so that if I and r denote the natural and the 
stretched lengths of a string, and T the tension, 

^-■"-^ = ^ (1) 

where ^ is a constant, depending on the material and the section, 
which may be interpreted to mean the tension that would be 
necessary to stretch the string to twice its natural length, if the 
law applied to so great extensions, which, in general, it is far 
firom doing. 

119. The vibrations of the second kind are transverse ; that is 
to say, the particles of the string move sensibly in planes perpen- 
dicular to the line of the string. In this case the potential energy 
of a displacement depends upon the general tension, and the 
small variations of tension accompanying the additional stretching 
due to the displacement may be left out of account. It is here 
assumed that the stretching due to the motion may be neglected 
in comparison with that to which the string is already subject in 
its position of equilibrium. Once assured of the fulfilment of this 
condition, we do not, in the investigation of transverse vibrations, 
require to know anything further of the law of extension. 

The most general vibration of the transverse, or lateral, kind 
may be resolved, as we shall presently prove, into two sets of 
component normal vibrations, executed in perpendicular planes. 
Since it is only in the initial circumstances that there can be any 
distinction, pertinent to the question, between one > plane and 
another, it is sufficient for most purposes to regard the motion as 
entirely confined to a single plane passing through the line of the 

In treating of the theory of strings it is usual to commence 
with two particular solutions of the partial diflferential equation, 
representing the transmission of waves in the positive and nega- 
tive directions, and to combine these in such a manner as to suit 
the case of a finite string, whose ends are maintained at rest; 
neither of the solutions taken by itself being consistent with the 
existence of nodes, or places of permanent rest. This aspect of the 
question is very important, and we shall fully consider it; but it 

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seems scarcely desirable to found the solution in the first instance 
on a property so peculiar to a uniform string as the undisturbed 
transmission of waves. We will proceed by the more general 
method of assuming (in conformity with what was proved in the 
last chapter) that the motion may be resolved into normal com- 
ponents of the harmonic type, and determining their periods and 
character by the special conditions of the system. 

Towards carrying out this design the first step would naturally 
be the investigation of the partial differential equation, to which 
the motion of a continuous string is subject. But in order to 
throw light on a point, which it is most important to understand 
clearly, — the connection between finite and infinite freedom, and 
the passage corresponding thereto between arbitrary constants 
and arbitrary functions^ we will commence by following a some- 
what different course. 

120. In Chapter ill. it was pointed out that the fundamental 
vibration of a string would not be entirely altered in character, 
if the mass were concentrated at the middle point. Following 
out this idea, we see that if the whole string were divided into a 
number of small parts and the mass of each concentrated at its 
centre, we might by sufficiently multiplying the number of parts 
arrive at a system, still of finite freedom, but capable of represent- 
ing the continuous string with any desired accuracy, so far at 
least as the lower component vibrations are concerned. If the 
analytical solution for any number of divisions can be obtained, 
its limit will give the result corresponding to a uniform string. 
This is the method followed by Lagrange. 

Let I be the length, pi the whole mass of the string, so that 
p denotes the mass per unit length, T^ the tension. 

Fig. 19. 

The length of the string is divided into m + 1 equal parts (a), 
so that 

(m + l)a = Z (1). 

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At the m points of division equal masses (jjl) are supposed con- 
centrated, which are the representatives of the mass of the por- 
tions (a) of the string, which they severally bisect. The mass of 
each terminal portion of length ^a is supposed to be concentrated 
at the final points. On this understanding, we have 

(m+l)/A = /)i 


We proceed to investigate the vibrations of a string, itself 
devoid of inertia, but loaded at each of m points equidistant 
(a) from themselves and from the ends, with a mass /a. 

If i|^, ifr, V^nH-s denote the lateral displacements of the 

loaded points, including the initial and final points, we have the 
following expressions for T and F, 

J'=4/^{^i' + ^s'H-...H-t'm+iH-t'm+4 


with the conditions that '^i and y^m+n vanish. These give by 
Lagrange's Method the m equations of motion. 

Bf.+Ayfr, +Bylt, =0 
Bfn. + Air^, + Bylt^+, = 


A=fiD^ + 





Supposing now that the vibration under consideration is one 
of normal type, we assume that yjti, i^s, &c. are all proportional to 
cos(ni — e), where n remains to be determined. A and B may 
then be regarded as constants, with a substitution of — «' for D*. 

If for the sake of brevity we put 



the determinantal equation, which gives the values of n^, assumes 
the form 

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C, 1, 0, 0, 0. 

1, C, 1, 0, 0. 

0, 1. C, 1, 0. 

0, 0. 1. C. 1. 

0, 0, 0, 1, c. 

m rows 

= 0. 


From this equation the values of the roots might be fouud. 
It may be proved that, if (7= 2 cos 6y the determinant is equivalent 
to sin (774 H- 1) ^ -r sin ^ ; but we shall attain our object with greater 
ease directly from (5) by acting on a hint derived from the known 
results relating to a continuous string, and assuming for trial a 
particular type of vibration. Thus let a solution be 

yltr = P sin(r— l)/3 cos(n^ — e) 


a form which secures that 1^1 = 0. In order that -^m+s may 

(mH-l)/3 = S7r (10), 

where 8 is an integer. Substituting the assumed values of yp' in 
the equations (5), we find that they are satisfied, provided that 

2Bcosy3H-^=0 (11); 

so that the value of n in term^ of /3 is 

A normal vibration is thus represented by 

"=^«^f\/S <'')• 

tr = P.8in^-^— ^co8(M-e,) (13). 



V M 


sin in — rr^ 
fia 2 (w + 1) 


and Pgy €t denote arbitrary constants independent of the general 
constitution of the system. The m admissible values of n are 
found irom (14) by ascribing to 8 in succession the values 1, 2, 
d...7n, and are all different. If we take « = m+l, yp'r vanishes, 
so that this does not correspond to a possible vibration. Greater 
values of 8 give only the same periods over again. If m + 1 be 
even, one of the values of n — ^that, namely, corresponding to 

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« = ^(m + l), — is the same as would be found in the case of only 
a single load (m » 1). The interpretation is obvious. In the kind 
of vibration considered every alternate particle remains at rest, so 
that the intermediate ones really move as though they were 
attached to the centres of strings of length 2a, fastened at 
the ends. 

The most general solution is found by putting together all the 
possible particular solutions of normal type 

tr = S*"" P. sin ^^^^^ COS (n.t-e.) (15). 

and, by ascribing suitable values to the arbitrary constants, can 
be identified with the vibration resulting from arbitrary initial 

Let X denote the distance of the particle r from the end of the 
string, so that (r — l)a = a?; then by substituting for fju and a 
from (1) and (2), our solution may be written, 

'^{x) = P,sin8 J- co3(n,t — e,) (16), 

2(m + l) /5\ . sir ,,,, 

In order to pass to the case of a continuous string, we have 
only to put m infinite. The first equation retains its form, and 
specifies the displacement at any point x. The limiting form of 
the second is simply 

^ = TV7 (^^)' 

whence for the periodic time, 

"?-y^ ■ w 

The periods of the component tones are thus aliquot parts of 
that of the gravest of the series, found by putting s = h ' The 
whole motion is in all cases periodic ; and the period is 21 \/(/>/7i). 
This statement, however, must not be understood as excluding^ 
a shorter period; for in particular cases any number* of the 
lower components may be absent. All that is asserted is that the 

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above-mentioned interval of time is sufficient to bring about a com- 
plete recun'ence. We defer for the present any further discussion 
of the important formula (19), but it is interesting to observe the 
approach to a limit in (17), as m is made successively greater and 
greater. For this purpose it will be sufficient to take the gravest 
tone for which « = 1, and accordingly to trace the variation of 
2(m + l) 





The following are a series of simultaneous values of the func- 
tion and variable : — 









2(m+l) . w 








It will be seen that for very moderate values of m the limit is 
closely approached. Since m is the number of (moveable) loads, 
the case m = 1 corresponds to the problem investigated in Chapter 
III., but in comparing the results we must remember that we there 
supposed the whole mass of the string to be concentrated at the 
centre. In the present case the load at the centre is only half as 
great; the remainder being supposed concentrated at the ends, 
where it is without effect. 

From the fifict that our solution is general, it follows that any 
initial form of the string can be represented by 

-^ (^) = S (P cos €)g sin 8 





And, since any form possible for the string at all may be 
regarded as initial, we infer that any finite single valued function 
of X, which vanishes at ^ = and x = l, can be expanded within 
those limits in a series of sines of irx/l and its multiples, — which 
is a case of Fourier's theorem. We shall presently shew how the 
more general form can be deduced. 

121. We might now determine the constants for a continuous 
string by integration as in § 93, but it is instructive to solve the 
problem first in the general case (m finite), and afterwards to 
proceed to the limit. The initial conditions are 

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• / \ A ' "^^ , A • a'''^ . A ' ^^ 

• / \ >! • 'Ttt , , . ^ Tra . . >« • ^" 

where, for brevity, J., = P,co8€,, and '^(a), yjr{2a) ylt(ma) 

are the initial displacements of the m particles. 

To determine any constant Ag, multiply the first equation by 
sin (87ra/l\ the second by sin (2«7ra//), &c., and add the results. 
Then, by Trigonometry, the coefficients of all the constants, except 
At, vanish, while that of -4, = ^ (m + 1)^ Hence 

^'=^,^2^.^('-«)«"^^«r ^^>- 

We need not stay here to write down the values of Bg (equal 
to Pg sin €g) as depending on the initial velocities. When a becomes 
infinitely small, ra under the sign of summation ranges by infi- 
nitesimal steps from zero to L At the same time — — ^ = y , 
so that writing ra = iv, a==dx, we have ultimately 

^ = f£v^Wsm(?^)d^ •• <2)' 

expressing Ag in terms of the initial displacements. 

122. We will now investigate independently the partial diflfer- 
ential equation governing the transverse motion of a perfectly 
flexible string, on the suppositions (1) that the magnitude of the 
tension may be considered constant, (2) that the square of the 
inclination of any part of the string to its initial direction may be 
neglected. As before, p denotes the linear density at any point, 
and Ti is the constant tension. Let rectangular co-ordinates be 
taken parallel, and perpendicular to the string, so that x gives the 
equilibrium and x, y, z the displaced position of any particle at 
time t The forces acting on the element dx are the tensions at 

. I Todhunter'fl ItU. Calc,, p. 267. 
R. 12 

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its two ends, and any impressed forces Yp dx, Zp dx. By D'Alem- 
bert's Principle these form an equilibrating system with the 
reactions against acceleration, ^pdhfjd^, —pd^zld^. At the 
point X the components of tension are 

rpdy rpdz 
^'dx' ^'dx' 

if the squares of dy/dx, dz/dx be neglected ; so that the forces 
acting on the element dx arising out of the tension are 

<{%h- '-iii)^- 

Hence for the equations of motion. 

' (1), 

dt^ p da^ 

d^ p da?'^ ) 

from which it appears that the dependent variables y and z are 
altogether independent of one another. 

The student should compare these equations with the corre- 
sponding equations of finite differences in § 120. The latter may 
be written 

Now in the limit, when a becomes infinitely small, 
'^{x-a)'\-'>^{x'\-a)- 2i|r (a?) = i|r" (a?) a\ 
while fi = pa; and the equation assumes ultimately the form 

agreeing with (1). 

In like manner the limiting forms of (3) and (4) of § 120 are 

^"i/"®'^ • «■ 

''-''•■/(i)"'^ «• 

which may also be proved directly. 

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The first is obvious from the definition of T, To prove the 
second, it is sufficient to notice that the potential energy in any 
con6guration is the work required to produce the necessary 
stretching against the tension J\. Reckoning from the configura- 
tion of equilibrium, we have 


and, so far as the third power of -^ , 

dx * \dx) 

123. In most of the applications that we shall have to make, 
the density p is constant, there are no impressed forces, and the 
motion may be supposed to take place in one plane. We may 
then conveniently write 


j-^' a). 

and the differential equation is expressed by 

d{aty dx" ^ ^* 

If we now assume that y varies as cos ma^, our equation 

|j+wi*y = (3), 

of which the most general solution is 

. y = {Asmmx-\'GQOH7nx)co&mat (4). 

This, however, is not the most general harmonic motion of 
the period in question. In order to obtain the latter, we must 

y = yi cos mat + y, sin mat (5), 

where yi, y, are functions of x, not necessarily the same. On 
substitution in (2) it appears that yi and y, are subject to equations 
of the form (3), so that finally 

y = {A sin ma + G cos mx) cos mat ] ,^v 

+ (i?sin 7na?-hDcosm{r)sin7na^| 

an expression containing four arbitrary constants. For any con- 
tinuous length of string satisfying without interruption the differ- 


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ential equation, this is the most general solution possible, under 
the condition that the motion at every point shall be simple 
harmonic. But whenever the string forms part of a system 
vibrating freely and without dissipation, we know from former 
chapters that all parts are simultaneously in the same phase, 
which requires that 

A : B^C : D (7); 

and then the most general vibration of simple harmonic type is 

y = {a sin WW? + )9 cos wwp} cos (ma^ — €) (8). 

124. The most simple as well as the most important problem 
connected with our present subject is the investigation of the free 
vibrations of a finite string of length I held fast at both its ends. 
If we take the origin of x at one end, the terminal conditions are 
that when a? = 0, and when x^l, y vanishes for all values of t. 
The first requires that in (6) of § 123 

C=0, D = (1); 

and the second that 

sin mi = (2), 

or that mZ = «7r, where 8 is an integer. We learn that the only 
harmonic vibrations possible are such as make 

^ = T (3). 

and then 

y = sm-^(ilcos-j- +5sm— =- 1 (4). 

Now we know a priori that whatever the motion may be, it 
can be represented as a sum of simple harmonic vibrations, and 
we therefore conclude that the most general solution for a string, 
fixed at and 2, is 

y = 2^^ sm-j-|^^,cos-^ + i?,sm-pj (5). 

The slowest vibration is that corresponding to «=1. Its 
period (tj) is given by 

^.4'-^Vf. w 

The other components have periods which are aliquot parts 
of Ti : — 

T, = Ti^s (7); 

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so that, as has been already stated, the whole motion is under all 
circumstances periodic in the time Ti. The sound emitted con- 
stitutes in general a musical notey according to our definition of 
that term, whose pitch is fixed by r,, the period of its gravest 
component. It may happen, however, in special cases that the 
gravest vibration is absent, and yet that the whole motion is not 
periodic in any shorter time. This condition of things occurs, if 
jli*-h-B,« vanish, while, for example, A^-\-B^ and A^-{-B^ are 
finite. In such cases the sound could hardly be called a note; 
but it usually happens in practice that, when the gravest tone is 
absent, some other takes its place in the character of fundamental, 
and the sound still constitutes a note in the ordinary sense, 
though, of course, of elevated pitch. A simple case is when all 
the odd components beginning with the first are missing. The 
whole motion is then periodic in the time ^Tj, and if the second 
component be present, the sound presents nothing unusual. 

The pitch of the note yielded by a string (6), and the character 
of the fundamental vibration, were first investigated on mechanical 
principles by Brook Taylor in 1715 ; but it is to Daniel Bernoulli 
(1765) that we owe the general solution contained in (5). He 
obtained it, as we have done, by the synthesis of particular 
solutions, permissible in accordance with his Principle of the 
Coexistence of Small Motions. In his time the generality of the 
result so arrived at was open to question ; in fact, it was the 
opinion of Euler, and also, strangely enough, of Lagrange ^ that 
the series of sines in (5) was not capable of representing an 
arbitrary function; and Bernoulli's argument on the other side, 
drawn from the infinite number of the disposable constants, 
was certainly inadequate'. 

Most of the laws embodied in Taylor's formula (6) had been 
discovered experimentally long before (1636) by Mersenne. They 
may be stated thus : — 

^ See Riemann's PartieUe Differential Gleiehungenj § 78. 

' Dr Toang, in his memoir of 1800, seems to have understood this matter quite 
oorrectly. He says, ** At the same time, as M. Bernoulli has justly observed, since 
every figure may be infinitely approximated, by considering its ordinates as 
composed of the ordinates of an infinite number of trochoids of different magni- 
tudes, it may be demonstrated that all these constituent curves would revert to 
their initial state, in the same time that a similar chord bent into a trochoidal 
curve would perform a single vibration ; and this is in some respects a convenient 
and compendious method of considering the problem." 

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( 1) For a given string and a given tension, the time varies as 
the length. 

This is fphe fundamental principle of the monochord, and 
appears ta have been understood by the ancients^ 

(2) When the length of the string is given, the time varies 
iDversely as the square root of the tension. 

(S) Strings of the same length and tension vibrate in times, 
which are proportional to the square roots of the linear density. 

These important results may all be obtained by the method of 
dimensions, if it be assumed that t depends only on I, />, and Tj. 

For, if the units of length, time and mass be denoted re- 
gpectively by [i], [T], [if], the dimensions of these symbols are 
given by 

i = [Z], p = [JlfX-a Z = [MLT^], 
and thus (see § 52) the only combination of them capable of re- 
presenting a time is Tr^.p^.l, The only thing left undetermined 
is the numerical £eictor. 

125. Mersenne's laws are exemplified in all stringed instru- 
ments. In playing the violin diflferent notes are obtained from 
the same string by shortening its efficient length. In tuning 
the violin or the pianoforte, an adjustment of pitch is eflFected 
with a constant length by varying the tension ; but it must be 
remembered that p is not quite invariable. 

To secure a prescribed pitch with a string of given material, it is 
requisite that one relation only be satisfied between the length, the 
thickness, and the tension; but in practice there is usually no great 
latitude. The length is often limited by considerations of con- 
venience, and its curtailment cannot always be compensated by 
an increase of thicknea*^, because, if the tension be not increased 
proportionally to the section, there is a loss of flexibility, 
while if the tension be so increased, nothing is effected towards 
lowering the pitch. The diflficulty is avoided in the lower strings 
of the pianoforte and violin by the addition of a coil of fine wire, 
whose effect is to impart inertia without too much impairing 

^ Aristotle ** knew that a pipe or a chord of double length produced a sound of 
which the yibratioDs occupied a double time; and that the properties of concords 
depended on the proportions of the times occupied by the vibrations of the 
aeparate aoundfl." — Young's Lectures on Natural Philosophy , VoL i. p. 404, 

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125.] mersenne's laws. 183 

For quantitative investigations into the laws of strings, the 
sonometer is employed. By means of a weight hanging over a 
pulley, a catgut, or a metallic wire, is stretched across two bridges 
mounted on a resonance case. A moveable bridge, whose position 
is estimated by a scale running parallel to the wire, gives the 
means of shortening the efficient portion of the wire to any 
desired extent. The vibrations may be excited by plucking, as 
in the harp, or with a bow (well supplied with rosin), as in the 

If the moveable bridge be placed half-way between the fixed 
ones, the note is raised an octave ; when the string is reduced to 
one-third, the note obtained is the twelfth. 

By means of the law of lengths, Mersenne determined for the 
first time the frequencies of known musical notes. He adjusted the 
length of a string until its note was one of assured position in the 
musical scale, and then prolonged it under the same tension until 
the vibrations were slow enough to be counted. 

For experimental purposes it is convenient to have two, or 
more, strings mounted side by side, and to vary in turn their 
lengths, their masses, and the tensions to which they are subjected. 
Thus in order that two strings of equal length may yield the 
interval of the octave, their tensions must be in the ratio of 1 : 4, 
if the masses be the same ; or, if the tensions be the same, the 
masses must be in the reciprocal ratio. 

The sonometer is very useful for the numerical determination 
of pitch. By varying the tension, the string is tuned to unison 
with a fork, or other standard of known frequency, and then by 
adjustment of the moveable bridge, the length of the string is 
determined, which vibrates in unison with any note proposed for 
measurement. The law of lengths then gives the means of 
effecting the desired comparison of firequencies. 

Another application by Scheibler to the determination of 
absolute pitch is important. The principle is the same as that 
explained in Chapter ill., and the method depends on deducing 
the absolute pitch of two notes from a knowledge of both the 
ratio and the difference of their frequencies. The lengths of the 
sonometer string when in unison with a fork, and when giving with 
it four beats per second, are carefully measured. The ratio of the 

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lengths is the inverse ratio of the frequencies, and the diflTerence 
of the frequencies is four. From these data the absolute pitch of 
the fork can be calculated. 

The pitch of a string may be calculated also by Taylor's 
formula from the mechanical elements of the system, but 
great precautions are necessary to secure accuracy. The tension 
m produced by a weight, whose mass (expressed with the same 
unit as p) may be called P; so that Ti=gP, where g = 32% 
if the units of length and time be the foot and the second. In 
order to secure that the whole tension acts on the vibrating 
segment, no bridge must be interposed, a condition only to be 
satisfied by suspending the string vertically. After the weight is 
attached, a portion of the string is isolated by clamping it firmly 
at two points, and the length is measured. The mass of the unit 
of length p refers to the stretched state of the string, and may be 
found indirectly by observing the elongation due to a tension 
of the same order of magnitude as 7\, and calculating what 
would be produced by T^ according to Hooke's law, and by 
weighing a known length of the string in its normal state. 
After the clamps have been secured great care is required to 
avoid fluctuations of temperature, which would seriously influence 
the tension. In this way Seebeck obtained very accurate results. 

126. When a string vibrates in its gravest normal mode, the 
excursion is at any moment proportional to sin (irx/ 1), increasing 
numerically from either end towards the centre ; no intermediate 
point of the string remains permanently at rest. But it is other- 
wise in the case of the higher normal components. Thus, if the 
vibration be of the mode expressed by 

. STTX ( . sirat n ' 8wat\ 
y = Qm—^{AtCOB—j — hi>«sm— y- j , 

the excursion is proportional to sin (sttx/I), which vanishes at « — 1 
points, dividing the string into s equal parts. These points of no 
motion are called nodes, and may evidently be touched or held 
fast without in any way disturbing the vibration. The produc- 
tion of * harmonics ' by lightly touching the string at the points of 
aliquot division is a well-known resource of the violinist. All 
component modes are excluded which have not a node at the 
point touched ; so that, as regards pitch, the efl^ect is the same as 
if the string were securely fastened there. 

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127. The constants, which occur in the general value of y, 
§ 124, depend on the special circumstances of the vibration, and 
may be expressed in terms of the initial values of y and y. 

Putting ^ = 0, we find 

yo = X,^i il,sin j-\ . yo= y 2,-i «^# sin -y- . 



Multiplying by sin— r-, and integrating fix)m to Z, we obtain 

. 2 r^ . 8irx J ^ 2 r' . . sirx , .^. 

A.^jj^y,^-^dx', B.^—j^yoSm-^dx (2). 

These results exemplify Stokes' law, § 95 ; for that part of y, which 
depends on the initial velocities, is 

'^t-* 2 . STTX . swat r' . . STTX , 

and from this the part depending on initial displacements may 
be inferred, by differentiating with respect to the time, and 
substituting y^ for y«. 

When the condition of the string at some one moment is 
thoroughly known, these formulae allow us to calculate the 
motion for all subsequent time. For example, let the string be 
initially at rest, and so displaced that it forms two sides of a 
triangle. Then J?« = ; and 

Fig. 20. 

. 2y(f^x, airx , f^ l—x . airx , ) 


. STrh 


on integration. 

We see that -4, vanishes, if sin (sirb/l) = 0, that is, if there be 
a node of the component in question situated at P, A more 
comprehensive view of the subject will be afforded by another 
mode of solution to be given presently. 

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128. In the expression for y the coefficients of sin (sirx/l) are 
the normal co-ordinates of Chapters iv. and V. We will denote 
them therefore by ^«, so that the configuration and motion of the 
t^ystem at any instant are defined by the values of <^< and ^« 
according to the equations 

y = <^iSin-=- + ^aSm-y- + ...+<^fSm-^ + ... 

^ ^ \ ......(1). 

y = <pi8m-y + ^,8m -^+ ... + 4>«sm-2- + ... I 

We proceed to form the expressions for T and F, and thence 
to deduce the normal equations of vibration. 

For the kinetic energy, 

T = ip/^' y'cfo = ip £ {s;:: ^. sin *7}'(ir 

= i/o j 2,^1 <^,» sm» -J- dx, 

the product of every pair of terms vanishing by the general 
property of normal co-ordinates. Hence 

T = ipl'Z',l'^.'' (2). 

In like manner, 




' dx 


=mx::^<t>'' (3). 

These expressions do not presuppose any particular motion, either 
natural, or otherwise; but we may apply them to calculate the 
whole energy of a string vibrating naturally, as follows : — ^If M 
be the whole mass of the string (p[), and its equivalent (a*/t>) be 
substituted for Tu we find for the sum of the energies, 

2'+F=iif.2;:r{<^.'-.^^ (4), 

or, in terms of Ag and Bg of § 126, 

T+v^-.'ifX::^^^ (5)- 

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128.] young's theorem. 187 

If the motion be not confined to the plane of xy^ we have 
merely to add the energ}' of the vibrations in the perpendicular 

Lagrange's method gives immediately the equation of motion 

*-+(?)"*-l*- »■ 

which has been already considered in § 66. If <f>o and ^o be the 
initial values of <^ and <^, the general solution is 

. • sinn^ . 
9 = 4*0 ^ 9o cos nt 

^^{^^n{t-^1f)^dlf (7), 

Ifm jo 

where n is written for STrajL 

By definition 4>« is such that <!>« Btfyg represents the work done 
by the impressed forces on .the displacement B<f>g. Hence, if the 
force acting at time ^ on an element of the string pdxhe p Ydx, 

<I>, = fpFsin?^(ir (8). 


In these equations ^t is a linear quantity, as we see from (1); and 
4>, is therefore a force of the ordinary kind. 

129. In the applications that we have to make, the only 
impressed force will be supposed to act in the immediate neigh- 
bourhood of one point a=^b, and may usually be reckoned as 
a whole, so that 

<!>, = sin ^jpFda: (1). 

If the point of application of the force coincide with a node of 
the mode (*), <1>, = 0, and we learn that the force is altogether 
without influence on the component in question. This principle 
is of great importance ; it shews, for example, that if a string be 
at rest in its position of equilibrium, no force applied at its centre, 
whether in the form of plucking, striking, or bowing, can generate 
any of the even normal components ^ If after the operation of 
the force, its point of application be damped, as by touching it 

1 The observation that a harmonio is not generated, when one of its nodal 
points is placked, is dae to Tonng. 

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with the finger, all motion must forthwith cease ; for those com- 
ponents which have not a node at the point in question are 
stopped by the damping, and those which have, are absent from 
the beginning^ More generally, by damping any point of a 
sounding string, we stop all the component vibrations which have 
not, and leave entirely unaffected those which have a node at the 
point touched. 

The case of a string pulled aside at one point and afterwards 
let go from rest may be regarded as included in the preceding 
statements. The complete solution may be obtained thus. Let 
the motion commence at the time ^ = 0; from which moment 
^s = 0. The value of <^, at time t is 

<^« = (^«)ocosne + -(<^,)o8inn< (2), 

where {<Pt)o» {^»)o denote the initial values of the quantities 
affected with the suffix s. Now in the problem in hand (^«)« = 0, 
and {(t>g)o is determined by 

„.(<^.)..2^.= ^rsin?^ (3). 

if Y' denote the force with which the string is held aside at the 
point b. Hence at time t 

y = rp^ -S^ «in -^sin -J- -^ (o). 

and by (1) of §128 

where n = 87ra/L 

The S3rmmetry of the expression (5) in x and 6 is an example 
of the principle of § 107. 

The problem of determining the subsequent motion of a string 
set into vibration by an impulse acting at the point 6, may be 
treated in a similar manner. Integrating (6) of § 128 over the 
duration of the impulse, we find ultimately, with the same nota- 
tion as before, 

... 2 . sirb ^ 
(</>,), = ^sm-y-F„ 

^ A like resnlt ensnes when the point which is damped is at the same distance 
from one end of the string as the point of excitation is from the other end. 

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if IT'dt be denoted by F,. At the same time (^,)o = 0, so that by 

<2) at time t 

.. 2F, ^. . mrb . nrx sinnf . 



The series of component vibrations is less convergent for a struck 
than for a plucked string, as the preceding expressions shew. 
The reason is that in the latter case the initial value of y is 
continuous, and only dy/dx discontinuous, while in the former it 
is y itself that makes a sudden spring. See §§ 32, 101. 

The problem of a string set in motion by an impulse may also 
be solved by the general formulae (7) and (8) of § 128. The force 
finds the string at rest at ^ = 0, and acts for an infinitely short 
time fix>m ^ = to t = T\ Thus (^t)o and (<^,)o vanish, and (7) 
of § 128 reduces to 

while by (8) of §128 


Hence, as before, 






rdf' = 8iD?y F,. 

, 2 17. . 8wb . - 


Hitherto we have supposed the disturbing force to be concen- 
trated at a single point. If it be distributed over a distance ^ 
on either side of 6, we have only to integrate the expressions (6) 
and (7) with respect to 6, substituting, for example, in (7) in place 
of Yism{87rb/l), 

Yi sm -=- db. 

b-fi ^ 

If F/ be constant between the limits, this reduces to 


^,21 . sir 8 . sirb 
Yi — sm —Y- sm -7- 
sir I I 


The principal effect of the distribution of the force is to render 
the series for y more convergent. 

130. The problem which will next engage our attention is 
that of the pianoforte wire. The cause of the vibration is here 
the blow of a hammer, which is projected against the string, and 

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after the impact rebounds. But we should not be justified in 
assuming, as in the last section, that the mutual action occupies 
so short a time that its duration may be neglected. Measured by 
the standards of ordinary life the duration of the contact is indeed 
very small, but here the proper comparison is with the natural 
periods of the string. Now the hammers used to strike the wires 
of a pianoforte are covered with several layers of cloth for the 
express purpose of making them more yielding, with the eflTect of 
prolonging the contact. The rigorous treatment of the problem 
would be diiBcult, and the solution, when obtained, probably too 
complicated to be of use ; but by introducing a certain simplifica- 
tion Helmholtz has obtained a solution representing all the 
essential features of the case. He remarks that since the actual 
yielding of the string must be slight in comparison with that of 
the covering of the hammer, the law of the force called into play 
during the contact must be nearly the same as if the string were 
absolutely fixed, in which case the force would vary very nearly as 
a circular function. We shall therefore suppose that at the time 
^ = 0, when there are neither velocities nor displacements, a force 
Fsiapt begjns to act on the string &tx = b, and continues through 
half a period of the circular function, that is, until t = 7r/p, after 
which the string is once more free. The magnitude of p will 
depend on the mass and elasticity of the hammer, but not to any 
great extent on the velocity with which it strikes the string. 

The required solution is at once obtained by substituting for 
<J>, in the general formula (7) of § 128 its value given by 

4>, = jF sin^sinpt' (1), 

the range of the integration being from to ir/p. We find 



6. = 1 — sm -y- I &inn(t — t) sin pt at 

^ Inp I Jo 


'.-i — 7-- — ^. .jFsm-v- .sm 



and the final solution for y becomes, if we substitute for n and p 

their values, 

aiT^a . sirb 

(*f\Q Sin '^■^~ 

^apl'F ^»~m 2pl ' I . 8irx . 8Tra( ir\ .^. 

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We see that all components vanish which have a node at the 
point of excitement, but this conclusion does not depend on any 
particular law of force. The interest of the present solution lies 
in the information that may be elicited from it as to the depend- 
ence of the resulting vibrations on the duration of contact. If 
we denote the ratio of this quantity to the fundamental period of 
the string by v, so that v^ira: 2pl, the expression for the ampli- 
tude of the component 8 is 


V cos {STTV) . «7r6 


We fall back on the case of an impulse by putting i/=0, 



P ' 

When J/ is finite, those components disappear, whose periods 
are |, |, f, ... of the duration of contact; and when 8 is very 
great, the series converges with s~'. Some allowance must also 
be made for the finite breadth of the hammer, the effect of which 
will also be to favour the convergence of the series. 

The laws of the vibration of strings may be verified, at least 
in their main features, by optical methods of observation — either 
with the vibration-microscope, or by a tracing point recording the 
character of the vibration on a revolving drum. This character 
depends on two things, — the mode of exciten^ent, and the point 
whose motion is selected for observation. Those components do 
not appear which have nodes either at the point of excitement, or 
at the point of observation. The former are not generated, and 
the latter do not manifest themselves. Thus the simplest motion 
is obtained by plucking the string at the centre, and observing 
one of the points of trisection, or vice versa. In this case the 
first harmonic which contaminates the purity of the principal 
vibration is the fifth component, whose intensity is usually in- 
sufficient to produce much disturbance. 

[The dynamical theory of the vibration of strings may be 
employed to test the laws of hearing, and the necessary experi- 
ments are easily carried out upon a grand pianoforte. Having 
freed a string, say c, from its damper by pressing the digital, pluck 
it at one-third of its length. According to Young's theorem the 
third component vibration is not excited then, and in corre- 

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spondence with that fact the ear fails to detect the component ^. 
A slight displacement of the point plucked brings ^ in again; 
and if a resonator {g'^ be used to assist the ear, it is only with 
difficulty that the point can be hit with such precision as entirely 
to extinguish the tone. Experiments of this kind shew that the 
ear analyses the sound of a stiing into precisely the same con- 
stituents as are found by sympathetic resonance, that is, into 
simple tones, according to Ohm's definition of this conception. 
Such experiments are also well adapted to shew that it is not a 
mere play of imagination when we hear overtones, as some people 
believe it is on hearing them for the first time\ 

If, after the string has been sounded loudly by striking the 
digital, it be touched with the finger at one of the points of 
trisection, all components are stopped except the 3rd, 6th, &c., so 
that these are left isolated. The inexperienced observer is usually 
surprised by the loudness of the residual sound, and begins to 
appreciate the large part played by overtones.] 

131. The case of a periodic force is included in the general 
solution of § 128, but we prefer to follow a somewhat different 
method, in order to make an extension in another direction* We 
have hitherto taken no account of dissipative forces, but we will 
now suppose that the motion of each element of the string is 
resisted by a force proportional to its velocity. The partial 
differential equation becomes 



by means of which the subject may be treated. But it is still 
simpler to avail ourselves of the results of the last chapter, 
remarking that in the present case the dissipation-function F is 
of the same form as T. In fact 



where 0i, <f>2,... are the normal co-ordinates, by means of which 

T and V are reduced to sums of squares. The equations of 

motion are therefore simply 

4>i + fC(l>, + n^<f>t=-^<Ps (3), 

1 Helmholtz, Ch. it. ; Brandt, Pogg. Ann., Vol. czii. p. 324, 1861. 

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of the same form as obtains for systems with but one degree of 
freedom. It is only necessary to add to what was said in 
Chapter in., that since sc ib independent of s, the natural vibra- 
tions subside in such a manner that the amplitudes maintain their 
relative values. 

If a periodic force Fcoapt act at a single point, we have 

<I>, = ^sin-,- Gospt (4), 

and §46 0,= IJ^^^^T ^^(^^"^) (^)' 

where tan€= ^ — r (6). 

If among the natural vibrations there be any one nearly 
isochronous with cos jot, then a large vibration of that type will 
be forced, unless indeed the point of excitement should happen to 
fall near a node. In the case of exact coincidence, the component 
vibration in question vanishes ; for no force applied at a node can 
generate it, under the present law of friction, which however, it 
may be remarked, is very special in character. If there be no 
friction, ic = 0, and 

lp4>, = -~--~ sm-^- cos pt (/), 

which would make the vibration infinite, in the case of perfect 
isochronism, unless sin (sTrb/l) = 0. 

The value of y is here, as usual, 

y = ^sm-^ + 0a8m y- + ^,sm -/-+ (8). 

132. The preceding solution is an example of the use of 
normal co-ordinates in a problem of forced vibrations. It is of 
course to free vibrations that they are more especially applicable, 
and they may generally be used with advantage throughout, 
whenever the system after the operation of various forces is 
ultimately left to itself. Of this application we have already had 

In the case of vibrations due to periodic forces, one advantage 
of the use of normal co-ordinates is the facility of comparison with 
the equUxbrium theory^ which it will be remembered is the theory 
R. 13 

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of the motion on the supposition that the inertia of the system 
may be left out of account. If the value of the normal co-ordinate 
0, on the equilibrium theory be A g cos pt, then the actual value 
will be given by the equation 


0, = - 

^ cos pt. 


so that, when the result of the equilibrium theory is known and 
can readily be expressed in terms of the normal co-ordinates, the 
true solution with the effects of inertia included can at once be 
written down. 

In the present instance, if a force F cos pt of very long period 
act at the point b of the string, the result of the equilibrium 
theoiy, in accordance with which the string would at any moment 
consist of two straight portions, will be 

- ^ 2F . sirb 


from which the actual result for all values of p is derived by simply 
writing (w* — p^) in place of n\ 

The value of y in this and similar cases may however be 
expressed in finite terms, and the difficulty of obtaining the 
finite expression is usually no greater than that of finding the 
form of the normal functions when the system is free. Thus in 
the equation of motion 

dt' "" d^^^' 

suppose that Y varies as cos mat The forced vibration will then 

S+-!'-l.r W 

If F= 0, the investigation of the normal functions requires the 
solution of 

and a subsequent determination of m to suit the boundar}'' con- 
ditions. In the problem of forced vibrations m is given, and we 
have only to supplement any particular solution of (3) with the 
complementary function containing two arbitrary constants. This 
function, apart from the value of m and the ratio of the constants^ 

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is of the same form as the normal functions ; and all that remains to 
be effected is the determination of the two constants in accordance 
with the prescribed boundary conditions which the complete 
solution must satisfy. Similar considerations apply in the case 
of any continuous system. 

133. If a periodic force be applied at a single point, there are 
two distinct problems to be considered; the first, when at the 
point ^ = 6, a given periodic force acts ; the second, when it is the 
actual motion of the point b that is obligatory. But it will be 
convenient to treat them together. 

The usual differential equation 

dl?^" dt " da^ ^^^' 

is satisfied over both the parts into which the string is divided at 
h, but is violated in crossing from one to the other. 

In order to allow for a change in the arbitrary constants, we 
must therefore assume distinct expressions for y, and afterwards 
introduce the two conditions which must be satisfied at the point 
of junction. These are 

(1) That there is no discontinuous change in the value of y ; 

(2) That the resultant of the tensions acting at h balances the 
impressed force. 

Thus, if J?* cos pt be the force, the second condition gives 

r,A(^)+^cosp^=:0 (2), 

where A{dy/dx) denotes the alteration in the value of dy/dx 
incurred in crossing the point x=b in the positive direction. 

We shall, however, find it advantageous to replace cospt by 
the complex exponential 6*^^ and finally discard the imaginary 
part, when the symbolical solution is completed. On the assump- 
tion that y varies as e^^, the differential equation becomes 

S+'^'^=<^ <3>' 

where \* is the complex constant, 




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The most general solution of (3) consists of two terms, pro- 
portional respectively to sinX^, and cosXa;; but the condition to 
be satisfied at a^sO shews that the second does not occur here. 
Hence if 7 6*** be the value of y at a? = 6, 

sinXd? .^ ,^. 

y^'^i^^-'^ <^>' 

is the solution applying to the first part of the string from x—0 
to x^b. In like manner it is evident that for the second part we 

shall have 

sm\(l'-x) .^ 

y-'^si^w^b)'^ <«> 

If 7 be given, these equations constitute the symbolical solution 
of the .problem ; but if it be the force that is given, we require 
further to know the relation between it and 7. 

Differentiation of (5) and (6) and substitution in the equation 
analogous to (2) gives 

F sinXfc si n \ (? — 6) 
'^'T, \~si^id ^^^• 


_ F si nXj; 8inX(t — 6) ^^^ 
*^""Fi XsinAi 

from x^O to x^b 

^Fein \(l — x) sin \b ^ 
^""Ti XsinXZ ^ 


from x=ib to x^l 

These equations exemplify the general law of reciprocity 
proved in the last chapter ; for it appears that the motion at x 
due to the force at b is the same as would have. been found at i, 
had the force acted at x. 

In discussing the solution we will take first the case in which 
there is no friction. The coefficient sc is then zero ; while X is 
real, and equal to p/a. The real part of the solution, correspond- 
ing to the force F cob pt, is found by simply putting cospt for ^ 
in (8), but it seems scarcely necessary to write the equations again 
for the sake of so small a change. The same remark applies to 
the forced motion given in terms of 7. 

It appears that the motion becomes infinite in case the force 
^ Donkin'8 Acoutticif p. 121. 

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is isochronous with one of the natural vibrations of the entire 
string, unless the point of application be a node ; but in practice 
it is not easy to arrange that a string shall be subject to a force 
of given magnitude. Perhaps the best method would be to attach 
a small mass of iron, attracted periodically by an electro-magnet, 
-whose coils are traversed by an intermittent current. But unless 
some means of compensation were devised, the mass would have 
to be veiy small in order to avoid its inertia introducing a new 

A better approximation may be obtained to the imposition of 
an obligatory motion. A massive fork of low pitch, excited by 
a bow or sustained in permanent operation by electro-magnetism, 
executes its vibrations in approximate independence of the re- 
actions of any light bodies which may be connected with it. In 
order therefore to subject any point of a string to an obligatory 
transverse motion, it is only necessary to attach it to the extremity 
of one prong of such a fork, whose plane of vibration is perpendicular 
to the length of the string. This method of exhibiting the forced 
vibrations of a string appears to have been first used by Melded 

Another arrangement, better adapted for aural observation, 
has been employed by Helmholtz. The end of the stalk of a 
powerful tuning-fork, set into vibration with a bow, or otherwise, 
is pressed against the string. It is advisable to file the surface, 
which comes into contact with the string, into a suitable (saddle- 
shaped) form, the better to prevent slipping and jarring. 

Referring to (5) we see that, if sin 7d> vanished, the motion 
(according to this equation) would become infinite, which may be 
taken to prove that in the case contemplated, the motion would 
really become great, — so great that corrections, previously insigni- 
ficant, rise into importance. Now sin X6 vanishes, when the force 
is isochronous with one of the natural vibrations of the first part 
of the string, supposed to be held fixed at and b. 

When a fork is placed on the string of a monochord, or other 
instrument properly provided with a sound-board, it is easy to 
find by trial the places of maximum resonance. A very slight 
displacement on either side entails a considerable falling off in the 
volume of the sound. The points thus determined divide the 
string into a number of equal parts, of such length that the 
natural note of any one of them (when fixed at both ends) is 

1 Pogg. Ann. cix. p. 198, 1869. 

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the same aa the note of the fork, as may readily be verified. The 
important applications of resonance which Helmholtz has made to 
purify a simple tone from extraneous accompaniment will occupy 
OUT attention later. 

134. Returning now to the general case where \ is complex, 
we have to extract the real parts from (5), (6), (8) of § 133. Far 
this purpose the sines which occur as factors, must be reduced to 
the form Re^. Thus let 

sinXa? = i2a.6**«..* (1), 

with a like notation for the others. From (3) § 133 we shall thus 



from a? 8= to a? = 6, 
and from (6) § 133 


y = 7 1^ cos (pt + e,-x - €i^\ 

from x — btox = l, 

corresponding to the obligatory motion y = y cospt at b. 

By a similar process from (8) § 133, if 

X = a + i/3 (3), 

we should obtain 

from a? = to a7 = 6 

y=r, V(«'+/3')'ig^ '''"(^*"^'"^'^'^"""^°"'^^^°^) 


from a? = 6 to a? = ? 

corresponding to the impressed force F cos pt at 6. It remains to 
obtain the forms of Rx, e^, &c. 

The values of o and fi are determined by 

«»-^ = g. 2«^ = -f (5). 

and sin Xo; = sin our cos ifix + cos ax sin %/3x 

= sin ax s 1- 1 cos ax ^ . 


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SO that 

R,- = siu*ax {^'■^^--')\ci^*wc ( ^Y " )'••• (6)' 



cot cu; 

V(a»-h)8»)=:--y(p^ +;)>)«») 


This completes the solution. 

If the friction be very small, the expressions may be simpli- 
fied. For instance, in this case, to a sufficient approximation, 

so that, corresponding to the obligatory motion at 6 y = 7 cos/>^, the 
amplitude of the motion between ^ = and a; = 6 is, approximately 

a 4a* c 

.\pb . #c^6* .pb 

n. iLn* n. 



which becomes great, but not infinite, when sin {phia) = 0, or the 
point of application is a node. 

If the imposed force, or motion, be not expressed by a single 
harmonic term, it must first be resolved into such. The preceding 
solution may then be applied to each component separately, and 
the results added together. The extension to the case of more than 
one point of application of the impressed forces is also obvious. 
To obtain the most general solution satisfying the conditions, the 
expression for the natural vibrations must also be added; but 
these become reduced to insignificance after the motion has been 
in progress for a sufficient time. 

The law of friction assumed in the preceding investigation is 
the only one whose results can be easily followed deductively, and 
it is sufficient to give a general idea of the effects of dissipative 
forces on the motion of a string. But in other respects the con- 
clusions drawn from it possess a fictitious simplicity, depending on 
the fact that F — the dissipation-function — is similar in form to T, 
which makes the normal co-ordinates independent of each other. 

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Id almofifc any other case (for example, when but a single point of 
the string is retarded by friction) there are no normal co-ordinates 
properly so called. There exist indeed elementary types of vibra- 
tion into which the motion may be resolved, and which are 
perfectly independent, but these are essentially different in cha- 
racter from those with which we have been concerned hitherto, for 
the various parts of the system (as affected by one elementary 
vibration) are not simultaneously in the same phase. Special cases 
excepted, no linear transformation of the co-ordinates (with real 
coefficients) can reduce T, F, and V together to a sum of 

If we suppose that the string has no inertia, so that 7^ = 0, 
F and V may then be reduced to sums of squares. This problem 
is of no acoustical importance, but it is interesting as being 
mathematically analogous to that of the conduction and radiation 
of heat in a bar whose ends are maintained at a constant tem- 

136. Thus far we have supposed that at two fixed points, 
^ = and x^l, the string is held at rest. Since absolute fixity 
cannot be attained in practice, it is not without interest to inquire 
in what manner the vibrations of a string are liable to be modified 
by a yielding of the points of attachment; and the problem 
will furnish occasion for one or two remarks of importance. 
For the sake of simplicity we shall suppose that the system is 
symmetrical with reference to the centre of the string, and that 
each extremity is attached to a mass M (treated as unextended in 
space), and is urged by a spring (/i) towards the position of equi- 
librium. If no fiictional forces act, the motion is necessarily 
resolvable into normal vibrations. Assume 

y = {a sin wkc + i8 cos 7?w;} cos(ma^- e) (1). 

The conditions at the ends are that 

when a? = 0, Jlfy + /iy= 2\^] 

7^ (2), 

when a? = Z, My-\-fiy^-T^^] 

which give 

?. — ^ tan mZ — a _ M — Mdhrt} , . 

/8~atanmZ + /S mT7~ ^ 

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two equations, sufiScient to detennine m, and the ratio of )8 to a. 
Eliminating the latter ratio, we find 

tan mi as y-— J (4), 

if for brevity we write v for jp . 

Equation (3) has an infinite number of roots, which may be 
found by writing tan for v, so that tan ml == tan 20, and the result 
of adding together all the corresponding particular solutions, each 
with its two arbitrary constants a and e, is necessarily the most 
general solution of which the problem is capable, and is therefore 
adequate to represent the motion due to an arbitrary initial dis- 
tribution of displacement and velocity. We infer that any function 
of X may be expanded between x^Q and ^ = Z in a series of terms 

^ (vi ainmi^ + cos rti^x) + 0, {v^ sin m^ + cos m^) -h (5), 

mi, 772,, &c. being the roots of (3) and y^, v^, &c. the corresponding 
values of v. The quantities ^i, ^, &c. are the normal co-ordinates 
of the system. 

From the symmetry of the sjrstem it follows that in each 
normal vibration the value of y is numerically the same at points 
equally distant from the micldle of the string, for example, at the 
two ends, where a? = and x^L Hence v, sin mj, H- cos mJL = ± 1 , 
as may be proved also from (4). • 

The kinetic energy T of the whole motion is made up of the 
energy of the string, and that of the masses M, Thus 

T^\p\ \%^(ymimx-\-Go&ma)Ydx 


+ iJf {<^ -h </>,+ ...}» + iJf {<^i (i/i sin miZ -h cos miO + ... 1^ 

But by the characteristic property of normal co-ordinates, terms 
containing their products cannot be really present in the expres- 
sion for Ty so that 

p I (Pr sin mfX + cos mrx) (i/, sin mgX + cos myx) dx 

+ M + M(vrsmmfl -^ coswrl) (vgsijimgl + cosm^ = (6), 

if r and 8 be different. 

This theorem suggests how to determine the arbitrary con- 

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fitants, so that the series (5) may represent an arbitrary function 
y. Take the- expression 

pi y{vt sin m^ + cos m^)dx + My^ + Myi (v, sin m^ + cos m/). . .(7), 

and substitute in it the series (5) expressing y. The result is a 
series of terms of the type 

pi ^r {vr BiT^ 7n^ + cos inja) {pg sin msX + cos m^)dx 

+ M(l>r + Jf0r (j'r siu rWyZ + COS TTifl) (vg sin m,? + COS mj^), 

all of which vanish by (6), except the one for which r=«. Hence 
<f>g is equal to the expression (7) divided by 

p I (v,sinm,a? + cosmja:)^da? + Jf+ Jf(i/,sin7?iaZ + cosm^)^..(8), 

and thus the coeflScients of the series are determined. If Jf = 0, 
even although fi be finite, the process is of course much simpler, 
but the unrestricted problem is instructive. So much stress is 
often laid on special proofs of Fourier's and Laplace's series, that 
the student is apt to acquire too contracted a view of the nature 
of those important results of analysis. 

We shall now shew how Fourier's theorem in its general form 
can be deduced from our present investigation. Let ilf = ; then 
if /i = 00 , the ends of the string are fast, and the equation de- 
termining m becomes tan ml = 0, or r)il = sw, as we know it must 
be. In this case the series for y becomes 

, . irx . . 27ra? . . Zirx ,^. 

y = -dism-y- + ^jsm -y- +-d88m-y- + (9), 

which must be general enough to represent any arbitrary functions 
of X, vanishing at and I, between those limits. But now suppose 
that /i is zero, M still vanishing. The ends of the string may be 
supposed capable of sliding on two smooth rails perpendicular to 
its length, and the terminal condition is the vanishing of dyjdx. 
The equation in m is the same as before; and we learn that any 
function y whose rates of variation vanish' at x=^Q and x^l, can 
be expanded in a series 

y =5iC08-y +-BjCos ,- +B3C0S-J- + (10). 

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This series remains unaffected when the sign of a; is changed, 
and the first series merely changes sign without altering its 
numerical magnitude. If therefore y^ be an even function of x, 
(10) represents it firom —Ito + l. And in the same way, if y be 
an odd function of x, (9) represents it between the same limita 

Now, whatever function of x (j) (x) may be, it can be divided 
into two parts, one of which is even, and the other odd, thus : 

^ W 2 ■*■ 2 ' 

so that, if <^ (x) he such that (- i) = ^ (+ 1) and ^' (- 1) = i\> (+ 0, 
it can be represented between the limits ± 2 by the mixed series 

-d^sm-j- + J^i cos -J- + -4j sm -, +52C0s-t— + (11). 

This series is periodic, with the period 21. If therefore <f> (x) 
possess the same property, no matter what in other respects its 
character may be, the series is its complete equivalent. This is 
Fourier's theorem \ 

We now proceed to examine the effects of a slight yielding of 
the supports, in the case of a string whose ends are approximately 
fixed The quantity v may be great, either through fj, or through 
M. We shall confine ourselves to the two principal cases, (1) 
when /i is great and M vanishes, (2) when /i vanishes and M is 

In the first case 


and the equation in m is approximately 

, 2 2T,m 
tan m6 = — = . 

Assume ml = 87r + x, where x is small ; then 

• tan a? = — - 



ml = sir 




^ The befit * system * for proving Fourier's theorem from dynamical oonsidera- 
tions is an endless chain stretched round a smooth cylinder (§ 189), or a thin 
re-entrant column of air enclosed in a ring-shaped tube. 

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To this order of approximation the tones do not cease to form 
a harmonic scale, but the pitch of the whole is slightly lowered. 
The effect of the yielding is in &ct the same as that of an increase 

in the length of the string in the ratio 1 : IH ^ , as might 

have been anticipated. 

The result is otherwise if fi vanish, while M is great. Here 


and tan mf = ^ ^ approximately. 

Hence m? = ^tt + , , , ^ — (13). 

Ma^ .air 

The effect is thus equiva,lent to a decrease in I in the ratio 

and consequently there is a rise in pitch, the rise being the 
greater the lower the component tone. It might be thought 
that any kind of yielding would depress the pitch of the string, 
but the preceding investigation shews that this is not the case. 
Whether the pitch will be raised or lowered, depends on the 
sign of v^ and this again depends on whether the natural note of 
the mass M urged by the spring fi is lower or higher than that of 
the pomponent vibration in question. 

136. The problem of an otherwise uniform string carrying 
a finite load M B,t x — h can be solved by the formulae investigated 
in § 133. For, if the force F cos pt be due to the reaction against 
acceleration of the mass if, 

F^yP'M. (1), 

which combined with equation (7) of § 133 gives, to determine the 
possible values of X (or p : a), 

a^MXsin-Kb sin X (i - 6) = 2\sinXi (2). 

The value of y for any normal vibration corresponding to X is 

y = P sin Xa? sin X (Z — 6) cos (aXt — e) ' 

from ic = to a? = 6 
y = P sin X (? — a;) sin X6 cos (aX^ — e) 

from x^b to x = l 
where P and € are arbitrary constants. 


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136.] FINITE LOAD. 205 

It does not require analysis to prove that any normal com- 
ponents which have a node at the point of attachment are un- 
afiFected by the presence of the load. For instance, if a string be 
weighted at the centre, its component vibrations of even orders 
remain unchanged, while all the odd components are depressed in 
pitch. Advantage may sometimes be taken of this effect of a 
load, when it is desired for any purpose to disturb the harmonic 
relation of the component tones. 

If Jlf be very great, the gravest component is widely sepa- 
rated in pitch from all the others. We will take the case when 
the load is at the centre, so that & = Z — &==^{. The equation in 
X then becomes 

. U (\Z \l pl\ ^ ... 

^2"-l"2*^2-"5fp^ ^^)' 

where pi : M, denoting the ratio of the masses of the string and 
the load, is a small quantity which may be called o^. The first 
root corresponding to the tone of lowest pitch occurs when ^X{ is 
small, and such that 

(i>i)«{l4i(i>i)*} = a» nearly, 

whence JXZ = a (1 — J a'), 

and the periodic time is given by 


v^(><i) <'>■ 

The second term constitutes a correction to the rough value 
obtained in a previous chapter (§ 52), by neglecting the inertia of 
the string altogether. That it would be additive might have 
been expected, and indeed the formula as it stands may be ob- 
tained from the consideration that in the actual vibration the two 
parts of the string are nearly straight, and may be assumed to be 
exactly so in computing the kinetic and potential energies, with- 
out entailing any appreciable error in the calculated period. On 
this supposition the retention of the inertia of the string increases 
the kinetic energy corresponding to a given velocity of the load in 
the ratio of Jf : Jf+ J^i, which leads to the above result. This 
method has indeed the advantage in one respect, as it might be 
applied when p is not uniform, or nearly uniform. All that is 
necessary is that the load M should be sufficiently predominant. 

There is no other root of (4), until sin \\l = 0, which gives 

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the second component of the string, — a vibration independent of 
the load. The roots after the first occur in closely contiguous 
pairs; for one set is given by ^Xl^sir, and the other approxi- 
mately by jXZ = «7r+— ^, in which the second term is small 
The two types of vibration for « = 1 are shewn in the figure. 

Fig. 21. 


The general formula (2) may also be applied to find the efibct 
of a small load on the pitch of the various components. 

137. Actual strings and wires are not perfectly flexible. 
They oppose a certain resistance to bending, which may be divided 
into two parts, producing two distinct effects. The first is called 
viscosity, and shews itself by damping the vibrations. This part 
produces no sensible effect on the periods. The second is con- 
servative in its character, and contributes to the potential eneray 
of the system, with the effect of shortening the periods. A com- 
plete investigation cannot conveniently be given here, but the 
case which is most interesting in its application to musical 
instruments, admits of a sufficiently simple treatment. 

When rigidity is taken into account, something more must be 
specified with respect to the terminal conditions than that v 
vanishes. Two cases may be particularly noted : — 

(i) When the ends are clamped, so that dy/dx = at the ends. 

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(ii) When the termiDal directions are perfectly free, in which 
case dh/jda? = 0. 

It is the latter which we propose now to consider. 

If there were no rigidity, the type of vibration would be 

y X sin , - , satisfying the second condition. 

The eflFect of the rigidity might be slightly to disturb the t)rpe; 
but whether such a result occur or not, the period calculated 
from the potential and kinetic energies on the supposition that 
the type remains unaltered is necessarily correct as far as the first 
order of small quantities (§ 88). 

Now the potential energy due to the stiffness is expressed by 





where £ is a quantity depending on the nature of the material 
and on the form of the section in a manner that we are not now 
prepared to examine. The forrn of SF is evident, because the force 
required to bend any element ds is proportional to ds, and to the 
amount of bending already effected, that is to ds/p. The whole 
work which must be done to produce a curvature l/p in da is 
therefore proportional to ds/p^; while to the approximation to 
which we work ds^dx, and l//) = d*y/(ic". 



Thus, if y = ^ sin -^ 

and the period of ^ is given by 

T = T,^^1-22T p) 

if To denote what the period would become if the string were 
endowed with perfect flexibility. It appears that the effect of the 
stiflhesa increases rapidly with the order of the component vibra- 
tions, which cease to belong to a harmonic scale. However, in the 
strings employed in music, the tension is usually sufiScient ta 
reduce the influence of rigidity to insignificance. 

The method of this section cannot be applied without modifi- 
cation to the other case of terminal condition, namely, when the 
ends are plamped. In their immediate neighbourhood the type of 

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vibration must differ from that assumed by a perfectly flexible 
string by a quantity, which is no longer small, and whose square 
therefore cannot be neglected. We shall return to this subject, 
when treating of the transverse vibrations of rods. 

138. There is one problem relating to the vibrations of strings 
which we have not yet considered, but which is of some practical 
interest, namely, the character of the motion of a violin (or cello) 
string under the action of the bow. In this problem the tnodus 
operandi of the bow is not sufficiently understood to allow us to 
follow exclusively the a priori method : the indications of theoiy 
must be supplemented by special observation. By a dexterous 
combination of evidence drawn from both sources Helmholtz has 
succeeded in determining the principal features of the case, but 
some of the details are still obscure. 

Since the note of a good instrument, well handled, is musical, 
we infer that the vibrations are strictly periodic, or at least that 
strict periodicity is the ideal. Moreover — and this is very import- 
ant — the note elicited by the bow has nearly, or quite, the same 
pitch as the natural note of the string. The vibrations, although 
forced, are thus in some sense free. They are wholly dependent 
for their maintenance on the energy drawn from the bow, and yet 
the bow does not determine, or even sensibly modify, their periods. 
We are reminded of the self-acting electrical interrupter, whose 
motion is indeed forced in the technical sense, but has that kind 
of freedom which consists in determining (wholly, or in part) under 
what influences it shall come. 

But it does not at once follow from the fact that the string 
vibrates with its natural periods, that it conforms to its natural 
tjrpes. If the coefficients of the Fourier expansion 

y = <^ism -^ + <^,8m-j-+ 

be taken as the independent co-ordinates by which the configura- 
tion of the system is at any moment defined, we know that when 
there is no friction, or friction such that Fee T, the natural vibra- 
tions are expressed by making each co-ordinate a simple harmonic 
(or quasi-harmonic) function of the time ; while, for all that has 
hitherto appeared to the contrary, each co-ordinate in the present 
case might be any function of the time periodic in time r. But a 

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138.] VIOLIN STRING. 209 

little examination will shew that the vibrations must be sensibly 
natural in their tjrpes as well as in their periods. 

The force exercised by the bow at its point of application may 
"be expressed by 

F= %Ar COS ( Crj ] 

so that the equation of motion for the co-ordinate ^« is 

^.+ «^#+ — p- <^, = ^sm -^ . 2^^ cos ^-^ - €rj , 

h being the point of application. Each of the component parts of 
4>, will give a corresponding term of its own period in the solu- 
tion, but the one whose period is the same as the natural period 
of ^t will rise enormously in relative importance. Practically then, 
if the damping be small, we need only retain that part of ^, 

which depends on J., cos ( e,j , that is to say, we may regard 

the vibrations as natural in their typea 

Another material fact, supported by evidence drawn both from 
theory and aural observation, is this. All component vibrations 
are absent which have a node at the point of excitation. "In 
order, however, to extinguish these tones, it is necessary that the 
coincidence of the point of application of the bow with the node 
should be very exact. A very small deviation reproduces the 
missing tones with considerable strengths" 

The remainder of the evidence on which Helmholtz' theory 
rests, was derived from direct observation with the vibration- 
microscope. As explained in Chapter li., this instrument affords 
a view of the curve representing the motion of the point under 
observation, as it would be seen traced on the surface of a trans- 
parent cylinder. In order to deduce the representative curve in 
its ordinary form, the imaginary cylinder must be conceived to 
be unrolled, or developed, into a plane. 

The simplest results are obtained when the bow is applied at a 
node of one of the higher components, and the point observed is 
one of the other nodes of the same system. If the bow work 
fairly so as to draw out the fundamental tone clearly and strongly, 
the representative curve is that shewn in figure 22; where the 

1 Donkin's Acovtvct^ p. 131. 


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abscissa} correspond to the time (AB being a complete period), 
and the ordinates represent the displacement. The remarkable 

Fig. 22. 

fact is disclosed that the whole period t may be divided into two 
parts To and t — To, during each of which the velocity of the 
observed point is constant ; but the velocities to and fro are in 
general unequal. 

We have now to represent this curve by a series of harmonic 
terms. If the origin of time correspond to the point A, and 
AD^ FC = 7, Fourier's theorem gives 

y=——/ .2 -sm— sm- It'-^] (1). 

^ tt'to (t - To) •-! «* T T V 2/ ^ ^ 

With respect to the value of t©, we know that all those com- 
ponents of y must vanish for which sin {sirx^jl) = {x^ being the 
point of observation), because under the circumstances of the case 
the bow cannot generate them. There is therefore i*eason to 
suppose that Tq:t^x^:1\ and in fact observation proves that 
AC : CB (in the figure) is equal to the ratio of the two parts into 
which the string is divided by the point of observation. 

Now the free vibrations of the string are represented in 
general by 

y = 2,-ism ^ j^,cos — +5,sm-^-k 

and this at the point x^a-^ must agree with (1). For convenience 
of comparison, we may write 

2sTrt . n . 28Trt ri 257r/ 

. 2fi7r< , o . 2«7re ^, 257r/^ To\ 
-A, cos + jB,sm = C^cos — {^— o 

T T T \ ^/ 

and it then appears that G^ = 0. 

+ ABin^(<-t), 

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138.] VIOLIN STRING. 211 

We find also to determine D, 

sin — y- . Dg - —1 — / 7 - sm -7- , 


^•-^t.(t-t,)«' ^^^' 

unless sin (sTrXo/l) = 0. 

In the case reserved, the comparison leaves D, undetermined, 
but we know on other grounds that Dg then vanishes. However, 
for the sake of simplicity, we shall suppose for the present that 
Dg is always given by (2). If the point of application of the bow 
do not coincide with a node of any of the lower components, the 
error committed will be of no great consequence. 

On this understanding the complete solution of the problem is 

The amplitudes of the components are therefore proportional to 5"^. 
In the case of a plucked string we found for the corresponding 
function 5^8in(s7r6/Z), which is somewhat similar. If the string 
be plucked at the middle, the even components vanish, but the 
odd ones follow the same law as obtains for a violin string. The 
equation (3) indicates that the string is always in the form of two 
straight lines meeting at an angle. In order more conveniently 
to shew this, let us change the origin of the time, and the constant 
multiplier, so that 

y=^2-,sm-^sm~;^ (4) 

will be the equation expressing the form of the string at any time. 

Now we know (§ 127) that the equation of the pair of lines 
proceeding from the fixed ends of the string, and meeting at a 
point whose co-ordinates are o, )8, is 

28fi ^ 1 . sva . sirx 

Thus at the time t, (4) represents such a pair of lines, meeting at 
the point whose co-ordinates are given by 



Sin ^ 

= ± 

. 2«7rf 




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These equations indicate that the projection on the axis of x 
of the point of intersection moves uniformly backwards and 
forwards between a? = and a? = Z, and that the point of inter- 
section itself is situated on one or other of two parabolic arcs, 
of which the equilibrium position of the string is a common 

Since the motion of the string as thus defined by that of the 
point of intersection of its two straight parts, has no especial 
relation to x^ (the point of observation), it follows that, according 
to these equations, the same kind of motion might be observed at 
any other point. And this is approximately true. But the theo- 
retical result, it will be remembered, was only obtained by as- 
suming the presence in certain proportions of component vibrations 
having nodes at x^, though in fact their absence is required by 
mechanical laws. The presence or absence of these components is 
a matter of indifference when a node is the point of observation, 
but not in any other case. When the node is departed from, the 
vibration curve shews a series of ripples, due to the absence of 
the components in question. Some further Retails will be found 
in Helmholtz and Donkin. 

The sustaining power of the bow depends upon the fact that 
solid friction is less at moderate than at small velocities, so that 
when the part of the string acted upon is moving with the bow 
(not improbably at the same velocity), the mutual action is greater 
than when the string is moving in the opposite direction with 
a greater relative velocity. The accelerating effect in the first 
part of the motion is thus not entirely neutralised by the sub- 
sequent retardation, and an outstanding acceleration remains 
capable of maintaining the vibration in spite of other losses of 
energy. A curious effect of the same peculiarity of solid friction 
has been observed by W. Froude, who found that the vibrations 
of a pendulum swinging from a shaft might be maintained or 
even increased by causing the shaft to rotate. 

[Another case in which the vibrations of a string are main- 
tained is that of the Aeolian Harp. It has often been suggested 
that the action of the wind is analogous to that of a bow ; but the 
analogy is disproved by the observation^ that the vibrations are 
executed in a plane iransfoerse to the direction of the wind. The 
true explanation involves hydrodynamical theory not yet de- 

1 VHL Mag., March, 1879, p. 161. 

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139. A string stretched on a smooth curved surface will in 
equilibrium lie along a geodesic line, and, subject to certain con- 
ditions of stability, will vibrate about this configuration, if dis- 
placed. The simplest case that can be proposed is when the 
surface is a cylinder of any form, and the equilibrium position 
of the string is perpendicular to the generating lines. The student 
will easily prove that the motion is independent of the curvature 
of the cylinder, and that the vibrations are in all essential respects 
the same as if the surface were developed into a plane. The case 
of an endless string, forming a necklace round the cylinder, is 
worthy of notice. 

In order to illustrate the characteristic features of this class of 
problems, we will take the comparatively simple example of a 
string stretched on the surface of a smooth sphere, and lying, 
when in equilibrium, along a great circle. The co-ordinates to 
which it will be most convenient to refer the system are the 
latitude measured from the great circle as equator, and the 
longitude ^ measured along it. If the radius of the sphere be a, 
we have 

T^\\p{adYad4> = '^ld'di> (1). 

The extension of the string is denoted by 

su that 


d** = (odd)* + (o cos tf d^y ; 



^ 1 \(^^W ./il* 1 l{d0\* 0* . ., 

If the ends be fixed, 

1 Cambridge Mathematical Tripos Examination, 1876. 

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and the equation of virtual velocities is 

aV f'eSed4>-aT,fB0(j^^'\-e)d(l>=^O, 
whence, since Bd is arbitrary, 

•«'''^=^>(|^.+^) (^> 

This is the equation of motion. 
If we assume x cosjp^, we get 

^+«-fv«-» <*). 

of which the solution, subject to the condition that vani^faes 
with <l>, is 

tf = 4 8in|^^p»-f llV.cos;)^ (5). 

The remaining condition to be satisfied is that vanishes when 
o^ = Z, or ^ = a, if a = l/a. 

This gives 

where m is an integer. 

The normal functions are thus of the same form as for a 
straight string, viz. 

tf = i4 sm — - co&pt (/), 

but the series of periods is diflferent. The effect of the curvature 
is to make each tone graver than the corresponding tone of a 
straight string. If a > w, one at least of the values of jp' is nega- 
tive, indicating that the corresponding modes are unstable. If 
« = "W", jpi is zero, the string being of the same length in the dis- 
placed position, as when ^ = 0. 

A similar method might be applied to calculate the motion of 
a string stretched round the equator of any surface of revolu- 

140. The approximate solution of the problem for a vibrating 
string of nearly but not quite uniform longitudinal density has been 
fully considered in Chapter I v. § 91, as a convenient example of 

> [For a more general treatment of this question see MioheU, Menenger of 
Mathematics t vol. xiz. p. 87, 1890.] 

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the general theory of approximately simple systems. It will be 
sufficient here to repeat the result. If the density be p© + Sp» the 
period t^ of the r^ component vibration is given by 

If the irregularity take the form of a small load of mass m 
at the point a; = 6, the formula may be written 

"-ti>-ft-°-t! <^^ 

These values of r* are correct as far as the first power of the 
small quantities hp and m, and give the means of calculating a 
correction for such slight departures from uniformity as must 
always occur in practice. 

As might be expected, the effect of a small load vanishes at 
nodes, and rises to a maximum at the points midway between 
consecutive nodea When it is desired merely to make a rough 
estimate of the effective density of a nearly uniform string, the 
formula indicates that attention is to be given to the neighbour- 
hood of loops rather than to that of nodes. 

[The effect of a small variation of density upon the period is 
the same whether it occur at a distance x from one end of the 
string, or at an equal distance from the other end. The mea^} 
variation at points equidistant from the centre is all that we need 
regard, and thus no generality will be lost if we suppose that the 
density remains symmetrically distributed with respect to the centre. 
Thus we may write 

T.» = ^^l + a,) (3) 

where oir = jj — (l — cos— , \dx (4). 

In this equation Sp may be expanded from to ^l in the series 

-^ = ^0 + ^1 cos — ,- + ... -f -4rC0S— ^— -f (o), 

Po ^ fr 


A.-'jf'^d. (6), 

. 4 r*' So 2Trrx , ,^^ 

Ar = j -^cos — j-dx (7). 

IJo po I 

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Or^Ao-iAr (8), 

This equation, as it stands, gives the changes in period in 
terms of the changes of density supposed to be known. And 
it shews conversely that a variation of density may alwa3r8 be 
found which will give prescribed arbitrary displacements to all 
the periods. This is a point of some intei'est. 

In order to secure a reasonable continuity in the density, it is 
necessary to suppose that cti, a, . . . are so prescribed that Or assumes 
ultimately a constant value when r is increased indefinitely. If 
this condition be satisfied, we may take ilo ^ ««> a«nd then Ar tends 
to zero as r increases. 

As a simple example, suppose that it be required so to vary 
the density of a string that, while the pitch of the fundamental 
tone is displaced, all other tones shall remain unaltered. The 
conditions give 


and -4i = — 2ai. 

Thus by (6) 

Sp/pQ = — 2ai cos (iirx/l),] 

141. The differential equation determining the motion of a 
string, whose longitudinal density p is variable, is 

^ dt^-^'d^ ^^>' 

from which, if we assume y x cosjp^, we obtain to determine the 
normal ftinctions 

%^^f^ = ^ (2)> 

where i^ is written for jpY^i. This equation is of the second 
order and linear, but has not hitherto been solved in finite terma 
Considered as defining the curve assumed by the string in the 
normal mode under consideration, it determines the curvature at 
any point, and accordingly embodies a rule by which the curve 
can be constructed graphically. Thus in the application to a 
stiing fixed at both ends, if we start fix)m either end at an arbitrary 

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inclination, and with zero curvature, we are always directed by the 
equation with what curvature to proceed, and in this way we 
may trace out the entire curve. 

If the assumed value of i/* be right, the curve will cross 
the axis of x at the required distance, and the law of vibration 
will be completely determined. If i/* be not known, different 
values may be tried until the curve ends rightly; a sufficient 
approximation to the value of v^ may usually be arrived at by a 
calculation founded on an assumed type (^ 88, 90). 

Whether the longitudinal density be uniform or not, the 
periodic time of any simple vibration varies costeris paribus as the 
square root of the density and inversely as the square root of the 
tension under which the motion takes place. 

The converse problem of determining the density, when the 
period and the type of vibration are given, is always soluble. For 
this purpose it is only necessary to substitute the given value of y, 
and of its second differential coefficient in equation (2). Unless 
the density be infinite, the extremities of a string are points of 
zero curvature. 

When a given string is shortened, every component tone is 
raised in pitch. For the new state of things may be regarded as 
derived fi:x)m the old by introduction, at the proposed point of 
fixture, of a spring (without inertia), whose stiffiiess is gradually 
increased without limit. At each step of the process the potential 
energy of a given deformation is augmented, and therefore (§ 88) 
the pitch of every tone is raised. In like manner an addition to 
the length of a string depresses the pitch, even though the added 
part be destitute of inertia. 

142. Although a general integration of equation (2) of § 141 
is beyond our powers, we may apply to the problem some of the 
many interesting properties of the solution of the linear equation 
of the second order, which have been demonstrated by MM. Sturm 
and Liouville^ It is impossible in this work to give anjrthing 
like a complete account of their investigations ; but a sketch, in 
which the leading features are included, may be found interesting, 
and will throw light on some points connected with the general 

^ The memoirs referred to in the text are contained in the first volame of 
liioaville's Journal (1836). 

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theory of the vibrations of continuous bodies. I have not thought 
it necessary to adhere very closely to the methods adopted in the 
original memoirs. 

At no point of the curve satisfjdng the equation 

S + '^''2/ = o (1). 

can both y and dyjdx vanish together. By successive differen- 
tiations of (1) it is easy to prove that, if y and dyjdx vanish 
simultaneously, all the higher differential coeflScients dh/lda?y 
d^y/dafy &c. must also vanish at the same point, and therefore 
by Taylor's theorem the curve must coincide with the axis of x. 

Whatever value be ascribed to i^, the curve satisfying (1) is 
sinuous, being concave throughout towards the axis of x, since 
p is everywhere positive. If at the origin y vanish, and dy/dx 
be positive, the ordinate will remain positive for all values of x 
below a certain limit dependent on the value ascribed to v*. 
If i;* be very small, the curvature is slight, and the curve will 
remain on the positive side of the axis for a great distance. We 
have now to prove that as i/* increases, all the values of x which 
satisfy the equation y = gradually diminish in magnituda 

Let y' be the ordinate of a second curve satisfying the equa- 

% + ^'W-O ...(2). 

as well as the condition that y' vanishes at the origin, and let us 
suppose that i/'* is somewhat greater than i/*. Multipljring (2) by 
y, and (1) by y\ subtracting, and integrating with respect to x 
between the limits and x, we obtain, since y and y' both vanish 
with X, 

y'f.-y%=<''"-''^l?yy''^ <^>- 

If we further suppose that x corresponds to a point at which 
y vanishes, and that the difference between p'^ and i^ is very small, 
we get ultimately 

y't-^^'iy^'^ w- 

The right-hand member of (4) being essentially positive, we 
learn that y and dy/dx are of the same sign, and therefore that, 

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142.] Sturm's theorem. 219 

whether dyjdx be positive or negative, y' is already of the same 
sign as that to which y is changing, or in other words, the value 
of X for which y vanishes is less than that for which y vanishes. 

If we fix our attention on the portion of the curve lying 
between d? = and a?=Z, the ordinate continues positive through- 
out as the value of i^ increases, until a certain value is attained, 
which we will call v^. The function y is now identical in form 
with the first normal function t^ of a string of density p fixed 
at and I, and has no root except at those points. As i^ again 
increases, the first root moves inwards from x=^l until, when a 
second special value v^ is attained, the curve again crosses the 
axis at the point a; = Z, and then represents the second normal 
function u^. This function has thus one internal root, and one 
only. In like manner corresponding to a higher value v^ we 
obtain the third normal function u^ ^with two internal roots, and 
so on. The n^^ function u^ has thus exactly n— 1 internal roots, and 
since its first differential coefficient never vanishes simultaneously 
with the frmction, it changes sign each time a root is passed. 

From equation (3) it appears that if Ur and u, be two diflferent 
normal functions, 

pUrUgdx=0 (.5). 


A beautiful theorem has been discovered by Sturm relating 
to the number of the roots of a function derived by addition 
from a finite number of normal functions. If Um be the component 
of lowest order, and v^ the component of highest order, the function 

f{x)=^<f)mUm + <f>m+ill-m+i't -\r <l>nUn (6), 

where <f>m, (f>m+i, &c. are arbitrary coefficients, has at least m — 1 
internal roots, and at most n — l internal roots. The extremities 
B,t x=^0 and a,t x = l correspond of course to roots in all cases. 
The following demonstration bears some resemblance to that given 
by Liouville, but is considerably simpler, and, I believe, not less 

If we suppose that f{x) has exactly /a internal roots (any 
number of which may be equal), the derived function f (x) cannot 
have less than /a + 1 internal roots, since there must be at least 
one root of/* (x) between each pair of consecutive roots o{f(x), and 
the whole number of roots of /(a?) concerned is /i.+ 2. In like 
manner, we see that there must be at least /a roots of f" (x), 

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i I 


besides the extremities, which themselves necessarily correspond 
to roots; so that in passing from /(a?) to f (x) it is impossible 
that any roots can be lost. Now 

= - P {Vm^ 4>m Um + V^m+i 4>m+i t^tn+i + + I'n' ^n ^n)- • (7), 

as we see by (1); and therefore, since p is always positive, we 
infer that 

has at least fj, roots. 

Again, since (8) is an expression of the same form as f(x), 
similar reasoning proves that 

has at least /a internal roots ; and the process may be continued 
to any extent. In this way we obtain a series of functions, all 
with fi internal roots at least, which diflfer from the original 
function /(a?) by the continually increasing relative importance of 
the components of the higher orders. When the process has been 
carried sufficiently far, we shall arrive at a function, whose form 
differs as little as we please from that of the normal frinction of 
highest order, viz. u^, and which has therefore n — 1 internal roots. 
It follows that, since no roots can be lost in passing down the 
series of functions, the number of internal roots of /(a?) cannot 
exceed n — 1. 

The other half of the theorem is proved in a similar manner 
by continuing the series of functions backwards fit)m /(a?). In 
this way we obtain 

^t4,„+ <f>m+iUm+i-\r + ^»^ 

Vnr^<l>mUm-\rV'^fn+i<l>m+iUn^i-\- +I'n"'<^nWn 

arriving at last at a function sensibly coincident in form with the 
normal function of lowest order, viz. iim, and having therefore 
m — 1 internal roots. Since no roots can be lost in passing up the 
series from this function to f{x), it follows that f(x) cannot have 
fewer internal roots than m — 1 ; but it must be understood that 
any number of the m — 1 roots may be equal. 

We will now prove that f(x) cannot be identically zero, unless 

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all the coefficients ^ vanish. Suppose that <f>r is not zero. 
Multiply (6) by pUr, and integrate with respect to x between the 
limits and L Then by (5) 

I purf{x)dx^il>r\ pur^dx (9); 

Jo Jo 

from which, since the integral on the right-hand side is finite, we 
see thsLt/{x) cannot vanish for all values of x included within the 
range of integration. 

Liouville has made use of Sturm's theorem to shew how a 
series of normal functions may be compounded so as to have an 
arbitrary sign at all points lying between a? = and x=:l. His 
method is somewhat as follows. 

The values of x for which the ftinction is to change sign being 
a, 6, c, ..., quantities which without loss of generality we may 
suppose to be all diflferent, let us consider the series of determi- 

Wi(a), tii{x) 

1*1 (a), Wi(6), Ui(x) I 
t*8(a), Wa(6), tk(x) I 
u^(a)y M,(6), u^(x) l,&c. 

The first is a linear function of v^ (x) and ti, (x), and by Sturm's 
theorem has therefore one internal root at most, which root is 
evidently a. Moreover the determinant is not identically zero, 
since the coefficient of v^ (x), viz. t*i (a), does not vanish, whatever 
be the value of a. We have thus obtained a function, which 
changes sign at an arbitrary point a, and there only internally. 

The second determinant vanishes when x = a, and when x = b, 
and, since it cannot have more than two internal roots, it changes 
sign, when x passes through these values, and there only. The 
coefficient of w,(ic) is the value assumed by the first determinant 
when x = b, and is therefore finite. Hence the second determinant 
is not identically zero. 

Similarly the third determinant in the series vanishes and 
changes sign when a? = a, when a? = 6, and when a? = c, and at these 
internal points only. The coefficient of U4(x) is finite, being the 
value of the second determinant when x = c. 

It is evident that by continuing this process we can form 
functions compounded of the normal functions, which shall vanish 
and change sign for any arbitrary values of x, and not elsewhere 

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internally ; or, in other words, we can form a function whose sign 
is arbitrary over the whole range from x = to x = L 

On this theorem liouville founds his demonstration of the 
possibility of representing an arbitrary function between a; = and 
a? = i by a series of normal functions. If we assume the possibility 
of the expansion and take 

/(^) = </>i^(^) + <^*t^,(a?) + <^,w,(a?) + (10), 

the necessary values of <f>i, (fh, &c. are determined by (9), and we 

/{x) = ^\vr{x)j pUr(x)f{x)dx^j pUr"" (x) cLcY (11). 

If the series on the right be denoted by F(x\ it remains to 
establish the identity of /(a?) and F(xy 

If the right-hand member of (11) be multiplied by pUr(x) and 
integrated with respect to x from a? = to a? = Z, we see that 

I p tlr (x) F{x)dx—\ pUr {x)f{x) dx, 

Jo Jo 

or, as we may also write it, 

^ {F(x)-f(x)}pur(x)dx==0 (12), 


where iv(a?) is any normal function. From (12) it follows that 


{F(x) -f(x)] [A,u, (x) + A^u^ (x) + i4,w,(a?)+ •. .} pdx^O.. .(13), 

where the coeflBcients Ai, A^^ &c. are arbitrary. 

Now if F{x) -f(x) be not identically zero, it will be possible 
so to choose the constants Aj, -4j, &c. that A^Ui (x) + A^v^(x)-{' ... 
has throughout the same sign as F (x) —f(x)y in which case every 
element of the integi-al would be positive, and equation (13) could 
not be true. It follows that F(x)—f(x) cannot differ from zero, 
or that the series of normal functions forming the right-hand 
member of (11) is identical with /(a?) for all values of a? from x = 
to a? = i. 

The arguments and results of this section are of course ap- 
plicable to the particular case of a uniform string for which the 
normal functions are circular. 

[As a particular case of variable density the supposition that 

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p = ax^ is worthy of notice, § 148 6. In the notation there 

m«+i = n«=pVyi (14), 

and the general solution is 

y = .4ic*+*"*+-Bi»*-»*"* (15). 

If the string be fixed at two points, whose abscissae x^, x^ are 
as r to 1, the frequency equation is r^^ = 1, or 

"'^i + ofgC). « 

where s denotes an integer. The proper frequencies thus depend 
only upon the ratio of the terminal abscissae. By supposing r 
nearly equal to unity we may fall back upon the usual formula 
(§ 124) applicable to a uniform string. 

The general form of the normal function is 

142 a. The points where the string remains at rest, or nodes, 
are of course determined by the root.s of the normal functions, 
when the vibrations are free. In this case the frequency is limited 
to certain definite values ; but when the vibrations are forced, they 
may be of any frequency, and it becomes possible to trace the 
motion of the nodal points as the frequency increases continuously. 

For example, suppose that the imposed force acts at a single 
point P of a string AB, whose density may be variable. So long 
as the frequency is less than that of either of the two parts AP, 
PB (supposed to be held at rest at both extremities) into which 
the string is divided, there can be no (interior) node (Q). Other- 
wise, that part of the string AQ between the node Q and one 
extremity {A\ which does not include P, would be vibrating 
freely, and more slowly than is possible for the longer length AP, 
included between the point P and the same extremity. When the 
frequency is raised, so as to coincide with the smaller of those 
proper to AP, PB, say -4P, a node enters at P and then advances 
towards A. At each coincidence of the frequency with one of 
those proper to the whole string AB, the vibration identifies itself 
with the corresponding free vibration, and at each coincidence with 
a frequency proper to AP, or BP, a new node appears at P, and 

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advances in the first case towards A and in the second towards B. 
And throughout the whole sequence of events all the nodes move 
outwards from P towards A or B. 

Thus, if the string be uniform and be bisected at P, there is 
no node until the pitch rises to the octave {&) of the note (c) of the 
string. At this stage two nodes enter at P, and move outwards 
sjnmmetrically. When g' is reached, the mode of vibration is that 
of the free vibration of the same pitch, and the nodes are at the 
two points of trisection. At c" these nodes have moved outwards 
so far as to bisect AP^ BP, and two new nodes enter at P. 

143. When the vibrations of a string are not confined to one 
plane, it is usually most convenient to resolve them into two sets 
executed in perpendicular planes, which may be treated inde- 
pendently. There is, however, one case of this description worth 
a passing notice, in which the motion is most easily conceived and 
treated without resolution. 

Suppose that 

. SfTX 287rt 

y = sm -,- cos 

^ I T 

. STTX . 28'7rt 

z = sin — f- sm 

I T 




r = V(y» + ^«) = sin-p (2), 

and z : y = tan (2s7r^/T) (3), 

shewing that the whole string is at any moment in one plane, 
which revolves uniformly, and that each particle describes a circle 
with radius sin {sirxjl). In fact, the whole system turns without 
relative displacement about its position of equilibrium, completing 
each revolution in the time rja. The mechanics of this case is 
quite as simple as when the motion is confined to one plane, the 
resultant of the tensions acting at the extremities of any small 
portion of the string's length being balanced by the centrifugal 

144. The general differential equation for a uniform string, 

iy-^a?^ (V) 

d1? " da? ^^^' 

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may be transformed by a change of variables into 

^1 = <^ (2), 

where w = a? — erf, v = a; + a^. The general solution of (2) is 

y^f{u)^-F{v)^f{x^at) + F{x^'aA) (3)S 

/, F being two arbitrary functions. 

Let us consider first the case in which F vanishes. When 
t has any particular value, the equation 

y^fix-ai) (4). 

expressing the relation between x and y, represents the form of the 
string. A change in the value of ^ is merely equivalent to an 
alteration in the origin of Xy so that (4) indicates that a certain 
form is propagated along the string with uniform velocity a in the 
positive direction. Whatever the value of y may be at the point 
X and at the time t, the same value of y will obtain at the point 
x + a^tB,\, the time ^ + A^. 

The form thus perpetuated may be any whatever, so long as it 
does not violate the restrictions on which (1) depends. 

When the motion consists of the propagation of a wave in the 
positive direction, a certain relation subsists between the inclina- 
tion and the velocity at any point. Differentiating (4) we find 

%-'% » 

Initially, dy/eft and dyjdx may both be given arbitrarily, but if 
the above relation be not satisfied, the motion cannot be repre- 
sented by (4). 

In a similar manner the equation 

y:=^F{x^-at) (6) 

denotes the propagation of a wave m the negative direction, and 
the relation between dyjdt and dyjdx corresponding to (5) is 

l-«S ('^ 

In the general case the motion consists of the simultaneous 
propagation of two waves with velocity a, the one in the positive, 

1 [Equations (1) and (3) are due to D'Alembert (1750).] 
R. 15 

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and the other in the negative direction; and these waves are 
entirely independent of one another. In the first dyjdt = — a dyjdx, 
and in the second dy/dt = a dy/dx. The initial values of dy/dt 
and dy/dx must be conceived to be divided into two parts, which 
satisfy respectively the relations (5) and (7). The first constitutes 
the wave which will advance in the positive direction without 
change of form ; the second, the negative wave. Thus, initially. 




equations which determine the functions /' and F' for all values 
of the argument from a? = — xtoa?=x,if the initial values of 
dy/da smd dy/dt be known. 

If the disturbance be originally confined to a finite portion of 
the string, the positive and negative waves separate after the 
interval of time required for each to traverse half the disturbed 

Fig. 28. 

Suppose, for example, that AB ia the part initially disturbed. 
A point P on the positive side remains at rest until the positive 
wave has travelled from A to P, is disturbed during the passage 
of the wave, and ever afber remains at rest. The negative wave 
never affects P at all. Similar statements apply, mutatis mutandis, 
to a point Q on the negative side of AB. If the character of the 
original disturbance be such that a dyjdx — dyjdt vanishes initially, 
there is no positive wave, and the point P is never disturbed at 
all ; and if a dyjdx + dyjdt vanish initially, there is no negative 
wave. If dyjdt vanish initially, the positive and the negative 
waves are similar and equal, and then neither can vanish. In 
cases where either wave vanishes, its evanescence may be con- 
sidered to be due to the mutual destruction of two component 

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waves, one depending on the initial displacements, and the other 
on the initial velocities. On the one side these two waves con- 
spire, and on the other they destroy one another. This explains 
the apparent paradox, that P can fail to be affected sooner or later 
after AB has been disturbed. 

The sabsequent motion of a string that is initially displaced 
mthout velocity, may be readily traced by graphical methods. 
Since the positive 8md the negative waves are equal, it is only 
necessary to divide the original disturbance into two equal parts, 
to displace these, one to the right, 8md the' other to the left, 
through a space equal to at, and then to recompound them. We 
shall presently apply this method to the case of a plucked string 
of finite length. 

146. Vibrations are called stationary, when the motion of each 
particle of the system is proportional to some function of the time, 
the same for all the particles. If we endeavour to satisfy 

dt-"'' da^ • ^^^' 

by assuming y = XT, where X denotes a function of x only, and 
T a function of t only, we find 

TdWy^Xd^"^"^ (a constant), 
fio that 

7= -4 cos mat + 5 sin rnat h .^. 

X = cosmx +Dsmnix J ^ ** 

proving that the vibrations must be simple harmonic, though of 
arbitrary period. The value of y may be written 

y = P cos (mat — e) cos {mx — a) 
= i P cos (mat + 7M« — € — a) -h J P cos (wo^ — ma — € + a).,.(3), 

shewing that the most general kind of stationary vibration may 
be regarded as due to the superposition of equal progressive vibra- 
tions, whose directions of propagation are opposed. Conversely, 
two stationary vibrations may combine into a progressive one. 

The solution y^f{x — at)'^F{x + at) applies in the first 
instance to an infinite string, but may be interpreted so as to 
give the solution of the problem . for a finite string in certain 


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casea Let us suppose, for example, that the string terminates 
at x==0, and is held fast there, while it extends to infinity in 
the positive direction only. Now so long as the point ^ =: 
actually remains at rest, it is a matter of indiflference whether 
the string be prolonged on the negative side or not. We are 
thus led to regard the given string as forming part of one doubly 
infinite, and to seek whether and how the initial displacements 
and velocities on the negative side can be taken, so that on 
the whole there shall be no displacement at a; =: throughout the 
subsequent motion. The initial values of y and y on the positive 
side determine the corresponding parts of the positive and negative 
waves, into which we know that the whole motion can be resolved. 
The former has no influence at the point x — 0. On the negative 
side the positive and the negative waves are initially at our dis- 
posal, but with the latter we are not concerned. The problem is 
to determine the positive wave on the negative side, so that in 
conjunction with the given negative wave on the positive side 
of the origin, it shall leave that point undisturbed. 

Let OPQRS... be the line (of any form) representing the 
wave in OX, which advances in the negative direction. It is 

Fig. 24. 

evident that the requirements of the case are met by taking on 
the other side of what may be called the contrary wave, so that 
is the geometrical centre, bisecting every chord (such as PP^ 
which passes through it. Analytically, if y =/(aj) is the equation 

of 0PQR8 , -y=^f(-co) is the equation of OFQ'RS 

When after a time t the curves are shifted to the left and to 
the right respectively through a distance at, the co-ordinates 
corresponding to a; = are necessarily equal and opposite, and 
therefore when compounded give zero resultant displacement 

The effect of the constraint at may therefore be represented 

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by supposing that the negative wave moves through undisturbed, 
but that a positive wave at the same time emerges from 0. This 
reflected wave may at any time be found from its parent by the 
following rule : 

Let APQRS... be the position of the parent wave. Then the 
reflected wave is the position which this would assume, if it were 

Fig. 26. 

turned through two right angles, first about OX as an axis of 
rotation, and then through the same angle about OT. In other 
words, the return wave is the image of APQRS formed by 
successive optical reflection in OX and OY, regarded as plane 

The same result may also be obtained by a more analytical 
process. Id the general solution 

the functions /(^), F(z) are determined by the initial circumstances 
for all positive values of z. The condition at a? = inquires that 

f(-at) + F(at)^0 

for all positive values of t, or 

/(-z) = -Fiz) 

for positive values of z. The functions / and F are thus de- 
termined for all positive values of x and t 

There is now no difficulty in tracing the course of events when 
iuH) points of the string A and B are held fast. The initial dis- 
turbance in AB divides itself into positive and negative waves, 
which are reflected backwards and forwards between the fixed 
points, changing their character from positive to negative, and 
vice versd, at each reflection. After an even number of reflec- 
tions in each case the original form and motion is completely 

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recovered. The process is most easily followed in imagination 
when the initial disturbance is confined to a small part of the 
string, more particularly when its character is such as to give rise 
to a wave propagated in one direction only. The pulse travels with 
uniform velocity (a) to and fro along the length of the string, and 
after it has returned a second time to its starting point the 
original condition of things is exactly restored. The period of 
the motion is thus the time required for the pulse to traverse 
the length of the string twice, or 

T = 2l/a (1). 

The same law evidently holds good whatever may be the character 
of the original disturbance, only in the general case it may 
happen that the shortest period of recurrence is some aliquot part 
of T. 

146. The method of the last few sections may be advantage- 
ously applied to the case of a plucked string. Since the initial 
velocity vanishes, half of the displacement belongs to the positive 
and half to the negative wave. The manner in which the wave 
must be completed so as to produce the same effect as the con- 
straint, is shewn in the figure, where the upper curve represents 

Fig. 26. 

the positive, and the lower the negative wave in their initial 
positions. In order to find the configuration of the string at any 
future time, the two curves must be superposed, after the upper 
has been shifted to the right and the lower to the left through a 
space equal to at. 

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146. J 



The resultant curve, like its components, is made up of straight 
pieces. A succession of six at intervals of a twelfth of the period, 

Kg. 27. 

shewing the course of the vibration, is given in the figure (Fig. 27), 
taken from Helmholtz. From the string goes back again to A 
through the same stages \ 

It will be observed that the inclination of the string at the 
points of support alternates between two constant values. 

147. If a small disturbance be made at the time t at the 
point X of an infinite stretched string, the effect will not be felt 
at until after the lapse of the time xja, and will be in all 
respects the same as if a like disturbance had been made at 
the point a; + A^ at time t — ^w/a. Suppose that similar dis- 
turbances are communicated to the string at intervals of time 
T at points whose distcmces from increase each time by a Br, 
then it is evident that the result at will be the same as if the 
disturbances were all made at the same point, provided that the 
time-intervals be increaised from t to t + St. This remark con- 

1 This method of treating the vibration of a plucked string is due to Toung. 
Phil. Trant., 1800. The student is recommended to make himself &miliar with it 
by actually constructing the forms of Fig. 27. 

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tains the theory of the alteration of pitch due to motion of the 
source of disturbance ; a subject which will come under our notice 
again in connection with aerial vibrations. 

1498. When one point of an infinite string is subject to a forced 
vibration, trains of waves proceed from it in both directions ac- 
cording to laws, which are readily investigated. We shall suppose 
that the origin is the point of excitation, the string being there 
subject to the forced motion y^A^\ and it will be sufficient to 
consider the positive side. If the motion of each element (b be 
resisted by the frictional force Kpyda, the differential equation is 

d&^^dt''' da? ••••^^^' 

or since y oc c^, 

%-&-^y-^'y •<«)• 

if for brevity we write V for the coefficient of y. 

The general solution is 

y={C«r*» + D6+*»}6<'^ (3). 

Now since y is supposed to vanish at an infinite distance, D 
must vanish, if the real part of X be taken positive. Let 

where a is positive. 

Then the solution is 

y=^6-<»+*>*+<^ (4), 

or, on throwing away the imaginary part, 

y^Aer^ co&(pt-/3w) (5), 

corresponding to the forced motion at the origin 

y = -4 coapt (6). 

An arbitrary constant may, of course, be added to t 

To determine a and )3, we have 

«.-/3. — g; 2«/3 = f (7X 

If we suppose that k is small, 

j3=p/a, a = K/2a nearly, 

and y=:Ae-'^^ cos (pt—^xj (8). 

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Thi8 solution shews that there is propagated along the string 
a wave, whose amplitude slowly diminishes on account of the 
exponential factor. If k^O, this factor disappears, and we have 

y = 4 cos (pt-^) (9). 

This result stands in contradiction to the general law that, 
when there is no friction, the forced vibrations of a system (due 
to a single simple harmonic force) must be synchronous in phase 
throughout. According to (9), on the contrary, the phase varies 
continuously in passing from one point to another along the string. 
The &ct is, that we are not at liberty to suppose /c^O in (8), 
inasmuch as that equation was obtained on the assumption that 
the real part of X. in (3) is positive, and not zero. However long 
a finite string may be, the coe£Scient of friction may be taken so 
small that the vibrations are not damped before reaching the 
further end. After this point of smallness, reflected waves begin 
to complicate the result, and when the friction is diminished 
indefinitely, an infinite series of such must be taken into account, 
and would give a resultant motion of the same phase throughout. 

This problem may be solved for a string whose mass is supposed 
to be concentrated at equidistant points, by the method of § 120. 
The co-ordinate -^i may be supposed to be given {—H^^\ and 
it will be found that the system of equations (5) of § 120 may all 
be satisfied by taking 

^r = «^^^i (10), 

where is a complex constant determined by a quadratic equa- 
tion. The result for a continuous string may be afterwards 

[In the notation of § 120 the quadratic equation is 

5^ + il^ + 5 = (11), 

where ^=-/*p» + =^', B^-^ (12). 

The roots of (11) are 

«.-^±^'(^:=«■) („), 

and are imaginary if 4^ > il^ that is, if 

^<*i <")• 

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a condition always satisfied in passing to the limit where a and /jl 
are infinitely small. In any case when (14) is satisfied the 
modulus of ^ is unity, so that (10) represents wave propagation. 

If, however, (14) be not satisfied, the values of are real In 
this case all the motions are in the same phase, and no wave 
is propagated. The vibration impressed upon y^i ib imitated upon 

a reduced scale by i^j, i^, , with amplitudes which form a 

geometrical progression. In the first case the motion is pro- 
pagated to an infinite distance, but in the second it is practically 
confined to a limited region round the source.] 

148 a. So long as the conditions of § 144 are satisfied, a 
positive, or a negative, wave is propagated undisturbed. If 
however there be any want of uniformity, such (for example) as 
that caused by a load attached at a particular point, reflection 
will ensue when that point is reached. The most interesting 
problem under this head is that of two strings of different 
longitudinal densities, attached to one another, and vibrating 
transversely under the common tension Tj. Or, if we regard the 
string as single, the density may be supposed to vary dis- 
continuously from one uniform value (pi) to another (pj). If 
Oi, Os denote the corresponding velocities of propagation, 

a,«=rV/>i, a,' = r,//>, (1), 

and M = ai/aa = VW/)i) (2). 

The conditions to be satisfied at the junction of the two parts 
are (i) the continuity of the displacement y, and (ii) the continuity 
of dy/da. If the two parts met at a finite angle, an infinitely 
small element at the junction would be subject to a finite force. 

Let us suppose that a positive wave of harmonic type, travelling 
in the first part (pj), impinges upon the second (/)j). In the latter 
the motion will be adequately represented by a positive wave, 
but in the former 'We must provide for a negative reflected wave. 
Thus we may take for the two parts respectively 

y = fi6*» <•»*-«» -fiTe*** <*»*+*> (3), 

y=Z;6**«w-«) (4), 

where ki = 27r/Xi , k^ = 2'7r/X5 , 

so that kjOa — k^ (5). 

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The conditions at the junction {x = 0) give 

H+K^L (6), 

hH-hK^kJL '. (7); 

whence 5-^^^' = -^ W- 

Since the ratio KjH is real, we may suppose that both 
quantities are real; and if we throw away the imaginary parts 
from (3) and (4) we get as the solution in terms of real quantities 

y = J?cosA:i(ai^-a?)+ircosii(ai^ + a?) (9); 

y«(fl' + Z)cosA?,(a,«-a?) (10). 

The ratio of amplitudes of the reflected and the incident 
waves expressed by (8) is that first obtained by T. Young for 
the corresponding problem in Optics. 

148 6. The expression for the intensity of reflection established 
in § 148 a depends upon the assumption that the transition from 
the one density to the other is sudden, that is occupies a distance 
which is small in comparison with a wave length. If the 
transition be gradual, the reflection may be expected to tsX\ off, 
and in the limit to disappear altogether. 

The problem of gradual transition includes, of course, that of 
a variable medium, and would in general be encumbered with 
great difficulties. There is, however, one case for which the 
solution may be readily expressed, and this it is proposed to 
consider in the present section. The longitudinal density is 
supposed to vary as the inverse square of the abscissa. If y, 
denoting the transverse displacement be proportional to e**, the 
equation which it must satisfy as a function of a?, is (§ 141), 

g + n'a;-^ = (1), 

where v? is some positive constant, of the nature of an abstract 

The solution of (1) is y = ila^+^n ^. ^^im (2), 

where m^^v?'-^ (3). 

If m be real, that is, if w > \, we may obtain, by supposing 
A ss 0» as a final solution in real quantities, 

y as (7^ cos (p< — wloga-fe) (4), 

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which represents a positive progressive wave, in many respects 
similar to those propagated in uniform media. 

Let us now suppose that, to the left of the point x = Xi, the 
variable medium is replaced by one of uniform constitution, suck 
that there is no discontinuity of density at the point of transition ; 
and let us inquire what reflection a positive progressive wave in 
the uniform medium will undergo on arrival at the variable 
medium. It will be sufficient to consider the case where m is 
I'eal, that is, where the change of density is but moderately rapid. 

By supposition, there is no negative wave in the variable 
medium, so that ^ = in (2). Thus 

Jiud, when x — Xi, -y='- (5). 

ydx Xi ^ ^ 

The general solution for the uniform medium, satisfying the 
equation d^jdnf + v?x{'^ = 0, may be written 

y^He *» -{-Ke *» (6), 

from which, when oo^Xi, 

dy in H-K .,.. 

ydx^ x,H + K ^^ 

In equation (6), H represents the amplitude of the incident 
positive wave, and K the amplitude of the reflected negative 
wave. The condition to be satisfied at a; 3=0^ is expressed by 

equating the values of — ^ given by (5) and (7). Thus 

jy"i(n+m)-i ^ ^' 

which gives, in symbolical form, the ratio of the reflected to the 
incident vibration. 

Having regard to (3), we may write (8) in the form 

^- -:ii- (9)- 

so that the amplitude of the reflected wave is ^(n + m)"^ of 
that of the incident. Thus, as was to be expected, when n and m 
are great, %.e., when the density changes slowly in the variable 

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medium, there is but little reflection. As regards phase, the 
result embodied in (9) may be represented by supposing that the 
reflection occurs at ^ = a^, and involves a change of phase amount- 
ing to a quarter period. 

Passing on now to the more important problem, we will 
suppose that the variable medium extends only so far as the point 
x=^x^, beyond which the density retains uniformly its value at 
that point. A positive wave travelling at first in a uniform 
medium of density proportional to Wi"^, passes at the point x = Xi 
into a variable medium of density proportional to ar^, and again, at 
the point x^x^, into a uniform medium of density proportional to 
x^. The velocities of propagation are inversely proportional to 
the square roots of the densities, so that, if /li be the refractive 
index between the extreme media, 

f^'l (lO)- 

The thickness (d) of the layer of transition is 

d-x^ — Xi (11). 

The wave-lengths in the two media are given by 

_ 27rXi _ 27rdg, ^ 

n n 

«othat „ = ___=.^__^ (12). 

For the first medium we take, as before, 

y^He '^ -hiTe *. (6), 

giving, when x^x^, 

dy inH — K in0^ .... 

ydi*"""^2r+ir~ "^ ^ ^' 

if, for brevity, we write 6 for „ r-^ • 

For the variable medium, 

y = ila:*+*"«+5a:*-*'« (2), 

giving, when a? = a?i, 

^y - ^ -1 (i + im)Ax,^ + {\ - im) BxT'- 

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Hence the condition to be satisfied at a? = d^ gives 

whence ^ = ^-^«^^--^^-|^* (14). 

The condition to be satisfied at a? = aj, may be deduced firom (14), 
by substituting x^tor a^, putting at the same time ^ = 1 in virtue 
of the supposition that in the second medium there is no negative 
wave. Hence, equating the two values ot A\B, we get 

^ t^ + tn^ + i""^* im + tn + i ^^^^' 

as the equation from which the reflected wave in the first medium 
is to be found. Having regard to (3), we get 

^ _ ^r-iT ^ m + n + ii + /A»~ (rn - n - ii) 
" H-{-K m + n-ii + /[i»^« (m- n + it) ' 

so that rr=o/ \ . o aim/ \ (16)- 

-ff 2 (m + n) + 2/Lt*** (m — n) ^ 

This is the symbolical solution. To interpret it in real quantities, 
we must distinguish the cases of m real and m imaginary. If the 
transition be not too sudden, m is real, and (16) may be written 

K ^ % — 1 -f cos (2m log ^) + 1 sin (2m log /a) 

fl" *" 2 m + n + (m — n) cos (2m log fi) +i{m — n) sin (2m log ft) " 

Thus the expression for the ratio of the intensities of the reflected 
and the incident waves is, after reduction. 



in'(mlog /i) .^y. 

+ sin' (m log /*) ^ 

If m be imaginary, we may write im = m'] (16) then gives for 
the ratio of intensities, 

or, if we introduce the notation of hyperbolic trigonometry § 170, 

sinh' (m' log fi) 

sinh' (mf log/x) + 4m'' 
For the'critical value m = 0, we get, from (17) or (19), 


4 + (log^)' ^^"^- 

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These expressions allow us to trace the effect of a more or 
less gradual transition between media of given indices. If the 
transition be absolutely abrupt, n = 0, by (12); so that rn!=^\. 
In this case, (18) gives us (§ 148 a) Young's well-known formula 

U + lJ 


Since increases continually from a: = 0, the ratio (19) 


increases continually bom. m=0 to m's=J, i.e,, diminishes 
continually from the case of sudden transition m' = ^, when its 
value is (21), to the critical case m = 0, when its value is (20), 
after which this form no longer holds good. When m' = 0, w = J, 
and, by (12), d = (X, - \)l Anr. 

When n>\, (17) is the appropriate form. We see from it 
that with increasing n the reflection diminishes, until it vanishes, 
when mlog/A = 7r, %,e. when 

"■=i^<i^y •• • « 

With a still more gradual transition the reflection revives, reaches 
a maximum, again vanishes when m log /bb «= 27r, and so on^ 

148 a In the problem of connected strings, vibrating under 
the influence of tension alone, the velocity in each uniform part is 
independent of wave length, and there is nothing corresponding to 
optical dispersion. This state of things will be departed from if 
we introduce the consideration of stiffness, and it may be of interest 
to examine in a simple case how far the problem of reflection is 
thereby modified. As in § 148 a, we will suppose that at a? = () 
the density changes discontinuously from pi to pa, but that now 
the vibrations of the second part occur under the influence of 
sensible stiffness. The differential equation applicable in this 
case is, § 188, 

or, if y vary as e*»*, 

-'^S+«'*S+"*y=<^ <!>' 

so that, if y vary as e***, 

y8»fe* + a,«A:»-n* = (2). 

^ Proe, Math. Soc., vol. zi. February, 1S80 ; where will also be found a numeri- 
cal example illustrative of optical conditions. 

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In consequence of the stiffiiess represented by ^ the velocity 
of propagation deviates from a^y and must be found from (2). The 
two values of Ar* given by this equation are real, one being positive 
and the other negative. The four admissible values of k may thus 
be written + k^, ± iK* so that the complete solution of (1) will be 

y = -4e*^ + jBe-*««+(7e-*«* + i)6*^ (3), 

Aa, k^ being real and positive. The Velocity of propagation is njk^ 

In the application which we have to make the disturbance of 
the imperfectly flexible second part is due to a positive wave 
entering it from the first part. When x is great and positive, (3) 
must reduce to its second term. Thus 

^=0, i) = 0; 

and we are left with 

y = Ber*^ + Ce-^ (4). 

This holds when x is positive. When x is negative, corresponding 
to the perfectly flexible first part, we have 

y = ire-^t«+ire«t* (5), 

in which ki-n/oi (6). 

The " refi^iCtive index " is given by 

fi^kjk, (7). 

The conditions at the junction are first the continuity of y and 
dyldx. Further, d^y/dx^ in (4) must vanish at this place, inasmuch 
as curvature implies a couple (§ 162), and this could not be 
transmitted by the first part. Hence 

H + K=B-hC (8), 

k,{H'-K) = k^^ih,C (9), 

-A8»5 + VC=0 (10). 

From these we deduce 


H-K' kji, ^^^^' 

K_h^ (k^ - Aj) + ik^ . . ^ 

H' h {k\ + k,) + ikA ^^^^' 

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and thence for the intensity of reflection, equal to Mod^ (K/H), 

If the second part, as well as the first, be perfectly flexible, 
/8 = 0, Aj = 00 , and we fall back on YouDg's formula In general, 
the intensity of reflection is not accurately given by this formula, 
even though we employ therein the value of the refractive index 
appropriate to the waves actually under propagation. 


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149. The next system to the string in order of simplicity 
is the bar, by which term is usually understood in Acoustics a 
mass of matter of uniform substance and elongated cylindrical 
form. At the ends the cylinder is cut off by planes perpendicular 
to the generating lines. The centres of inertia of the transverse 
sections lie on a straight line which is called the axis. 

The vibrations of a bar are of three kinds — longitudinal, 
torsional, and lateral. Of these the last are the most important, 
but at the same time the most difficult in theory. They are 
considered by themselves in the next chapter, and will only be 
referred to here so far as is necessary for comparison and contrast 
with the other two kinds of vibrations. 

Longitudinal vibrations are those in which the axis remains 
unmoved, while the transverse sections vibrate to and fro in the 
direction perpendicular to their planes. The moving power is 
the resistance offered by the rod to extension or compression. 

One peculiarity of this class of vibrations is at once evident. 
Since the force necessary to produce a given extension in a bar 
is proportional to the area of the section, while the mass to be 
moved is also in the same proportion, it follows that for a bar of 
given length and material the periodic times and the modes of 
vibration are independent of the area and of the form of the 
transverse section. A similar law obtains, as we shall presently 
see, in the case of torsional vibrations. 

It is otherwise when the vibrations are lateral. The periodic 
times are indeed independent of the thickness of the bar in the 
direction perpendicular to the plane of flexure, but the motive power 


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in this case, viz. the resistance to bending, increases more rapidly 
than the thickness in that plane, and therefore an increase in 
thickness is accompanied by a rise of pitch. 

In the case of longitudinal and lateral vibrations, the mechan- 
ical constants concerned are the density of the material and the 
value of Young's modulus. For small extensions (or compressions) 
Hooke's law, according to which the tension varies as the extension, 

- -J J xi. .1 ^ • • actual length — natural length 

holds good. If the extension, viz. ^ ^-^i -r — , 

° natural length 

be called e, we have T=qe, where q is Young's modulus, and T 
is the tension per unit area necessary to produce the extension €. 
Young's modulus may therefore be defined as the force which would 
have to be applied to a bar of unit section, in order to double its 
length, if Hooke's law continued to hold good for so great exten- 
sions ; its dimensions are accordingly those of a force divided by an 

The torsional vibrations depend also on a second elastic con- 
stant fjL, whose interpretation will be considered in the proper 

Although in theory the three classes of vibrations, depending 
respectively on resistance to extension, to torsion, and to flexure 
are quite distinct, and independent of one another so long as the 
squai-es of the strains may be neglected, yet in actual experiments 
with bars which are neither uniform in material nor accurately 
cylindrical in figure it is often found impossible to excite longi- 
tudinal or torsional vibrations without the accompaniment of some 
measure of lateral motion. In bars of ordinaiy dimensions the 
gravest lateral motion is far graver than the gravest longitudinal 
or torsional motion, and consequently it will generally happen that 
the principal tone of either of the latter kinds agrees more or less 
perfectly in pitch with some overtone of the former kind. Under 
such circumstances the regular modes of vibrations become 
unstable, and a small irregularity may produce a great eflfect. The 
difficulty of exciting purely longitudinal vibrations in a bar is 
similar to that of getting a string to vibrate in one plane. 

With this explanation we may proceed to consider the three 
classes of vibrations independently, commencing with longitudinal 
vibrations, which will in fact raise no mathematical questions 
beyond those already disposed of in the previous chapters. 


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160. When a rod is stretched by a force parallel to its length, 
the stretching is in general accompanied by lateral contraction in 
such a manner that the augmentation of volume is less than if 
the displacement of every particle were parallel to the axis. In the 
case of a short rod and of a particle situated near the cylindrical 
boundary, this lateral motion would be comparable in magnitude 
with the longitudinal motion, and could not be overlooked without 
risk of considerable error. But where a rod, whose length is great 
in proportion to the linear dimensions of its section, is subject 
to a stretching of one sign throughout, the longitudinal motion 
accumulates, and thus in the case of ordinary rods vibrating 
longitudinally in the graver modes, the inertia of the lateral 
motion may be neglected. Moreover we shall see later how a 
correction may be introduced, if necessary. 

Let X be the distance of the layer of particles composing any 
section from the equilibrium position of one end, when the rod 
is unstretched, either by permanent tension or as the result of 
vibrations, and let f be the displacement, so that the actual 
position is given by d? + f. The equilibrium and actual position 

of a neighbouring layer being x+ Bx, a? + &c+f+-^&p re- 
spectively, the elongation is d^/dx, and thus, if T be the tension 
per unit area acting across the section, 

T = q 



Consider now the forces acting on the slice bounded by x 

and X + Bx, If the area of the section be o), the tension at a; is 

by (1) qcod^/dx, acting in the negative du-ection, and at ar + Sa? 

the tension is 

(d^ d'i 


acting in the positive direction ; and thus the force on the slice 
due to the action of the adjoining parts is on the whole 




The mass of the element is pa) &r, if p be the original density, 
and therefore if X be the accelerating force acting on it, the 
equation of equilibrium is 

^^fj-o W 

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In what follows we shall not require to consider the operation 
of an impressed force. To find the equation of motion we have 
only to replace X by the reaction against acceleration — ^, and 
thus if g : p = a^ we have 

t^-a^tl (ON 

df " da? ^^>- 

This equation is of the same form as that applicable to the 
transverse displacements of a stretched string, and indicates the 
undisturbed propagation of waves of any type in the positive and 
negative directions. The velocity a is relative to the unstretched 
condition of the bar ; the apparent velocity with which a disturb- 
ance is propagated in space will be greater in the ratio of the 
stretched and unstretched lengths of any portion of the bar. The 
distinction is material only in the case of permanent tension. 

161. For the actual magnitude of the velocity of propagation, 
we have 

a^ = q : p = qa} : pcD, 

which is the ratio of the whole tension necessary (according to 
Hooke's law) to double the length of the bar and the longitudinal 
density. If the same bar were stretched with total tension T, 
and were flexible, the velocity of propagation of waves along it 
would be aJ{T : pay). In order then that the velocity might be 
the same in the two cases, T must be qay, or, in other words, the 
tension would have to be that theoretically necessary in order to 
double the length. The tones of longitudinally vibrating rods 
are thus very high in comparison with those obtainable from 
strings of comparable length. 

In the case of steel the value of q is about 22 x 10* grammes 
weight per square centimetre. To express this in absolute units 
of force on the c. G.s.* system, we must multiply by 980. In 
the same system the density of steel (identical with its specific 
gravity referred to water) is 78. Hence for steel 

a = /y/ 

^^^-^^f^^ = 530,000 

approximately, which shews that the velocity of sound in steel is 
about 530,000 centimetres per second, or about 16 times greater 

^ Centimetre, Gramme, SecoDd. This system is recommended by a Committee 
of the British Association. Brit, Ass. Report, 1873. 

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than the velocity of sound in air. In glass the velocity is about 
the same as in steel. 

It ought to be mentioned that in strictness the value of q deter- 
mined by statical experiments is not that which ought to be used 
here. As in the case of gases, which will be treated in a subsequent 
chapter, the rapid alterations of state concerned in the propaga- 
tion of sound are attended with thermal effects, one result of 
which is to increase the effective value of q beyond that obtained 
from observations on extension conducted at a constant tempera- 
ture. But the data are not precise enough to make ibis correction 
of any consequence in the case of solids. 

162. The solution of the general equation for the longitudinal 
vibrations of an unlimited bar, namely 

f =/(a7 - aO + ^(^ + aO» 

being the same as that applicable to a string, need not be further 
considered here. 

When both ends of a bar are free, there is of course no perma- 
nent tension, and at the ends themselves there is no temporarj' 
tension. The condition for a free end is therefore 




To determine the normal modes of vibration, we must assume 
that f varies as a harmonic function of the time— cos nat. Then 
as a function of ^, ^ must satisfy 


+ n>f = 0. 


of which the complete integral is 

f = J. cosrw7+ Bsmnx (3), 

where A and B are independent of x. 

Now since d^jdx vanishes always when x = 0, we get £ = 0; and 
again since d^jdx vanishes when x = I — the natural length of the 
bar, sin TiZ = 0, which shews that n is of the form 

n = 




i being integral. 

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Accordingly, the normal modes are given by equations of the 


-. J. XTTX iirat ,^v 

f = -4 cos-,- cos— ^ (o), 

in which of course an arbitrary constant may be added to f, if 

The complete solution for a bar with both ends free is there- 
fore expressed by 


f = 2 

.-.^« I 


iirat rt • 
cos — ; — I- Bi sin 



vrhere -4^ and Bi are arbitrary constants, which may be determined 
in the usual manner, when the initial values of f and ^ are 

A zero value of i is admissible ; it gives a term representing a 
displacement f constant with respect both to space and time, 
and amounting in fact only to an alteration of the origin. 

The period of the gravest component in (6) corresponding to 
1 = 1, is 2l/a, which is the time occupied by a disturbance in 
travelling twice the length of the rod. The other tones found 
by ascribing integral values to i form a complete harmonic scale ; 
so that according to this theory the note given by a rod in 
longitudinal vibration would be in all cases musical. 

In the gravest mode the centre of the rod, where x = ^Z, is a 
place of no motion, or node ; but the periodic elongation or com- 
pression d^/dx is there a maximum. 

163. The case of a bar with one end free and the other fixed 
may be deduced from the general solution for a bar with both 
ends free, and of twice the length. For whatever may be the 
initial state of the bar free at a? = and fixed at x = l, such dis- 
placements and velocities may always be ascribed to the sections 
of a bar extending from to 21 and free at both ends as shall 
make the motions of the parts from to i identical in the two 
cases. It is only necessary to suppose that from I to 21 the dis- 
placements and velocities are initially equal and opposite to those 
found in the portion from to Z at an equal distance from the 
centre x=^L Under these circumstances the centre must by 
the symmetry remain at rest throughout the motion, and then the 

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portion from to i satisfies all the required conditions. We con- 
clude that the vibrations of a bar free at one end and fixed at the 
other are identical with those of one half of a bar of twice the 
length of which both ends are free, the latter vibrating only in the 
uneven modes, obtained by making i in succession all odd integers. 
The tones of the bar still belong to a harmonic scale, but the 
even tones (octave, &c. of the fundamental) are wanting. 

The period of the gravest tone is the time occupied by a pulse 
in travelling /owr times the length of the bar. 

164. When both ends of a bar are fixed, the conditions to 
be satisfied at the ends are that the value of f is to be invariable. 
At a? = 0, we may suppose that f = 0. At a; = Z, f is a small 
constant a, which is zero if there be no permanent tension. In- 
dependently of the vibrations we have evidently f = a: a -r Z, and 
we should obtain our result most simply by assuming this term 
at once. But it may be instructive to proceed by the general 

Assuming that as a function of the time f varies as 

A cos nat + B sin nat, 

we see that as a function of x it must satisfy 

of which the general solution is 

^ = (7 cos Tio! •}- D sin nx (1). 

But since | vanishes with x for all values of ^, (7 = 0, and thus 
we may write 

f = 2 sin 7WJ \A cos nat -f B sin nat]. 

The condition at a? = Z now gives 

2 sin TiZ {A cos nat + B sin nat] = a, 
from which it follows that for every finite admissible value of n 

sin nZ = 0, • or n = 
But for the zero value of w, we get 
Aq sin nl = a. 


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and the corresponding term in f is 

^ . . sinrw? x 

f = -do sin 7WJ = a -i — i = a r . 
* sinm ^ 

The complete value of f is accordingly 

f = a y + 2^.1 sm y- V^i cos —v- + 5f sm — p k..(2). 

The series of tones form a complete harmonic scale (from 
which however any of the members may be missing in any 
actual case of vibration), and the period of the gravest com- 
ponent is the time taken by a pulse to travel twice the length 
of the rod, the same therefore as if both ends were free. It 
must be observed that we have here to do with the unstretched 
length of the rod, and that the period for a given natural length 
is independent of the permanent tension. 

The solution of the problem of the doubly fixed bar in the 
case of no permanent tension might also be derived from that 
of a doubly free bar by mere differentiation with respect to x. 
For in the latter problem d^jdx satisfies the necessary differential 
equation, viz. 

dt' \dx) da^ {dx) ' 

inasmuch as { satisfies 

dt''^^ dx^' 

and at both ends d^jdx vanishes. Accordingly dUdx in this 
problem satisfies all the conditions prescribed for f in the case 
when both ends are fixed. The two series of tones are thus 

165. The effect of a small load M attached to any point of 
the rod is readily calculated approximately, as it is sufficient 
to assume the type of vibration to be unaltered (§ 88). We 
will take the case of a rod fixed at a: = 0, and free at x = I, The 
kinetic energy is proportional to 


pay sm^ -^j- dx + J^Jlf sm« -^ , 

p(ol /- 2M . . i7rx\ 

«^*^ 4 (l + po,i«^°'l^J• 


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Since the potential energy is unaltered, we see by the prin- 
ciples of Chapter iv., that the eflfect of the small load 3f at a 
distance x from the fixed end is to increase the period of the 
component tones in the ratio 

The small quantity M : p<d is the ratio of the load to the 
whole mass of the rod. 

If the load be attached at the free end, sinn*Va?/2Z) = l, and 
the effect is to depress the pitch of every tone by the same small 
interval. It will be remembered that i is here an uneven integer. 

If the point of attachment of Jlf be a node of any component, 
the pitch of that component remains unaltered by the addition. 

166. Another problem worth notice occurs when the load at 
the free end is great in comparison with the mass of the rod. 
In this case we may assume as the type of vibration, a condition 
of uniform extension along the length of the rod. 

If f be the displacement of the load M, the kinetic energy is 

r=iJif|'+i|»fV«^Ar = ilniJf+i/>a,o (1). 

The tension corresponding to the displacement f is qca^/l, 
and thus the potential energy of the displacement is 

F^?^ (2) 

The equation of motion is 

and if f X cos pt 

P' = ^^{M + ip<ol) (3). 

The correction due to the inertia of the rod is thus equivalent 
to the addition to M of one-third of the mass of the rod. 

166 a. So long as a rod or a wire is uniform, waves of longi- 
tudinal vibration are propagated along it without change of type, 
but any interruption, or alteration of mechanical properties, will 
in general give rise to reflection. If two uniform wires be joined, 

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the problem of determining the reflection at the junction may be 
conducted as in § 148 a. The conditions to be satisfied at the 
junction are (i) the continuity of f, and (ii) the continuity of 
qcod^/dx, measuring the tension. If pi, ps, <Oi, o),, Oy, Oa denote 
the volume densities, the sections, and the velocities in the two 
wires, the ratio of the reflected to the incident amplitude is 
given by 

H pi (Oiai + piCo^a^ 

The reflection vanishes, or the incident wave is propagated 
through the junction without loss, if 

PiCOitti = p.,a}.,ai (2). 

This result illustrates the difficulty which is met with in obtaining 
effective transmission of sound from air to metal, or from metal to 
air, in the mechanical telephone. Thus the value of pa is about 
100,000 times greater in the case of steel than in the case of air. 

157. Our mathematical discussion of longitudinal vibrations 
may close with an estimate of the error involved in neglecting 
the inertia of the lateral motion of the parts of the rod not 
situated on the axis. If the ratio of lateral contraction to longi- 
tudinal extension be denoted by /a, the lateral displacement of a 
particle distant r from the axis will be /jlvc in the case of equili- 
brium, where e is the extension. Although in strictness this 
relation will be modified by the inertia of the lateral motion, yet 
for the present purpose it may be supposed to hold good, § 88. 

The constant /a is a numerical quantity, lying between and ^. 
If fjL were negative, a longitudinal tension would produce a lateral 
swelling, and if p, were greater than i, the lateral contraction 
would be great enough to overbalance the elongation, and cause 
a diminution of volume on the whole. The latter state of things 
would be inconsistent with stability, and the former can scarcely 
be possible in ordinary solids. At one time it was supposed 
that fi was necessarily equal to ^, so that there was. only one 
independent elastic constant, but experiments have since shewn 
that fi is variable. For glass and brass Wertheim found experi- 
mentally /i = ^. 

If fj denote the lateral displacement of the particle distant r 

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from the axis, and if the section be circular, the kinetic energy 
due to the lateral motion is 

Thus the whole kinetic energy is 

In the case of a bar free at both ends, we have 

iTTX df ITT . iirx 
f X cos ~, , ^ X — r sm -=- , 
* I ax I I 

and thus 

748^:7=1 + ^^^. 

The effect of the inertia of the lateral motion is therefore to 
increase the period in the ratio 

1:1 + 

4 ¥' 

This correction will be nearly insensible for the graver modes of 
bars of ordinary proportions of length to thickness. 

[A more complete solution of the problem of the present 
section has been given by Pochhammer^ who applies the general 
equations for an elastic solid to the case of an infinitely extended 
cylinder of circular section. 'The result for longitudinal vibrations, 
so far as the term in r*/P, is in agreement with that above deter- 
mined. A similar investigation has also been published by Chree^ 
who has also treated the more general question* in which the 
cylindrical section is not restricted to be circular.] 

168. Experiments on longitudinal vibrations may be made 
with rods of deal or of glass. The vibrations are excited by 
friction § 138, with a wet cloth in the case of glass ; but for metal 
or wooden rods it is necessary to use leather charged with powdered 
i-osin. " The longitudinal vibrations of a pianoforte string may be 
excited by gently rubbing it longitudinally with a piece of india 
rubber, and those of a violin string by placing the bow obliquely 
across the string, and moving it along the string longitudinally, 
keeping the same point of the bow upon the string. The note is 
unpleasantly shrill in both cases." 

» Crelle, Bd. 81, 1876. 

» Ihid, Vol. 23, p. 317, 1889. 

a Quart, Math. Joum., Vol. 21, p." 287, 1886. 


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" If the peg of the violin be turned so as to alter the pitch of 
the lateral vibrations very considerably, it will be found that the 
pitch of the longitudinal vibrations has altered very slightly. The 
reason of this is that in the case of the lateral vibrations the 
change of velocity of wave-transmission depends chiefly on the 
change of tension, which is considerable. But in the case of the 
longitudinal vibrations, the change of velocity of wave-transmis- 
sion depends upon the change of extension, which is comparatively 
slight \'* 

In Savart's experiments on longitudinal vibrations, a peculiar 
sound, called by him a "son rauque," was occasionally observed, 
whose pitch was an octave below that of the longitudinal vibra- 
tion. According to Terquem * the cause of this sound is a trans- 
verse vibration, whose appearance is due to an approximate 
agreement between its own period and that of the sub-octave of 
the longitudinal vibration § 68 6. If this view be correct, the 
phenomenon would be one of the second order, probably referable 
to the fact that longitudinal compression of a bar tends to produce 

169. The second class of vibrations, called torsional, which 
depend on the resistance opposed to twisting, is of very small 
importance. A solid or hollow cylindrical rod of circular section 
may be twisted by suitable forces, applied at the ends, in such a 
manner that each transverse section remains in its own plane. 
But if the section be not circulai*, the effect of a twist is of a 
more complicated character, the twist being necessarily attended 
by a warping of the layers of matter originally composing the 
normal sections. Although the effects of the warping might pro- 
bably be determined in any particular case if it were worth 
while, we shall confine ourselves here to the case of a circular 
section, when there is no motion parallel to the axis of the rod. 

The force with which twisting is resisted depends upon an 
elastic constant different from g, called the rigidity. If we de- 
note it by n, the relation between q, n, and fi may be written 


n ?_ 


^ Donkin's Acoustics, p. 154. 
« Atm. de ChinUe, Lvn. 129—190. 

' Thomson and Tait, § 688. This, it shonld be remarked, applies to isotropic 
material only. 

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shewing that n lies between Jg and ^q. In the case of /A = i, 
n = fg. 

Let us now suppose that we have to do with a rod in the form 

of a thin tube of radius r and thickness dr, and let denote the 

angular displacement of any section, distant x from the origin. 

The rate of twist at x is represented by dOjdx, and the shear of the 

material composing the pipe by rddjdx. The opposing force per 

unit of area is nr dOjdx ; and since the area is 27rr dr, the moment 

round the axis is 


^mrr^ dr 


Thus the force of restitution acting on the slice dx has the 


2mn^ dr dx 


Now the moment of inertia of the slice under consideration 
is 2irrdr.dx,p.r^, and therefore the equation of motion assumes 

the form 

d^e d'0 



Since this is independent of r, the same equation applies to a 
cylinder of finite thickness or to one solid throughout. 

The velocity of wave propagation is *J(n/p), and the whole 
theory is precisely similar to that of longitudinal vibrations, the 
condition for a free end being dO/dx = 0, and for a fixed end ^ = 0, 
or, if a permanent twist be contemplated, = constant. 

The velocity of longitudinal vibrations is to that of torsional 
vibrations in the ratio V? - V*^ or \/(2 + 2/a) : 1. The same ratio 
applies to the frequencies of vibration for bars of equal length 
vibrating in corresponding modes under corresponding terminal 
conditions. If /i = ^, the ratio of frequencies would be 

Vg: Vw = V8 : V3 = l-63, 

corresponding to an interval rather greater than a fifth. 

In any case the ratio of frequencies must lie between 

V2 : 1 = 1-414, and V3 : 1 = 1732. 

Longitudinal and torsional vibrations were first investigated by 

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160. In the present chapter we shall consider the lateral 
vibrations of thin elastic rods, which in their natural condition are 
straight. Next to those of strings, this class of vibrations is per- 
haps the most amenable to theoretical and experimental treatment. 
There is diflSculty sufficient to bring into prominence some im- 
portant points connected with the general theory, which the fami- 
liarity of the reader with circular functions may lead him to pass 
over too lightly in the application to strings ; while at the same 
time the difficulties of analysis are not such as to engross attention 
which should be devoted to general mathematical and physical 

Daniel Bernoulli ^ seems to have been the first who attacked 
the problem. Euler, Riccati, Poisson, Cauchy, and more recently 
Strehlke ', Lissajous ', and A. Seebeck ^ are foremost among those 
who have advanced our knowledge of it. 

161. The problem divides itself into two parts, according to 
the presence, or absence, of a permanent longitudinal tension. 
The consideration of permanent tension entails additional compli- 
cation, and is of interest only in its application to stretched 
strings, whose stiffiiess, though small, cannot be neglected al- 
together. Our attention will therefore be given principally to the 
two extreme cases, (1) when there is no permanent tension, 
(2) when the tension is the chief agent in the vibration. 

^ Comment. Acad, Petrop. t. xiii. > Pogg. Ann. Bd. xxvii. p. 505, ISSS. 

» Ann. d. CUmie (3), xxx. 386, 1860. 

« AbhandUmgen d. Math. Phys. Classe d. K. Sdchs. Gesellschaft d, Witten- 
tehaften. Leipzig, 1862. 

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With respect to the section of the rod, we shall suppose that 
one principal axis lies in the plane of vibration, so that the bending 
at every part takes place in a direction of maximum or minimum 
(or stationary) flexural rigidity. For example, the surface of the 
rod may be one of revolution, each section being circular, though 
not necessarily of constant radius. Under these circumstances the 
potential energy of the bending for each element of length is pro- 
portional to the square of the curvature multiplied by a quantity 
depending on the material of the rod, and on the moment of 
inertia of the transverse section about an axis through its centre of 
inertia perpendicular to the plane of bending. If od be the area 
of the section, k^o) its moment of inertia, q Young's modulus, ds the 
element of length, and dV the corresponding potential energy for 
a curvature 1 -s- ii of the axis of the rod, 

dV = iqK^<o^ 


This result is readily obtained by considering the extension of 
the various filaments of which the bar may be supposed to be 
made up. Let rj be the distance from the axis of the projection 
on the plane of bending of a filament of section da). Then the 
length of the filament is altered by the bending in the ratio 

li being the radius of curvature. Thus on the side of the axis for 
which 7f is positive, viz. on the outward side, a filament is extended, 
while on the other side of the axis there is compression. The 
force necessary to produce the extension rjlR is q rf/R . da> by the 
definition of Young's modulus; and thus the whole couple by 
which the bending is resisted amounts to 



. d(li) = -^ K^CO, 

if CD be the area of the section and k its radius of gyration about 
a line through the axis, and perpendicular to the plane of bending. 
The angle of bending corresponding to a length of axis ds is ds-i-It, 
and thus the work required to bend ds to curvature 1 -r- iZ is 

1 a ^ 

since the mean is half the final value of the couple. 

[For a more complete discussion of the legitimacy of the 

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foregoing method of calculation the reader must be referred to 
iiirorks upon the Theory of Elasticity. The question of lateral 
vibrations has been specially treated by Pochhammer^ on the 
basis of the general equations.] 

For a circular section /c is one-half the radius. 

That the potential energy of the bending would be proportional, 
ccBteris paribus, to the square of the curvature, is evident before- 
hand. If we call the coeflScient -B, we may take 

or, in view of the approximate straightness, 

^'^K^^ «• 

in which y is the lateral displacement of that point on the axis of 
the rod whose abscissa, measured parallel to the undisturbed posi- 
tion, is X, In the case of a rod whose sections are similar and 
similarly situated £ is a constant, and may be removed from under 
the integral sign. 

The kinetic energy of the moving rod is derived partly from 
the motion of translation, parallel to y, of the elements composing 
it, and partly from the rotation of the same elements about axes 
through their centres of inertia perpendicular to the plane of vibra- 
tion. The former part is expressed by 

i I /t>ft> y^dx , 


if p denote the volume-density. To express the latter part, we have 
only to observe that the angular displacement of the element dx is 
dy/dx, and therefore its angular velocity d^y/dt dx. The square of 
this quantity must be multiplied by half the moment of inertia of 
the element, that is, by ^/v'/xo dx. We thus obtain 

2'=i//,a.y'(te + i/«»p«(Hy«ir (4). 

1 CreUe, Bd. 81, 1876. 
R. 17 

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162. In order to form the equation of motion we may avail 
ourselves of the principle of virtual velocities. If for simplicity we 
confine ourselves to the case of uniform section, we have 

'"St-^^-'i^^ «• 

where the terms free from the integral sign are to be taken between 
the limits. This expression includes only the internal forces due 
to the bending. In what follows we shall suppose that there are 
no forces acting from without, or rather none that do work upon 
the system. A force of constraint, such as that necessary to hold 
any point of the bar at rest, need not be regarded, as it does no 
work and therefore cannot appear in the equation of virtual velo- 

The virtual moment of the accelerations is 
Thus the variational equation of motion is 

in which the terms free from the integral sign are to be taken 
between the limits. From this we derive as the equation to be 
satisfied at all points of the length of the bar 

while at each end 

or, if we introduce the value of B, viz. y/c*©, and write q/p = 6^ 
^'y + 6V»'^^-*»-^ = (4) 


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and for each end 

In these equations b expresses the velocity of transmission of 
longitudinal waves. 

The condition (5) to be satisfied at the ends assumes different 
forms according to the circumstances of the case. It is possible to 
conceive a constraint of such a nature that the ratio S (dy/dx) : Sy 
has a prescribed finite value. The second boundary condition is 
then obtained fi:om (5) by introduction of this ratio. But in all 
the cases that we shall have to consider, there is either no constraint 
or the constraint is such that either 8 {dyldx) or 8y vanishes, and 
then the boundary conditions take the form 


<t)-'- {^-"U]^'" <«^ 

We must now distinguish the special cases that may arise. If 
an end be free, Sy and B{dy/dx) are both arbitrary, and the 
conditions become 

a^ ' dt^dx daf 

the first of which may be regarded as expressing that no couple 
acts at the free end, and the second that no force acta 

If the direction at the end be free, but the end itself be con- 
strained to remain at rest by the action of an applied force of the 
necessary magnitude, in which case for want of a better word the 
rod is said to be supported, the conditions are 

S=0' «y=o (8). 

by which (5) is satisfied. 

A third case arises when an extremity is constrained to main- 
tain its direction by an applied couple of the necessary magnitude, 
but is free to take any position. We have then 



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Fourthly, the extremity may be constrained both as to 
position and direction, in which case the rod is said to be clamped. 
The conditions are plainly 


Sy = o (10). 

Of these four cases the first and the last are the more 
important; the third we shall omit to consider, as there are 
no experimental means by which the contemplated constraint 
could be realized. Even with this simplification a considerable 
variety of problems remain for discussion, as either end of the 
bar may be free, clamped or supported, but the complication 
thence arising is not so great as might have been expected. 
We shall find that diflferent cases may be treated together, 
and that the solution for one case may sometimes be derived 
immediately from that of another. 

In experimenting on the vibrations of bars, the condition 
for a clamped end may be realized with the aid of a vice of 
massive construction. In the case of a free end there is of course 
DO difficulty so far as the end itself is concerned ; but, when both 
ends are free, a question arises as to how the weight of the bar 
is to be supported. In order to interfere with the vibration 
as little as possible, the supports must be confined to the neigh- 
bourhood of the nodal points. It is sometimes sufficient merely 
to lay the bar on bridges, or to pass a loop of string round the bar 
and draw it tight by screws attached to its ends. For more exact 
purposes it would perhaps be preferable to cany the weight of 
the bar on a pin traversing a hole drilled through the middle of 
the thickness in the plane of vibration. 

When an end is to be 'supported,' it may be pressed into 
contact with a fixed plate whose plane is perpendicular to the 
length of the bar. 

163. Before proceeding further we shall introduce a sup- 
position, which will greatly simplify the analysis, without seriously 
interfering with the value of the solution. We shall assume that 
the terms depending on the angular motion of the sections of 
the bar may be neglected, which amounts to supposing the 
inertia of each section concentrated at its centre. We shall 
afterwards (§ 186) investigate a correction for the rotatory in- 

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ertia, and shall prove that under ordinary circumstances it is 
small. The equation of motion now becomes 

S^-'-S-o «• 

xmd the boundary conditions for a free end 

g-». s-» *^^ 

The next step in conformity with the general plan will be 
the assumption of the harmonic form of y. We may conveniently 

y^u cos 

(ym'f) (3), 

where I is the length of the bar, and 7n is an abstract number, 
whose value has to be determined. Substituting in (1), we 

d^^T"" ^*>- 

If t/ = eP"^' be a solution, we see that p is one of the fourth 
roots of unity, viz. +1, —1, +i, — i; so that the complete 
solution is 

t* = 4cosm|+58iiim| + (7e«*" + jDe-^/' (4a), 

containing four arbitrary constants. 

[The simplest case occurs when the motion is strictly periodic 
with respect to x, C and D vanishing. If \ be the wave-length 
and T the period of the vibration, we have 

2ir m 27r ,m* 

«^*^** ^=2^6 ^*^>-l 

In the case of a finite rod we have still to satisfy the four 
boundary cx)nditions, — two for each end. These determine the 
ratios A : B : C : D, and furnish besides an equation which m 
must satisfy. Thus a series of particular values of m are alone 
admissible, and for each m the corresponding u is determined in 
everything except a constant multiplier. We shall distinguish the 
different fiinctions u belonging to the same system by suffixes. 

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The value of y at any time may be expanded in a series of 
the functions u (§§ 92, 93). If <^, ^, &c. be the normal co- 
ordinates, we liave 

j^ = <^Wi + <^ti,+ (5), 

and r = i/>« |(^t^i + ^atij-f ...ydx 

= i/>»Ui*[wi»da7 + 4>,«A/,»dar+...l (6), 

We are fully justified in asserting at this stage that each 
integrated product of the functions vanishes, and therefore the 
process of the following section need not be regarded as more 
than a verification. It is however required in order to determine 
the value of the integrated squares. 

164. Let Umy Unc denote two of the normal functions cor- 
responding respectively to m and m\ Then 

or, if dashes indicate differentiation with respect to {mxjl), 

tim"" = t^, t^'''" = U^' (2). 

If we subtract equations (1) after multiplying them by m,« , 
M,rt respectively, and then integrate over the length of the bar, 
we have 

•"''"*'d^ "'''"' da^^ dx dx' '^ dx dx' ^•^^' 

the integrated terms being taken between the limits. 

Now whether the end in question be clamped, supported, or 
f^ee^ each term vanishes on account of one or other of its 

^ The reader sbonld observe that the oases here specified are partioolar, and 
that the right-hand member of (S) yanishes, provided that 

Bnd ^^ : ^"«»=^"«>' ; ^^', 

dx ' dx' dx ' dx* 

These conditions indade, for instance, the case of a rod whose end is urged 
towards its position of eqnilibrinm by a force proportional to the displacement, as 
hy a spring without inertia. 


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fetctors. We may therefore conclude that, if Um, Um' refer to two 
modes of vibration (corresponding of course to the same terminal 
conditions) of which a rod is capable, then 


jUmthn'dx^O (4), 

provided m and m' be different. 

The attentive reader will perceive that in the process just 
followed, we have in fact retraced the steps by which the funda- 
mental differential equation was itself proved in § 162. It is the 
original variaHonal equation that has the most immediate con- 
nection with the conjugate property. If we denote y by w and 8y 

ajid the equation in question is 

^/SS*'+^'"/**'*'=^ <^>- 

Suppose now that u relates to a normal component vibration, 
so that H + v?u = 0, where n is some constant ; then 


By similar reasoning, if v be a normal function, and u represent 
any displacement possible to the system, 

n'*p<.fuvdx = BJ^^d<v. 

We conclude that if u and v be both normal functions, which 
have different periods, 

\yvdx = (6); 


and this proof is evidently as direct and general as could be 

The reader may investigate the formula corresponding to (6), 
when the term representing the rotatory inertia is retained. 

By means of (6) we may verify that the admissible values of n^ 
are real. For if w* were complex, and u = a + ifi were a normal 
function, then a -1^9, the conjugate of u, would be a normal 
function also, corresponding to the conjugate of n', and then the 

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product of the two functions, being a sum of squares, would not 
vanish, when integrated^ 

If in (3) 771 and m be the same, the equation becomes iden- 
tically true, and we cannot at once infer the value of jv^dir. 
We must take m' equal to m + Sm, and trace the limiting form of 
the equation as hm tends to vanish. [It should be observed that 
the function tt^+sm is not a normal function of the system ; it is 
supposed to be derived from v^ by variation of m in (4fa) § 163, 
the coeflScients A, B,C, D being retained constant.] In this way 
we find 

4m^ r 2^ « _^ ^ _ ^ ^ 4. ^ A. ^^ _du d d?u 
b J dmda^ dmda? da^dmdx dxdmdx^' 

the right-hand side being taken between the limits. 

*T du m , o du X , a 

Now dS = T"''^-' d;» = l"'"^' 

and thus 

in which v!'" = w, so that 

-y I Wm^Cto = 3mm " + -p t^« p U m'" - w'll" + -j- (it ')'. - .(7), 

between the limits. 

Now whether an end be clamped, supported, or free, 

and thus, if we take the origin of x at one end of the rod, 

[\t«(ia;= ft (tt»- 2w'ir + u"«)y 

= ii(M«-2M'u'" + w"Vf .....(8). 

The form of our integral is independent of the terminal con- 
dition at a? = 0. If the end ir = Z be free, u" and u'" vanish, and 

[ u^dx = \l u^{iy (9). 

^ This method is, I belieye, doe to Poisson. 

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that is to say, for a rod with one end free the mean value of u^ is 
one-fourth of the terminal value, and that whether the other end 
be clamped, supported, or free. 

Again, if we suppose that the rod is clamped at a; = Z, u and u' 
vanish, and (8) gives 

Since this must hold good whatever be the terminal condition at 
the other end, we see that for a rod, one end of which is fixed and 
the other free, 

( u^dx = ^lu^ (free end) = \W^ (fixed end), 

shewing that in this case u^ at the free end is the same as w"" at 
the clamped end. 

The annexed table gives the values of four times the mean of u' 
in the different cases. 

clamped, free 

free, free 

w' (free end), or w"' (clamped end) 

w* (free end) 

m"' (clamped end) 

- 2u'u"' (supported end) = 2u" 

M* (free end), or - 2u'u'" (supported end) 

w"* (clamped end), or - 2m' m'" (supported end) 

clamped, clamped ... 
supported, supported 

supported, free 

supported, clamped 

By the introduction of these values the expression for T 
assumes a simpler form. In the case, for example, of a clamped- 
free or a free-free rod, 

2'=^{^*V(0+^.''«,'(0 + ...} (10), 

where the end x=^l is supposed to be free. 

166. A similar method may be applied to investigate the 
values of ju'^dx, and jv!'^dx. In the derivation of equation (7) of 
the preceding section nothing was assumed beyond the truth of 
the equation v!'" ^u, and since this equation is equally true of any 

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of the derived functions, we are at liberty to replace u by u' or u\ 

taken between the limits, since the term u vl' vanishes in all three 

For a free-free rod 

~j u'^dx = 3 (uu')i - 3 {uu\ + m (u'O/ 

= 6(Mi£'), + m(tt'«), (1), 

for, as we shall see, the values of uu' must be equal and opposite 
at the two ends. Whether u be positive or negative at a? = /, 
u v! is positive. 

For a rod which is clamped at a; = and free at a; = / 

*PJu'^dx = 3 {uuy + mui'^ + {u''u'"\. 

[We have already seen that Uo'=± ui; and it may be proved 
from the formulee of § 173 that 

Wo'" _ w/ _ cos m + cosh m 
u{ " vi sin m sinh m * 



. 1 . (m"w'")o (cos m 4- cosh my , 

tnat -7-7 — r- = — r-T r— rr = — l.J 

{uu)i sm'msmh'm 

yju'*da!^2(uu)i + mur' (2), 

4m r' 
a result that we shall have occasion to use later. 


By applying the same equation to the evaluation of 1 u"*dx, we 

=rm(w"«-2w'a'" + t*'')/, 

since w'u" and wu'" vanish. 

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Comparing this with (8) § 164, we see that 

ju''^dx=ju*dx (3), 

whatever the terminal conditions may be. 

The same result may be arrived at more directly by integrating 
by parts the equation 

m* . d*u 

166. We may now form the expression for V in terms of the 
normal co-ordinates. 



If the functions u be those proper to a rod free at a; = /, this expres- 
sion reduces to 

F=^|^|7n,*K(0?*,« + 7i^*K(0?*,«+...} (2). 

In any case the equations of motion are of the form 

p(DWdx 4>i'h—ijr^nH*Wdx ^ = *i (3), 

and, since ^iS^ is by definition the work done by the impressed 
forces during the displacement S<^, 

^1 = j YtLipcadx (4). 

if YptDdx be the lateral force acting on the element of mass ptodx. 
If there be no impressed forces, the equation reduces to 

*> + ^t^V = (5). 

as we know it ought to do. 

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167. The significance of the reduction of the integrals 
Ju^dnc to dependence on the terminal values of the function and 
its derivatives may be placed in a clearer light by the following 
line of argument. To fix the ideas, consider the case of a 
rod clamped at a? = 0, and free at fl5 = Z, vibrating in the normal 
mode expressed by u. If a small addition Al be made to the 
rod at the free end, the form of u (considered as a function of 
x) is changed, but, in accordance with the general principle 
established in Chapter iv. (§ 88), we may calculate the period 
under, the altered circumstances without allowance for the change 
of type, if we are content to neglect the square of the change. 
In consequence of the straightness of the rod at the place where 
the addition is made, there is no alteration in the potential 
energy, and therefore the alteration of period depends entirely 
on the variation of T, This quantity is increased in the ratio 

I u^dx : I V 
Jo Jo 





which is also the ratio in which the square of the period is 
augmented. Now, as we shall see presently, the actual period 
varies as P, and therefore the change in the square of the period 
is in the ratio 

1:1 + 4Ai/i. 

A comparison of the two ratios shews that 


: ju^dx=^ 

4 : L 

The above reasoning is not insisted upon as a demonstration, 
but it serves at least to explain the reduction of which the in- 
tegral is susceptible. Other cases in which such integrals occur 
may be treated in a similar manner, but it would often require 
care to predict with certainty what amount of discontinuity in the 
varied type might be admitted without passing out of the range 
of the principle on which the argument depends. The reader 
may, if he pleases, examine the case of a string in the middle 
of which a small piece is interpolated. 

168. In treating problems relating to vibrations the usual 
course has been to determine in the first place the forms of the 
normal functions, viz. the functions representing the normal 

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types, and afterwards to investigate the integral formulse by 
means of which the particular solutions may be combined to 
suit arbitrary initial circumstances. I have preferred to follow 
a different order, the better to bring out the generality of the 
method, which does not depend upon a knowledge of the normal 
fiOictione. In pursuance of the same plan, I shall now investigate 
the connection of the arbitrary constants with the initial circum- 
stances, and solve one or two problems analogous to those treated 
under the head of Strings. 

The general value of y may be written 

y = f -4i cos y niiH + Bi sin ^- miHj Ui 

/ tcb Kb \ 

+ ( -4j cos -^ rn^H + B^ sin y m^Hj u^ 

+ (1), 

so that initially 

yo = ^iWi + -4,t4,+ (2), 

yo = -|i^{^"Ai*i + ^'^j^ + ...} (3). 

If we multiply (2) by t^ and integrate over the length of the 
rod, we get 

[y^xirdx — Ar lur^dx (4), 

and similarly from (3) 

■l^jyoUrdx=-nir''Brjur^dx (5), 

formulae which determine the arbitrary constants Art Br* 

It must be observed that we do not need to prove analytically 
the possibility of the expansion expressed by (1). If all the 
particular solutions are included, (1) necessarily represents the 
most general vibration possible, and may therefore be adapted 
to represent any admissible initial state. 

Let us now suppose that the rod is originally at rest, in its 
position of equilibrium, and is set in motion by a blow which 
imparts velocity to a small portion of it. Initially, that is, at 
the moment when the rod becomes free, y© = 0, and y© differs from 
zero only in the neighbourhood of one point {x = c). 

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From (4) it appears that the coefBcients A vanish, and frcn 
(5) that 

rrir^Br I Ur^dx ^-j^u^(c) I jff^dx. 

Calling fyopwdx, the whole momentum of the blow, Y, we 

J. _ 1*7 t/,(c) 

^'~Kb(m mr'fur'dx ^^^' 

and for the final solution 

l^y {Me)uy(a!).('cb \ 

-^5s^(f-'0- } (^)- 

In adapting this result to the case of a rod free at ^ = 2, we 
may replace 

fur^dx by \l[ur(l)]\ 


If the blow be applied at a node of one of the normal com- 
ponents, that component is missing in the resulting motion. The 
present calculation is but a particular case of the investigation 
of § 101. 

169. As another example we may take the case of a bar, 
which is initially at rest but deflected from its natural position 
by a lateral force acting at x = c. Under these circumstances 
the coeflScients B vanish, and the others are given by (4), § 168. 


and on integrating by parts 

j^y^l^^^y'd^^ di d^ 

in which the terms free from the integral sign are to be taken 
between the limits ; by the nature of the case j/q satisfies the 
same terminal conditions as does tir, and thus all these terms 

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169.] SPECIAL CASES. 271 

vanish at both limits. If the external force initially applied 
to the element dx be Ydx, the equation of equilibrium of the 
bar gives 

,«^6«g«=F (1). 

and accordingly 

If we now suppose that the initial displacement is due to 
a force applied in the immediate neighbourhood of the point 
a; = c, we have 

and for the complete value of y at time t, 

In deriving the above expression we have not hitherto made 
any special assumptions as to the conditions at the ends, but 
if we now confine ourselves to the case of a bar which is clamped 
at d; » and free at a? = i, we may replace 

Lr^dx by ii[Wr(OP- 

If we suppose further that the force to which the initial deflection 
is due acts at the end, so that c = /, we get 

When ^ = 0, this equation must represent the initial displace- 
ment. In cases of this kind a difficulty may present itself as 
to how it is possible for the series, every term of which satisfies 
the condition j/" ^0^ to represent an initial displacement in 
which this condition is violated. The fact is, that after triple 
differentiation with respect to x^ the series no longer converges 
for a? = Z, and accordingly the value of j/" is not to be arrived 
at by making the differentiations first and summing the terms 
afterwards. The truth of this statement will be apparent if 
we consider a point distant dl from the end, and replace 

M"\l^dl) by v:"{l)-u^{l)dl, 

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in which v}"^ (I) is equal to 

For the solution of the present problem by normal co-ordinates 
the reader is referred to § 101. 

170. The forms of the normal functions in the various par- 
ticular cases are to be obtained by determining the ratios of the 
four constants in the general solution of 

If for the sake of brevity w be written for (mx/l), the solution 
may be put into the form 

w = -4 (cos X 4- cosh x) + B (cos sc' - cosh a?') 

+ G(smx +sinh a?') +i5(sina?' — sinha?') (1), 

where cosh x and sinh x are the hyperbolic cosine and sine of x, 
defined by the equations 

coshir = J(6* + e-*), sinha? = J(e*-c-*) (2). 

I have followed the usual notation, though the introduction of 
a special symbol might very well be dispensed with, since 

cosh X = cos ix, sinh a? = — i sin ta? (3), 

where % = V(— 1) J ^^^ ^^^^ ^^^ connection between the formulae of 
circular and hyperbolic trigonometry would be more apparent. The 
rules for differentiation are expressed in the equations 

-7- cosh X = sinh x, -y- sinh x = cosh x 
ax ax 

-j-^ cosh X = cosh X, -7-^ sinh x = sinh x. 

In differentiating (1) any number of times, the same four com- 
pound functions as there occur are continually reproduced. The 
only one of them which does not vanish with x is cos x + cosh x\ 
whose value is then 2. 

Let us take first the case in which both ends are free. Since 
d^u/dx!^ and d^ujda? vanish with a?, it follows that jB = 0, i) = 0, so 

11 = A (cos x' + cosh x') + C (sin x' + sinh x) (4). 

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We have still to satisfy the necessary conditions when a? = Z, or 
X = 7». These give 

-4 (—cos mH- cosh m)+ 0(- sinm + sinhm) — ) 

A{^ sinw + sinhm)+ C(-co8mH-coshm) = j ^ '' 

equations whose compatibility requires that 

(cosh m — cos mf = sinh" m — sin" m, 

or in virtue of the relation 

cosh'm — sinh'w = l (6), 

cosm cosh w = l (7). 

This is the equation whose roots are the admissible values of m. 
If (7) be satisfied, the two ratios oi A \ G given in (6) are equal, 
and either of them may be substituted in (4). The constant multi- 
plier being omitted, we have for the normal function 

u = (sin m — sinh m) jcos -j- + cosh -j- 1 

— (cos m — cosh w) -jsin ,-H-sinh-y|- (8), 

or, if we prefer it, 

u = (cos m — cosh m) jcos -j- + cosh -p[ 

+ (sin mH- sinh 7w) -jsin -^ + sinh j-y (9); 

and the simple harmonic component of this type is expressed by 


y=:Pttcos(~m«^+e) (10). 

171. The frequency of the vibration is o~ii^'» ^^ which b is 

a velocity depending only on the material of which the bar is 
formed, and m is an abstract number. Hence for a given material 
and mode of vibration the frequency varies directly as k — ^the 
radius of gyration of the section about an axis perpendicular to the 
plane of bending — and inversely as the sqimre of the length. These 
results might have been anticipated by the argument from dimen- 
sions, if it were considered that the frequency is necessarily 
determined by the value of Z, together with that of xb — the 
only quantity depending on space, time and mass, which occurs in 
R. 18 

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the differential eqaation. If eyerything ooncenuDg a bar be given, 
except its absolute magnitude, the frequency yaries inversely as 
the linear dimension. 

These laws find an important application in the case of tuning- 
forks, whose prongs vibrate as rods, fixed at the ends where they 
join the stalk, and free at the other ends. Thus the period of vibra- 
tion of forks of the same material and shape varies as the linear 
dimension. The period will be approximately independent of the 
thickness perpendicular to the plane of bending, but will vary 
inversely with the thickness in the plane of bending. When the 
thickness is given, the period is as the square of the length. 

Jn order to lower the pitch of a fork we may, for temporary 
purposes, load the ends of the prongs with soft wax, or file away 
the metal near the base, thereby weakening the spring. To raise 
the pitch, the ends of the prongs, which act by inertia, may be 

The value of b attains its maximum in the case of steel, for 
which it amounts to about 5287 metres per second. For brass 
the velocity would be less in about the ratio 1*5 : 1, so that a 
tuning-fork made of brass would be about a fifth lower in pitch 
than if the material were steel. 

[For the design of steel vibrators and for rough determinations 
of frequency, especially when below the limit of hearing, the 
theoretical formula is often convenient. If the section of the bar 
be rectangular and of thickness t in the plane of vibration, k* « i^; 
and then with the above value of 6, and the values of m given 
later, we get as applicable to the gravest mode 

(clamped-free) frequency = 84590 f/P, 

(free-free) frequency = 538400 t/P, 

I and t being expressed in centimetrea 

The first of these may be used to calculate the pitch of steel 

The lateral vibrations of a bar may be excited by a blow, as 
when a tuning-fork is struck against a pad. This method is also 
employed for the barmonicon, in which strips of metal or glass are 
supported at the nodes, in such a manner that the fi*ee vibrations 
are but little impeded. A frictional maintenance may be obtained 

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with a bow, or by the action of the wetted fingers upon a slender 
rod of glass suitably attached. The electro-magnetic maintenance 
of forks has been already considered, § 64. It may be applied with 
equal facility to the case of metal bars, or even to that of 
wooden planks carrying iron armatures, free at both ends and 
supported at the nodes. The maintenance by a stream of wind 
of the vibrations of harmonium and organ reeds may also be 
referred to. 

The sound of a bar vibrating laterally may be reinforced by a 
suitably tuned resonator, which may be plcu^ed under the middle 
portion or under one end. On this principle dinner gongs have 
been constructed, embracing one octave or more of the diatonic 

172. The solution for the case when both ends are clamped 
may be immediately derived from the preceding by a double dif- 
ferentiation. Since y satisfies at both ends the terminal con- 

^y^o ^y=o 

it is clear that y" satisfies 

■-»• f-». 

which are the conditions for a clamped end. Moreover the general 
differential equation is also satisfied by y". Thus we may take, 
omitting a constant multiplier, as before, 

u = (sin m — sinh m) {cos a?' — cosh x'} 

— (cos m — cosh m) {sin a?' — sinh a?'} (1), 

while m ia given by the same equation as before, nam ely, 

cosm coshm=l (2). 

We conclude that the component tones have the same pitch in the 
two cases. 

In each case there are four systems of points determined by 
the evanescence of y and its derivatives. Where y vanishes, there 
is a node ; where y' vanishes; a loop, or place of maximum displace- 
ment; where y" vanishes, a point of inflection; and where y"' 
vanishes, a place of maximum curvature. Where there are in the first 
case (free-firee) points of inflection and of maximum curvature, there 


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are in the second (clamped-clamped) nodes and loops respectively; 
and vice versd, points of inflection and of maxiraum curvature for 
a doubly-clamped rod correspond to nodes and loops of a rod whose 
ends are free. 

173. We will now consider the vibrations of a rod clamped at 
a? = 0, and free at a? = Z. Reverting to the general integral (1) 
§ 170, we see that A and C vanish in virtue of the conditions at 
^ s 0, so that 

t^ = JB(cosa?' — coshir') + D(sina;'-8inha?') (1). 

The remaining conditions at x = l *give 

JB( cosm + cosh m) + i)(sin m -|-sinhm) = ) 
B (- sin m + sinh m) + D (cos m + cosh w) = j * 

whence, omitting the constant multiplier, 

u = (sin m + sinh m) jcos , cosh -j-y 

— (cos m + cosh m) jsin -, - sinh -,- 1 (2), 


u = (cos m + cosh m) jcos -j — cosn -j-Y 

+ (smm — smhm) jsm —, — smh-y^ > (3), 

where m must be a root of 

cosm cosh m + 1=0 .(4). 

The periods of the component tones in the present problem are 
thus different from, though, as we shall see presently, nearly re- 
lated to, those of a rod both whose ends are clamped, or free. 

If the value of w in (2) or (3) be differentiated twice, the re- 
sult {u") satisfies of course the fundamental differential equation. 
At a? = 0, d?u"lda^, d^u^jda^ vanish, but at a? = i u" and du"ldx 
vanish. The function u" is therefore applicable to a rod clamped 
at I and free at 0, proving that the points of inflection and of 
maximum curvature in the original curve are at the same distances 
from the clamped end, as the nodes and loops respectively are 
from the free end. 

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174 In default of tables of the hyperbolic cosine or its loga- 
rithm, the admissible values of m may be calculated as follows. 
Taking first the equation 

cosm coshm=sl (1), 

we see that m, when large, must approximate in value to 
^(2i + 1) TT, 1 being an integer. If we assume 

m = i(2t + l)^-(-l)»/8 (2), 

P will be positive and comparatively small in magnitude. 

Substituting in (1), we find 

cot i)9 = 6"* = e*<*<+^>' e-<-')^ ; 

or, if c*^'"'"''' be called a, 

atanii8=re(-W (3), 

an equation which may be solved by successive approximation after 
expanding tan^/8 and ^~'^'^ in ascending powers of the small 
quantity /3. The result is 

^ 2 , ^,,4 34 , ,wll2 


which is sufficiently accurate, even when % = 1. 

By calculation 

A « 0179666 - 0003228 + 0000082 - 0000002 = 0176518. 

/Ss) fit* 0*f fit are found still more easily. After ^o the first term of 
the series gives fi correctly as far as six significant figures. The 
table contains the value of fi, the angle whose circular measure is 
/3, and the value of sin ^/3, which will be required further on. 

Free-Free Bar. 


P expiesaed in degrees, 
minntes, and seoondg. 


1 1 10-' X -176518 

2 1 10-» X -777010 

3 10-« X -335506 

4 10-» X -144989 
6 ' 10-' X -626556 


1* 0' 40"-94 
2' 40''-2699 

10-* X -88258 
10-' X -38850 
10-* X -16775 
10-» X -72494 
10-' X -31328 

^ This process is somewhat similar to that adopted by Strehlke. 

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The values of r?i which satisfy (1) are 

Wi= 4-7123890 + i8,= 4-7300408 
r?i,= 7-8539816-^,= 7*8532046 
f/is = 10-9955743 + /S, = 10*9956078 
m, « 14-1371669 - A ^ 141371655 
m, = 17-2787596 + /^^ = l7-2787o9« 
after which m = ^(2i+ l)7r to seven decimal places. 

We will now consider the roots of the equation 

cosm co8hm = — 1 (5)^ 


w, = i(2i-l)7r-(-iyai (6), 

we have e"^ = cot ^Oi = e*^*'"*^' . e^^^^^^t , 

or a tan^Oi+i = e~<~^^*«+i (7), 

a having the value previously defined. 

Thus, as in (4), 

«"-'-(-v^,^.-(-»'"J+ (»)■ 

a,>, being approximately equal to /Si. 
The values calculated from (8) are 

a, = 10-^ X -182979, a, = 10"^ x 335527, 
a, - lO-» X -775804, a, = 10-» x 144989, 
after which the diflerence between «»•+! and fit does not appear.] 

The value of Oi may be obtained by trial and error from the 

logio cot i ai - -6821882 - -43429448 a, = 0, 

and will be found to be 

a, = -3043077. 

Another method by which mi may be obtained directly will be 
given presently. 

The values of m, which satisfy (5), are 

Tfh^ 1-5707963 + ai = 1875104 
m,= 4-7123890 -0^= 4-694098 
m,= 7-8539816 + a, = 7-854757 
m, = 10-9955743 - 04 = 10-995541 
VI, = 14-1371669 + a« = 14137168 
m. =: 17-2787596 - a. = 17-278759 , 

1 The caloolation of the roots of (5) giyen in the first edition was affected by an 
enor, ^hich has been pointed oat by Greenhill {Math, Me$s»^ Deo. 1SS6). 

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after which m = ^ (2t — 1) v sensibly. The frequencies are propor- 
tional to m', and are therefore for the higher tones nearly in the 
ratio of the squares of the odd numbera However, in the case of 
overtones of very high order, the pitch may be slightly disturbed 
by the rotatory inertia, whose effect is here neglected. 

175. Since the component vibrations of a system, not subject 
to dissipation^ are necessarily of the harmonic type, all the values 
of 711*, which satisfy 

cosm coshm= ± 1 (1), 

must be real. We see further that, if m be a root, so are also 
— m, m»J{— 1), — m^/('~ 1). Hence, taking first the lower sign, we 

^(c<.smcoshm+l) = l-j2 + j^2j^- 

-i^-m-w)'- «■ 

If we take the logarithms of both sides, expand, and equate co* 
efficients, we get 

2— ; = Tij; 2— :=St^.s^; &c (3). 

This is for a clamped-free rod. 

From the known value of 2m~^, the value of m^ may be derived 
with the aid of approximate values of ms, m, We find 

2w-^ = 006547621, 

and mf^ = -000004242 

mf^ = -000000069 

mr" = 000000005, 

whence m{-^ = 006543305 

giving rrii = "1875104, as before. 

In like manner, if both ends of the bar be clamped or free, 

•-igs^--(>-5)('-S)*- <*'■ 

whence 2 — r = tctoc ^^-y where of course the summation is exclu- 
nr IZ.O0 

sive of the zero value of m. 

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176. The frequencies of the series of tones are proportional to 
The interval between any tone and the gravest of the series 
may conveniently be expressed in octaves and fractions of an 
octave. This is effected by dividing the difference of the logarithms 
of m* by the logarithm of 2. The results are as follows : 







3-7382, &c. 

6-8288, &c. 

where the first column relates to the tones of a rod both whose 
ends are clamped, or free ; and the second column to the case of a 
rod clamped at one end but free at the other. Thus from the 
second column we find that the first overtone is 2*6478 octaves 
higher than the gravest tone. The fractional part may be reduced 
to mean semitones by multiplication by 12. The interval is then 
two octaves + 7*7736 mean semitones. It will be seen that the 
rise of pitch is much more rapid than in the case of strings. 

If a rod be clamped at one end and free at the other, the pitch 
of the gravest tone is 2 (log 4-7300 - log 1-8751) -r- log 2 or 2-6698 
octaves lower than if both ends were clamped, or both fr^e. 

177. In order to examine more closely the curve in which the 
rod vibrates, we will transform the expression for u into a form 
more convenient for numerical calculation, taking first the case 
when both ends are free. Since w = ^(2i + l)7r — (— 1)* /8, 
cosm = 8in/8, sinm = cosiV x cos)8; and therefore, m being a 
root of cos m cosh m = 1, cosh m = cosec /8. 


sinh' m = cosh' m — 1 = tan' m = cot^ /8, 

or, since cot /8 is positive, 

sinh m = cot /8. 


sin m — sinh m 1 — cos tV sin /3 

cos m — cosh m 


(cos ^ff — cos tV sin ^/8)' 

(cos J/3 — cos tV sin J/8)(cos i/8 + cos iir sin ^fi) 

_ cos ^/8 COS ITT — sin ^ff 
"" cos i/8 COB tTT + sin i^/S ' 


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We may therefore take, omitting the constant multiplier, 
u = (cos i/8 cos ITT + sm ijS) jsm -y- + smh -j- > 

cos -J- + cosh -y- r 

= V2cosi7rsin|^-^ + (-iy|| 

+ 8ini)8e««''-cosi7r cos^/Se-^*" (1). 

if we further throw out the factor V2, and put Z « 1, we 
may take 

W^J^i + i^ + i's, 


-Fj^cosiTTsinfma? — J7r + i( — l)*i8} \ 

logJ^,= Twa? log 6 + log sin ^^ — log V2 \ (*)» 

log±-F, = - Twojloge + logcosi/S — logV2 J 
from which u may be calculated for different values of i and x. 

At the centre of the bar, a? = ^, and -P,, F^ are numerically 
equal in virtue of ^ == cot ^ /3. When i is even, these terms cancel. 
For ^1, we have ^i = (— 1)* sin \ tV, which is equal to zero when 
% is even, and to ± 1 when t is odd. When i is even, therefore, 
the sum of the three terms vanishes, and there is accordingly a 
node in the middle. 

When a? = 0, w reduces to - 2 (- 1)< sin (J tt - i (- 1)* /8}, which 
(since fi is always small) shews that for no value of t is there a 
node at the end. If a long bar of steel (held, for example, at the 
centre) be gently tapped with a hammer while varying points of 
its length are damped with the fingers, an unusual deadness in 
the sound will be noticed, as the end is closely approached. 

178. We will now take some particular cases. 

Vibration witk two nodes. i=l. 

If i = 1, the vibration is the gravest of which the rod is capable. 
Our formulae become 

/\ « - sin [x{nO^ + V 0' 40" -94) - 45« - 30' 20" -47} 

log F^ = 2-054231 x + 3-7952391 

log jP, = - 2-054231 X + 1-8494681, 
from which is calculated the following table, giving the values of 
u for X equal to *00, 05, -10, &c. 

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The values o( u:u (-5) for the intermediate values of x (in the 
last column) were found by interpolation formulae. If o, p, q, r, e, t 
be six consecutive terms, that intermediate between q and r is 






u : u{-o) 



+ •7133200 

+ -0062408 


+ V4266401 

+ 1-645219 


• • • 

.. . 










. . . 












, ,, 





+ -0846166 







. . . 





- 1512020 



+ •I 394209 

+ 1607819 


< •• 



- 0054711 





- ^1415162 



< • • 

. .. 























. • • 























. . . 




-I 000000 

+ ^0664285 


- -8671433 

- 1^0000000 

Since the vibration curve is symmetrical with respect to the 
middle of the rod, it is unnecessary to continue ihe table beyond 
X = '5. The curve itself is shewn in fig. 28. 

Fig. 28. 

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To find the position of the node, we have by interpolation 

^ = -2<^ + SrO-<>2^ = -22418. 

which is the firaction of the whole length by which the node is 
distant Jrom the nearer end. 

Vibration with three nodes, i » 2. 

J*! = sin { (450» - 2' 40" -27) a; - 45» + 1' 20" -135} 

logFt= S-410604;e+ 4-438881 6 

log (- i",) = - 3-410604 X + 1-8494850. 


« : - M (0) 






+ •5847 


















- 0487 

[ 376 



+ 1175 





1 ^425 












In this table, as in the preceding, the values of u were calcu- 
lated directly for x = '000, "050, '100 &c , and interpolated for the 
intermediate values. For the position of the node the table gives 
by ordinary interpolation a? = '132. Calculating from the above 
formulae, we find 

i^(1321) = --000076. 

1^ (-1322)=: + -000881, 

whence a? = •132108, agreeing with the result obtained by Strehlke. 
The place of maximum excursion may be found from the derived 
function. We get 

u (-3083) = + 0006077, u' (3084) = - -0002227, 

whence u' (-308373) = 0. 

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Hence ti is a maximum, when a; = '308373; it then attains 
the value '6636, which, it should be observed, is much less than 
the excursion at the end. 

The curve is shewn in fig. 29. 

Fig. 29. 

Vibration with four nodes, i ^ 3. 

^1 = - sin j (630^ + 6"'92) « - 45« - 3'H6}, 
log F, =: 4-775332 x + 5-0741527, 
log F, « - 4-775332 x + 1'8494850. 
From this ^(0) = 1'41424, w(i) = 1-00579. The positions of 
the nodes are readily found by trial and error. Thus 

u (3558) = - -000037 u ('3559) = + '001047, 
whence u ('355803) = 0. The value of x for the node near the end 
is -0944, (Seebeck). 

The position of the loop is best found from the derived 
function. It appears that u' = 0, when x = -2200, and then 
u=s — -9349. There is also a loop at the centre, where however 
the excursion is not so great as at the two others. 

Fig. 30. 

We saw that at the centre of the bar F^ and F^ are numerical!; 
equal. In the neighbourhood of the middle, F^ is evidently veiy 
small, if i be moderately great, and thus the equation for the nodes 
reduces approximately to 

l 4^^ ^^ 2' 


n being an integer. If we transform the origin to the centre of 
the rod, and replace m by its approximate value ^(2t + l)9r, we 

05 _ ± 2n — i 

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shewing that near the middle of the bar the nodes are uniformly 
spaced, the interval between consecutive nodes being 22-f-(2t + 1). 
This theoretical result has been verified by the measurements of 
Strehlke and Lissajoua 

For methods of approximation applicable to the nodes near 
the ends, when i is greater than 3, the reader is referred to the 
memoir by Seebeck already mentioned § 160, and to Donkin's 
Acoustics (p. 194). 

179. The calculations are very similar for the case of a bar 
clamped at one end and free at the other. If uoc F, and 
F^Fi+Fi + Fi, we have in general 

jPi = cos {mx + i 7r + i (- 1 )»a}, 

C - IV 1 

= ^-^-sinia^«*; ^, = ---^cosia6-^. 

If t = 1, we obtain for the calculation of the gravest vibration- 

log (- Ft) = mx\oge + T-0300909. 
log (- F,)='-mx log e + 1-8444383. 
These give on calculation 

/'(0) = -000000. 

if(-2) = -102974, 

-F (-4) = -370625, 

i'C -6)= -743452, 
F( -8) = 1-169632. 
^(10) = 1-612224, 

from which fig. 31 was constructed. 

Fig. 81. 

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The distances of the nodes from the free end in the case of a 
rod clamped at the other end are given by Seebeck and by Donkin. 

2"^ tone -2261. 

3"" tone -1321, 4999. 

4'" tone -0944, -3558, -6439. 

-i, 1-3222 4-9820 9-0007 4/- 3 4t- 10-9993 4»- 7-0175 
^"^4i-2' 4i-2' 4i-2'4i-2' 4t-2 ' 4i-2 ' 

"The last row in this table must be understood as meaning 



, . Q may be taken as the distance of the j^ node from the 

free end, except for the first three and the last two nodes." 

When both ends are free, the distances of the nodes from the 
nearer end are 

1* tone -2242. 

2"* tone 1321 


3"* tone -0944 


^ , 1-3222 

intone -^.^2 

4i + 2 

41 + 2 

4;- 3 

4i + 2 

The points of inflection for a free-free rod (corresponding to 
the nodes of a clamped-clamped rod) axe also given by Seebeck ;— 

1"' point 

2°<1 point 



1»' tone 
2°d tone 
3^ tone 

t'^ tone 





No inflection point. 

4t + 2 



Except in the case of the extreme nodes (which have no 
corresponding inflection-point), the nodes and inflection-points 
always occur in close proximity. 

180. The case where one end of a rod is fr^ee and the other 
supported does not need an independent investigation, as it maybe 

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referred to that of a rod with both ends free vibrating in an even 
mode, that is, with a node in the middle. For at the central node 
y and y" vanish, which are precisely the conditions for a supported 
end. In like manner the vibrations of a clamped-supported rod 
are the same as those of one-half of a rod both whose ends are 
clamped, vibrating with a central node. 

181. The last of the six combinations of terminal conditions 
occurs when both ends are supported. Referring to (1) § 170, we 
see that the conditions at a? — 0, give -4. = 0, fi = ; so that 

M = (0 + i)) sin a?' + (C - i)) sinh a:'. 

Since u and u" vanish when a:' = m, C — D = 0, and sin m « 0. 

Hence the solution is 

. iirx i^it^Kh ^ ,_. 

y=8m ^- cos— p— e (1), 

where i is an integer. An arbitrary constant multiplier may of 
course be prefixed, and a constant may be added to t 

It appears that the normal curves are the same as in the case 
of a string stretched between two fixed points, but the sequence of 
tone is altogether different, the frequency varying as the square 
of 1. The nodes and inflection-points coincide, and the loops 
(which are also the points of maximum curvature) bisect the 
distances between the nodes. 

182. The theory of a vibrating rod may be applied to illustrate 
the general principle that the natural periods of a system fulfil the 
maximum-minimum condition, and that the greatest of the natural 
periods exceeds any that can be obtained by a variation of 
type. Suppose that the vibration curve of a clamped-free rod is 
that in which the rod would dispose itself if deflected by a force 
applied at its free extremity. The equation of the curve may be 
taken to be 

y = -3Za:» + ^, 

which satisfies d^yjdx^ = throughout, and makes y and y' vanish 
at 0, and y" at I, Thus, if the configuration of the rod at time t be 

y^i-Zla^-^-a*) Qospt (1), 

the potential energy is by (1) § 161, % qi^ <ol* cob^^ pty while the 

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kinetic energy is ^ptoP p* sm* pt ; and thus jj* = — . . 
Now pi (the true value of p for the gravest tone) is equal to 

SO that 

2>,:p = (l-8751)«y^ = -98556, 

shewing that the real pitch of the gravest tone is rather (but 
comparatively little) lower than that calculated from the hypo- 
thetical tjrpe. It is to be observed that the hypothetical tyi>e in 
question violates the terminal condition y^''= 0. This circumstance, 
however, does not interfere with the application of the principle, 
for the assumed type may be any which would be admissible as an 
initial configuration ; but it tends to prevent a very close agree- 
ment of periods. 

We may expect a better approximation, if we found our calcu- 
lation on the curve in which the rod would be deflected by a force 
acting at some little distance from the free end, between which 
and the point of action of the force {x^c) the rod would be 
straight, and therefore without potential energy. Thus 

potential energy = 6 g^oic* cos* 2>^. 

The kinetic energy can be readily found by integration from 
the value of y. 

From to c y = — 3ca?' 4- si^ ; 

and from ciol y^c^{C'- Zx), 

as may be seen from the consideration that y and y' must not 
suddenly change at a? = c. The result is 


kinetic energy = p<» p^ sin* l^d yg c' + i c* (Z - c) (c* + ZV) , 

The maximum value of l//>* will occur when the point of 
application of the force is in the neighbourhood of the node of the 
second normal component vibration. If we take c = f Z, we obtain 
a result which is too high in the musical scale by the interval 

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182.] LOADED END. 289 

expressed by the ratio 1 : '9977, and is accordingly extremely near 
the truth. This example may give an idea how nearly the period 
of a vibrating system may be calculated by simple means without 
the solution of diflFerential or transcendental equations. 

The type of vibration just considered would be that actually 
assumed by a bar which is itself devoid of inertia, but carries a 
load M at its free end, provided that the rotatory inertia of M could 
be neglected. We should have, in fact, 

F= 6gr/c*a>Z' cos» pt, T = iMV'p^ sin* j)t, 

BO that P'--M¥ (3>- 

Even if the inertia of the bar be not altogether negligible in 
comparison with if, we may still take the same type as the basis 
of an approximate calculation : 




r= {2MI' + 1? pwp"^ p» sin«pe, 

that is, M is to be increased by about one quarter of the mass of 
the rod. Since this result is accurate when M is infinite, and does 
not differ much from the truth, even when if =0, it may be re- 
garded as generally applicable as an approximation. The error 
will always be on the side of estimating the pitch too high. 

183. But the neglect of the rotatory inertia of M could not 
be justified under the ordinary conditions of experiment. It is as 
easy to imagine, though not to construct, a case in which the inertia 
of translation should be negligible in comparison with the inertia of 
rotation, as the opposite extreme which has just been considered. 
If both kinds of inertia in the mass M be included, even though 
that of the bar be neglected altogether, the system possesses two 
distinct and independent periods of vibration. 

Let z and denote the values of y and dyjdx at a; = Z. Then 
the equation of the curve of the bar is 

R. 19 

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^^{9^-3110+ I'd*] 

while for the kinetic energy 

T=iM£*+\MK'^^- (2), 

if k' be the radius of gyration of M about an axis perpendicular to 
the plane of vibration. 

The equations of motion are therefore 

Mk'*'e + ^-p^i-3lz + 21*6) = 
whence, if z and 6 vary as cos pt, we find 

corresponding to the two periods, which are always different. 

If we neglect the rotatory inertia by putting tc' = 0, we fiJl 
back on our previous result 


P' = 



The other value of p" is then infinite. 

1{ k' '.I be merely small, so that its higher powers may be 

^_4iqi(^(of, . 9«'^"\ 

P' = 

P Ml* \ 4 I*)) 


If on the other hand k^ be very great, so that rotation is 

^ _ 12 qfc^(o 




the latter of which is very small. It appears that when rotation 
is prevented, the pitch is an octave higher than if there were no 
rotatory inertia at all. These conclusions might also be derived 

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directly from the diflFerential equations ; for if ic' = oo , tf := 0, and 

but if «' = 0, = Szf2l, by the second of equations (3), aud in 
that case 

Mi + --^ — z = 0. 

184. If any addition to a bar be made at the end, the period 
of vibration is prolonged. If the end in question be free, suppose 
first that the piece added is without inertia. Since there would be 
no alteration in either the potential or kiuetic energies, the pitch 
would be unchanged; but in proportion as the additional part 
acquires inertia, the pitch falls (§ 88). 

In the same way a small continuation of a bar beyond a 
clamped end would be without eflFect, as it would acquire no 
motion. No change will ensue if the new end be also clamped ; 
but as the first clamping is relaxed, the pitch falls, in consequence 
of the diminution in the potential energy of a given deformation. 

The case of a ' supported ' end is not quite so simple. Let the 
original end of the rod be A, and let the added piece which is at 
first supposed to have no inertia, be AB. Initially the end A is 
fixed, or held, if we like so to regard it, by a spring of infinite stiflF- 
ness. Suppose that this spring, which has no inertia, is gradually 
relaxed. During this process the motion of the new end B 
diminishes, and at a certain point of relaxation, B comes to rest. 
During this process the pitch falls. J5, being now at rest, may be 
supposed to become fixed, and the abolition of the spring at A 
entails another fall of pitch, to be further increased 2isAB acquires 

186. The case of a rod which is not quite uniform may be 
treated by the general method of § 90. We have in the notation 
there adopted 

ar = I pcj^Ur^dx, Sar = I BpcoUr^dx, 


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whence, Pr being the uncorrected value ofpr, 

Pr -rr Y+ r /(Pu^V^ "TTI 


[If the motion be strictly periodic with respect to x, Ur" is 
proportional to w^, and both quantities vanish at a node. Ac- 
cordingly an irregularity situated at a node of this kind of motion 
has no eflFect upon the period. A similar conclusion will hold good 
approximately for the interior nodes of a bar vibrating with 
numerous subdivisions, even though, as when the terminals are 
clamped or free, the mode of motion be not strictly periodic with 
respect to a?.] 

If the rod be clamped at and free at I, 

^"^ p<oA l^fhBr lufJopay, 

The same formula applies to a doubly free bar. 

The effect of a small load dM is thus given by 

, 5om* f, , u^dM] 
p^ = 1:= — i 1 — 4 — ~iyr 

where M denotes the mass of the whole bar. If the load be at 
the end, its effect is the same as a lengthening of the bar in the 
ratio M : M + dM. (Compare § 167.) 

[In (2) dM is supposed to act by inertia only ; but a similar 
formula may conveniently be employed when an irregularity of 
mass dM depends upon a variation of section, without a change 
of mechanical properties. Since B = gr/c'©, 

S-B/£o = S(/c«a>)/(iC«a>)o; 

so that the effect of a local excrescence is given by 


pVi^ = i + 


lufj 'i 

dx . 


If the thickness in the plane of bending be constant, S/c* = 0, 
and S (f^o>)/(K*(o)Q = Sa)/a)Q, 

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TT. _xi_ [S(odx dM 

and thus ^/i>. = i+4^'i^' (4). 

If, however, the thickness in the plane perpendicular to that of 
bending be constant, and in the plane of bending variable (£7), 

then 8 (tc'w)/(K*<o)o = Brf/yo* = 3 87/70 = 38€d/©o ; 

and in place of (4) 

p^lP^^i^^^—^^ :-(5). 

If a tuning-fork be filed {dM negative) near the stalk (clamped 
end), the pitch is lowered ; and if it be filed near the free end, the 
pitch is raised. Since u^'^^ufy the effects of a given stroke of 
the file are equal and opposite in the circumstances of (4), but in 
the circumstances of (5) the effect at the stalk is three times as 
great as at the firee end.] 

186. The same principle may be applied to estimate the 
correction due to the rotatory inertia of a uniform rod. We have 
only to find what addition to make to the kinetic energy, supposing 
that the bar vibrates according to the same law as would obtain, 
were there no rotatory inertia. 

Let us take, for example, the case of a bar clamped at and 
firee at I, and assume that the vibration is of the type, 


where u is one of the functions investigated in § 179. The kinetic 
energy of the rotation is 

= ^^^^^8in»;>e (2uu' + mu%, 
by (2) §165. 

To this must be added 

^ 'f sin*/>^ I u^ dx, or ^ p* ain^|)< uf ; 

so that the kinetic energy is increased in the ratio 

1 : l+TT 2-4-m— . 

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The altered frequency bears to that calculated without allow- 
ance for rotatory inertia a ratio which is the square root of the 
reciprocal of the preceding. Thus 

p:P=l-i-7r- 2 — + m — J , 


By use of the relations cosh m = ~ sec m, sinh m = cos tTr.tan m, 
we may express u' : u when a? = Z in the form 

^ — 
u "" 

— slnm 


cos^7^+cos??i~ 1 

— cosiVsina' 

if we 

substitute for 

m from 

m = i(2i- 



In the case of the gravest tone, a = *3043, or, in degrees and 
minutes, a = 17*^ 26', whence 


- = •73413, 

2~+m^ = 2-4789. 


;>:P = 1-2-3241 J 


which gives the correction for rotatory inertia in the case of the 
gravest tone. 

When the order of the tone is moderate, a is very small, 

and then 

u' \u = \ sensibly. 


p..P = l-{x^-)— (3), 

shewing that the correction increases in importance with the 
order of the component. 

In all ordinary bars « : Z is very small, and the term depending 
on its square may be neglected without sensible error. 

187. When the rigidity and density of a bar are variable 
from point to point along it, the normal functions cannot in 
general be expressed analytically, but their nature may be investi- 
gated by the methods of Sturm and Liouville explained in § 142, 

If, as in § 162, B denote the variable flexural rigidity at any 

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point of the bar, and pw dx the mass of the element, whose length 
is (2a?, we find as the general differential equation 

^(*£)--i'-« «■ 

the effects of rotatory inertia being omitted. If we assume that 
y (X cos pt, we obtain as the equation to determine the form of the 
normal functions 

U^S)-'^y «- 

in which i^ is limited by the terminal conditions to be one of an 
infinite series of definite quantities Vi^, i/,', y,* 

Let us suppose, for example, that the bar is clamped at both 
ends, so that the terminal values of y and dy/da vanish. The first 
normal function, for which i/* has its lowest value i/i*, has no 
internal root, so that the vibration-curve lies entirely on one side 
of the equilibrium-position. The second normal function has one 
internal root, the third function has two internal roots, and, 
generally, the r^^ function has r — 1 internal roota 

Any two different normal functions are conjugate, that is to 
say, their product will vanish when multiplied by p<odx, and 
integrated over the length of the bar. 

Let us examine the number of roots of a function f(x) of 
the form 

/(«) = <^mt^m(a?) + <^m+iWm+i(a?)+...+<^nt«n(^) (3), 

compounded of a finite number of normal functions, of which the 
function of lowest order is Umi^) and that of highest order is 
Ujt, (x). If the number of internal roots oif{x) be /i, so that there 
are /li -I- 4 roots in all, the derived function f (x) cannot have less 
than fjL-\-l internal roots besides two roots at the extremities, and 
the second derived function cannot have less than fi + 2 roots. 
No roots can be lost when the latter function is multiplied by B, 
and another double differentiation with respect to x will leave at 
least /i internal roots. Hence by (2) and (3) we conclude that 

has at least as many roots as f{x). Since (4) is a function of the 
same form as f{x)y the same argument may be repeated, and a 
series of functions obtained, every member of which has at least 

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as many roots as f{x) has. When the operatibn by which (4) was 
derived from (3) has been repeated sufficiently often, a function is 
arrived at whose form differs as little as we please from that of the 
component normal function of highest order Un{x)\ and we con- 
clude that f{x) cannot have more than n — 1 internal roots. In 
like manner we may prove that f{x) cannot have less than m — 1 
internal roots. 

The application of this theorem to demonstrate the possibility 
of expanding an arbitrary function in an infinite series of normal 
functions would proceed exactly as in § 142. 

[An analytical investigation of certain cases where the section 
of a rod is supposed to be variable, will be found in a memoir by 

188. When the bar, whose lateral vibrations are to be con- 
sidered, is subject to longitudinal tension, the potential energj' of 
any configuration is composed of two parts, the first depending on 
the stiffness by which the bending is directly opposed, and the 
second on the reaction against the extension, which is a necessary 
accompaniment of the bending, when the ends axe nodes. The 
second part is similar to the potential energy of a deflected string ; 
the first is of the same nature as that with which we have been 
occupied hitherto in this Chapter, though it is not entirely 
independent of the permanent tension. 

Consider the extension of a filament of the bar of section dm, 
whose distance from the axis projected on the plane of vibration 
is 17. Since the sections, which were normal to the axis originally, 
remain normal during the bending, the length of the filament 
bears to the corresponding element of the axis the ratio -R + 17 : iJ, 
jR being the radius of curvature. Now the axis itself is extended 
in the ratio j : ? + T^ reckoning from the unstretched state, if 
Tto denote the whole tension to which the bar is subjected. 
Hence the actual tension on the filament is {r+i7(r+gr)/jB}c?o), 
from which we find for the moment of the couple acting across the 

1 Berlin Monataber.y 1879 ; Collected Works, p. 339. See also Todhanter and 
Pearson's HUtory of the Theory of EUutieity, Vol. 11., Part ii., § 1802. 

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and for the whole potential energy due to stiffness 

i(j+T)«»a,/(gy(ir (1), 

an expression differing from that previously used (§ 162) by the 
substitution of (q + T) for q. 

Since q is the tension required to stretch a bar of unit area to 
twice its natural length, it is evident that in most practical cases 
T woald be negligible in comparison with q. 

The expression (1) denotes the work that would be gained 
during the straightening of the bar, if the length of each element 
of the axis were preserved constant during the process. But 
when a stretched bar or string is allowed to pass from a displaced 
to the natural position, the length of the axis is decreased. The 
amount of the decrease is iJidy/dxydx, and the corresponding 
gain of work is 


F=i(?+r)«-«/(g)'d.H-i2'«/(|)'i^ (2). 

The variation of the first part due to a hypothetical displace- 
ment is given in § 162. For the second part, we have 

i«/(l)''^-/lf^-llM-/S*^ <'>• 

In all the cases that we have to consider, ^ vanishes at the 
limits. The general differential equation is accordingly 

or, if we put g + 7= 6*p, T = a'p, 

*V dor* dx^dt'l "^ dx'^ dt'^ ^*^" 

For a more detailed investigation of this equation the reader is 
referred to the writings of Clebsch^ and Donkin. 

189. If the ends of the rod, or wire, be clamped, dyjdx = 0, and 
the terminal conditions are satisfied. If the nature of the support 
be such that, while the extremity is constrained to be a node, there 

^ Theorie der EloMticitHt fe$ter Kdrper, Leipzig, 1862. 

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is DO couple acting on the bar, dhfjda? must vanish, that ia to say, 
the end must be straight. This supposition is usually taken to 
represent the case of a string stretched over bridges, as in manj 
musical instruments ; but it is evident that the part beyond the 
bridge must partake of the vibration, and that therefore its length 
cannot be altogether a matter of indifference. 

If in the general differential equation we take y proportional 
to cos nt, we get 

'•('■S--S)-S-"V-« ox 

which is evidently satisfied by 

y = 8ini , cosn^ (2), 

if n be suitably determined. The same solution also makes 
y and /' vanish at the extremities. By substitution we obtain 
for 71, 

'^ - P P + i>7r»ic^ ^^^ 

which determines the frequency. 

If we suppose the wire infinitely thin, n* = i*7r*a'-4- P, the same 
as was found in Chapter VL, by starting from the supposition of 
perfect flexibility. If we treat /e : Z as a very small quantity, the 
approximate value of n is 


For a wire of circular section of radius r, «• = J r*, and if we 
replace b and o by their values in terms of q, T, and p. 

7{>-rpf} <*)■ 

which gives the correction for rigidity ^ Since the expression 
within brackets involves i, it appears that the harmonic relation 
of the component tones is disturbed by the stiffness. 

190. The investigation of the correction for stiffness when the 
ends of the wire are clamped is not so simple, in consequence of 
the change of tjrpe which occurs near the enda In order to pass 
from the case of the preceding section to that now under con- 

^ Donkin's Acoustics, Art. 184. 

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sideration an additional constraint must be introduced, with the 
effect of still further raising the pitch. The following is, in the 
main, the investigation of Seebeck and Donkin. 

If the rotatory inertia be neglected, the differential equation 



' ^-&)^=»- 

where D stands for -5- 

In the equation 


one of the values of L* must be positive, and the other negative. 
We may therefore take 

-0*-^^-iS = (^-«')(i>' + /3') 


and for the complete integral of (1) 

y = A cosh ax + 3 sinh ouc + (7 cos ^a? + i) sin jSx (3), 

where a and fi are functions of n determined by (2). 

The solution must now be made to satisfy the four boundary 
conditions, which, as there are only three disposable ratios, lead 
to an equation connecting a, /3, L This may be put into the form 

sinhoZ sin/32 


= 0. 

1 - cosh al cosfil 0^ — ^ 
The value of -r-^^ , determined by (2), is — r— , so that 


sinh al smfil 2nbK _ ^ 

1 — cosh al cos fil 
From (2) we find also that 







Thus far our equations are rigorous, or rather as rigorous as 
the differential equation on which they are founded ; but we shall 
now introduce the supposition that the vibration considered is but 

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slightly affected by the existence of rigidity. This being the case, 
the approximate expression for y is 

. iirx fi'rr ^\ 
y = sm -T- cos I y a^ J , 

and therefore 

/B^tTr/l, n^iirajl (7). 


The introduction of these values into the second of equations 
(6) proves that n*6'/r*/a* or h^t^ja^J} is a small quantity under the 
circumstances contemplated, and therefore that aH^ is a large 
quantity. Since cosh aZ, sinhof are both large, equation (5) re- 
duces to 

, 2n6/e 
tani8Z= ^, , 

or, on substitution of the approximate value for fi derived fiom 


nl ^ nbK 

tan — = 2 
a 0/ 

2 ' 

The approximate value of nlja is iir. If we take idja^vir-^B, 
we get 

tan(iV-htf) = tantf=tf=.2^f = 2tV^p 

so that n = t 

. "wa /, c^b ic^ 


{'<t) <'^ 

According to this equation the component tones are all raised 
in pitch by the same small interval, and therefore the harmonic 
relation is not disturbed by the rigidity. It would probably be 
otherwise if terms involving i^ : Z* were retained ; it does not there- 
fore follow that the harmonic relation is better preserved in spite 
of rigidity when the ends are clamped than when they are free, 
but only that there is no additional disturbance in the former 
case, though the absolute alteration of pitch is much greater. It 
should be remarked that 6 : a or V(? + T) : ^T, is a large quantity, 
and that, if our result is to be correct, k : I must be small enou^ 
to bear multiplication by 6 : a and yet remain small. 

The theoretical result embodied in (8) has been compared with 
experiment by Seebeck, who found a satisfactory agreement. The 
constant of stifihess was deduced from observations of the rapiditj 

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of the vibratioDS of a small piece of the wire, when one end was 
clamped in a vice. 

[As the result of a second approximation Seebeck gives 
(foe. cit.) 

„. = ^.|l+4*^ + (12 + ».^)^j (9)]. 

191. It has been shewn in this chapter that the theory of bars, 
even when simplified to the utmost by the omission of unimportant 
quantities, is decidedly more complicated than that of perfectly 
flexible strings. The reason of the extreme simplicity of the 
vibrations of strings is to be found in the fact that waves of the 
harmonic type are propagated with a velocity independent of the 
wave length, so that an arbitrary wave is allowed to travel without 
decomposition. But when we pass from strings to bars, the con- 
stant in the differential equation, viz. cPy/rft* + ie*6'd*y/(ic* = 0, is 
no longer expressible as a velocity, and therefore the velocity of 
transmission of a train of harmonic waves cannot depend on the 
differential equation alone, but must vary with the wave length. 
Indeed, if it be admitted that the train of harmonic waves can 
be propagated at all, this consideration is sufficient by itself to 
prove that the velocity must vary inversely as the wave length. 
The same thing may be seen from the solution applicable to 

waves propagated in one direction, viz. y=^co8---(Vt — x), which 

satisfies the differential equation if 

v=^^ (1). 


Let us suppose that there are two trains of waves of equal 
amplitudes, but of different wave lengths, travelling in the same 
direction. Thus 

= 2co8 7r 



If t' — T, X' — X be small, we have a train of waves, whose 
amplitude slowly varies from one point to another between the 
values and 2, forming a series of groups separated from one 
another by regions comparatively free fix)m disturbance. In the 
case of a string or of a column of air, X varies as r, and then the 

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groups move forward with the same velocity as the component trains 
and there is no change of type. It is otherwise when, as in the cas€ 
of a bar vibrating transversely, the velocity of propagation is a 
function of the wave length. The position at time t of the middle 
of the group which was initially at the origin is given by 

which shews that the velocity of the group is 

If we suppose that the velocity F of a train of waves varies as 
X**, we find 

d(l/X) d(l/X) ^ ^ 


In the present case n = — 1, and accordingly the velocity of the 
groups is tvnce that of the component waves^ 

192. On account of the dependence of the velocity of propaga- 
tion on the wave length, the condition of an infinite bar at any 
time subsequent to an initial disturbance confined to a limited 
portion., will have none of the simplicity which characterises the 
corresponding problem for a string; but nevertheless Fourier's 
investigation of this problem may properly find a place here. 

It is required to determine a function of a? and <, so as to 

d*V d*y ^ „v 

and make initially y = (f> {x\ y = '^ {x). 
A solution of (1) is 

y=^QOHqH cosg(ir — o) (2), 

where q and a are constants, from which we conclude that 

y = j da F(a) I dq cos g^t cos q(x — a) 

^ In the oorresponding problem for waves on the Burfftce of deep water, the 
Telocity of propagation varies directly as the square root of the wave length, bo 
that n s } . The velocity of a group of such waves is therefore one half of that of 
the component trains. [See note on Progressive Waves, appended to this volume.] 

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192.] Fourier's solution. 303 

is also a solution, where F(a) is an arbitrary function of a. If 
now we put ^ = 0, 

r+oo r+flo 

yo = I daF(a) I dq cos j (a? — a), 

which shews that ^(a) must be taken to be 5- ^ (a), for then by 

Fourier's double integral theorem yo = ^(^). Moreover, y = 0; 

I r+flo r+ao 
y = ^ daif>(a)j dqcoaqH cosg(a?-a) (3) 

satisfies the differential equation, and makes initially 

y = <l>(x), y = 0. 

By Stokes' theorem (§ 95), or independently, we may now 
supply the remaining part of the solution, which has to satisfy the 
differential equation while it makes initially y = 0, y = -i/r (a?) ; it is 

I r+ao /•+» I 

y = g;-\ daylr(a)j dq-ain^t 0035(0? — a) (4). 

ZirJ __oo ,' _ao q^ 

The final result is obtained by adding the right-hand members 
of (3) and (4). 

In (3) the integration with respect to q may be effected by 
means of the formula 

j^^dqcosqHcosqz^A^^ sin^J + |^) (5), 

which may be proved as follows. If in the well-known integral 

we put a? -h 6 for x, we get 



Now suppose that a* = i = e^', where i = V (- 1), and retain 
only the real part of the equation. Thus 


I COS (x' -f 26a?) dx = */7r sin (6» + i tt), 

.' —00 

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/+• _ 

cos aj» cos 26a: dx^Jir sin (6* + \ir\ 

from which (5) follows by a simple change of variable. Thus 
equation (3) may be written 

.^ a — a? 

y^j^j *ti/i'(co8/i« + 8in/i«)^(« + 2/*V0 (6)- 

192 a. If the axis of the rod be curved instead of straight, 
we obtain problems which may be regarded as extensions of. 
those of the present and of the last chapters. The most impor- 
tant case under this head is that of a circular ring, whose section 
we will regard as also circular, and of radius (c) small in 
comparison with the radius (a) of the circular axis. 

The investigation of the flexural modes of vibration, executed 
in the plane of the ring, is analogous to the case of a cylinder 
(see § 233), and was first effected by Hopped If « be the number 
of periods in the circumference, the coeflScient p of the time in 
the expression for the vibrations is given by 

^4 !-!-«> pa' ^^^' 

where q is Young's modulus and p the density of the material. 
This may be compared with equation (9) § 233. To fisill back 
upon the case of a straight axis we have only to suppose 
8 and a to be infinite in such a manner that 27ra/« is equal to the 
proposed linear period. The vibrations in question are then purely 

In the class of vibrations considered above the circular axis 
remains unextended, and (§ 232) the periods are comparatively 
long. For the other class of vibrations in the plane of the ring, 
Hoppe found 

p'-(^^^^l^* (2> 

1 CrdU, Bd. 68, p. IfiS, 1871. 

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192 a.] CIRCULAR RINGS. 305 

The frequencies are here independent of c, and the vibrations 
are analogous to the longitudinal vibrations of straight rods. 

If « = in (2), we have the solution for vibrations which are 
purely radial. 

For flezural vibrations perpendicular to the plane of the 
riag, the result^ corresponding to (1) is 

i ^(^-iy gg (3) 

the difference consisting only in the occurrence of Poisson's ratio 
(jjt) in the denominator. 

Our limits will not allow of our dwelling further upon the 
problem of this section. A complete investigation will be found 
in Love's Treatise on Elasticity, Chapter XYiii. The effect of 
a small curvature upon the lateral vibrations of a limited bar 
has been especially considered by Lamb*. 

1 Miohell, Menenger of Mathenuitiei, zix., 1889. 
* Proe. Lond. McUh. Soe., xn., p. 365, 1888. 


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193. The theoretical membrane is a perfectly flexible and 
infinitely thin lamina of solid matter, of uniform material and 
thickness, which is stretched in all directions by a tension so great 
as to remain sensibly unaltered during the vibrations and displace- 
ments contemplated. If an imaginary line be drawn across the 
membrane in any direction, the mutual action between the two 
portions separated by an element of the line is proportional to the 
length of the element and perpendicular to its direction. If the 
force in question be T^ ds, Ti may be called the tension of the memr 
hrune; it is a quantity of one dimension in mass and — 2 in time. 

The principal problem in connection with this subject is the 
investigation of the transverse vibrations of membranes of different 
shapes, whose boundaries are fixed. Other questions indeed may 
be proposed, but they are of comparatively little interest ; and, 
moreover, the methods proper for solving them will be suflBciently 
illustrated in other parts of this work. We may therefore proceed 
at once to the consideration of a membrane stretched over the 
area included within a fixed, closed, plane boundary. 

194. Taking the plane of the boundary as that of xy^ let fo 
denote the small displacement therefrom of any point P of the 
membrane. Round P take a small area 8^ and consider the forces 
acting upon it parallel to z. The resolved part of the tension is 
expressed by 


where da denotes an element of the boundary of £•, and dn an 
element of the normal to the curve drawn outwards. This is 
balanced by the reaction against acceleration measured by pSw, 

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p being a symbol of one dimension in mass and —2 in length 
denoting the superficial density. Now by Green's theorem, if 

j^ds^jjV'wdS^VHu.S ultimately, 
and thus the equation of motion is 

dt^^ p\di^^ dy'J ^^^• 

The condition to be satisfied at the boundary is of course w = 0. 

The differential equation may also be investigated from the 
expression for the potential energy, which is found by multiplying 
the tension by the superficial stretching. The altered area is 

and thus 

''-i^-//((sr-(l)'}«' <^^ 

firom which SF is easily found by an integration by parts. 

If we write Ti -r /> = c*, then c is of the nature of a velocity, and 
the differential equation is 

dt^-'^Vdx^^d^^) ^^^• 

196. We shall now suppose that the boundary of the mem- 
brane is the rectangle formed by the coordinate axes and the lines 
ar = a, y = 6. For every point within the area (3) § 194 is satisfied, 
and for every point on the boundary w = 0. 

A particular integral is evidently 

w = sin sm— T^cosp^ (1), 

where p. = c»^g + »;) (2), 

and m and n are integers; and from this the general solution may 
be derived. Thus 

w=^z S sm-^— sm -r^ {^tiin cosp^ -h £,»n smpq (3). 


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That this result is really general may be proved a posteriori, 
by shewing that it may be adapted to express arbitrary initial 

Whatever function of the co-ordinates w may be, it can be ex- 
pressed for all values of x between the limits and a by the series 

y^sm — -h Fjsm- — + , 

a a 

where the coefficients Fi, F,, &c. are independent of x. Again 
whatever function of y any one of the coefficients F may be, it can 
be expanded between and h in the series 

C,sin7+C.sin^-^ + , 

where G^ &c. are constants. From this we conclude that any 
function of x and y can be expressed within the limits of the rect- 
angle by the double series 

m-flo n-oo ^^^ ^„ 

m-l n-1 d 


and therefore that the expression for w in (3) can be adapted to 
arbitrary initial values of w and w. In fEtct 

The character of the normal functions of a given rectangle, 

sm sm— r^ , 

a b 

as depending on m and n, is easily understood. If m and n be both 
unity, w retains the same sign over the whole of the rectangle, 
vanishing at the edge only; but in any other case there are 
nodal lines running parallel to the axes of coordinates. The 
number of the nodal lines parallel to a; ifi n — 1, their equations 

h 26 (n-1) 6 

y^:^^ 1^^ — - 

n n n 

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In the same way the equations of the nodal lines parallel to y 


_a 2a (m — l)a 

X—— y , f 

mm m 

being m — 1 in number. The nodal system divides the rectangle 
into mn equal parts, in each of which the numerical value of tc; is 

196. The expression for w in terms of the normal functions 

t(; = 22<^^n8in^^sin^^^- (1), 

where if>nm &c. are the normal coordinates. We proceed to form 
the expression for V in terms of ^«n. We have 

In integrating these expressions over the area of the rectangle 
the products of the normal coordinates disappear, and we find 


-f't'^e'^S*-' <2)' 

the summation being extended to all integral values of m and n. 

The expression for the kinetic energy is proved in the same 
way to be 

r=|^42^» (3). 

firbm which we deduce as the normal equation of motion 

In this equation ^ 

^mn = j ] Z sm -^ am -^dxdy (d), 

ii Zdxdy denote the transverse force acting on the element dxdy. 

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Let us suppose that the initial condition is one of rest under 
the operation of a constant force Z^ such as may be supposed to 
arise firom gaseous pressure. At the time ^ = 0, the impressed 
force is removed, and the membnCM left to itself Initially the 
equation of equilibrium is 

<^'^(S+3<^>'=^*^»» ^^ 

■whence (<^mn)o is to be found. The position of the system at time \ 
is then given by 

</>mn = (<Atnn)oCOsfy' — H-^.Clrtj (7), 

in conjunction with (1). 

In order to express *m»> we have merely to substitute for Z its 
value in (5), or in this case simply to remove Z fix)m under the 
integral sign. Thus 

, -r*f* . mirx . ntry J , 

= Z r (1 — COS imf) (1 — COS nir\ 

We conclude that *„»» vanishes, unless m and n are hoih odd, and 
that then 

Accordingly, m and n being both odd, 

16Z COSJO^ ,J^^ 

^^^^ ii-p^n^ ^^^' 

where p.= c»7r«(^ + g) (9). 

This is an example of (8), § 101. 

If the membrane, previously at rest in its position of equili- 
brium, be set in motion by a blow applied at the point (a, /3), the 
solution is 

^mn = ^ sm-^ 8m--^jJM;oCtody.smpe...(10> 

[As an example of forced vibrations, suppose that a harmonic 
foree acts at the centre. Unless m and n are both odd, <I>iiiji-0> 
aud in the case reserved 

^mn =±^1 cos 3« (11), 

Digitized by VjOOQ IC 

«t»m»= .Z. 


where Z^ is the whole force acting at time t, and ± represents 
sin^mTT sin JnTT. From (4) and (9) we have 

and w is then given by (1). 

In the case of a square membrane, j> is a symmetrical function 
of m and n. When m and n are unequal, the terms occur in pairs, 
such as 

±iZiCORqt f. m'rrx . rwrv . ri'rrx . miry] ,,-.v 
~r7 r-75\ ^^^ ^ sm - ^ + sm sm — ^k..(13), 

-&' combination symmetrical as between x and y. The vibration is 
of course similarly related as well to the four sides as to the four 
corners of the square. 

In the neighbourhood of the centre, where the force is applied, 
the series loses its convergency, and the displacement w tends to 
become (logarithmically) infinite.] 

197. The frequency of the natural vibrations is found by 
ascribing different integral values to m and n in the expression 


c Im^ n^ .^. 

For a given mode of vibration the pitch falls when either 
side of the rectangle is increased. In the case of the gravest 
mode, when m = l, n = l, additions to the shorter side are the 
more effective; and when the form is very elongated, additions 
to the longer side are almost without effect. 

When a? and 6* are incommensurable, no two pairs of values 
of m and n can give the same frequency, and each fundamental 
mode of vibration has its own characteristic period. But when 
a' and b' are commensurable, two or more fundamental modes 
may have the same periodic time, and may then coexist in any 
proportions, while the motion still retains its simple harmonic 
character. In such cases the specification of the period does 
not completely determine the type. The full consideration of 
the problem now presenting itself requires the aid of the theory 
of numbers; but it will be suflScient for the purposes of this 
work to consider a few of the simpler cases, which arise when 
the membrane is square. The reader will find fuller information 
in Riemann's lectures on partial differential equations. 

Digitized by 




Ifa = 6. 

VI /• , 

^ - /«i»-l-«« 

2ir-2a'^"' +" 



The lowest tone is found by patting m and n equal to unity, 
which gives only one fundamental mode : — 

w — sin — sm -^cosp^ (3). 

Next suppose that one of the numbers m,ni8 equal to 2, and 
the other to unity. In this way two distinct types of vibration 
are obtained, whose periods are the same. If the two vibrations 
be synchronous in phase, the whole motion is expressed by 


(^ . 2irx . 'try ^ J. . trx . 27ry) ^ ,^. 

\ a a a a ] ^ ^ '^ 

so that, although every part vibrates Sjmchronously with a 
harmonic motion, the type of vibration is to some extent arbitrary. 
Four particular cases may be especially noted First, if D = 0, 

sm sm-^cosp^ (5), 

which indicates a vibration with one node along the line x = \(k 
Similarly if (7 "= 0, we have a node parallel to the other pair of 
edges. Next, however, suppose that C and D are finite and 
equal Then w is proportional to 

. ^irx .Try . tto? . 27ry 

sm sm -^ 4- sm — sm — - , 

a a a a 

which may be put into the form 

g. . TTX . iry / irx ^ iry\ 

2 sm — sm -^ cos h cos -^ . 

a a \ a a] 

This expression vanishes, when 

sin irx\a = 0, or sin iry\a = 
or again, when 

cos irx\a + cos Try/a = 0. 

The first two equations give the edges, which were originally 
assumed to be nodal ; while the third gives y + a; = a, representing 
one diagonal of the square. 

In the fourth case, when (7 = — D, we obtain for the nodal 
lines, the edges of the square together with the diagonal y^^ 
The figures represent the four cases. 

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Fig. 82. 

2) = 0. C = 0. C~D«0. a + i) = o. 

[Frequency (referred to gravest) = 1'68.] 

For other relative values of C and D the interior nodal line 
is curved, but is always analytically expressed by 

Ccos— +Dcos^ = (6), 

a a 

and may be easily constructed with the help of a table of logarith- 
mic cosines. 

The next case in order of pitch occurs when m = 2, w « 2. 
The values of m and n being equal, no alteration is caused by 
their interchange, while no other pair of values gives the same 
frequency of vibration. The only type to be considered is 

. 2irx . 27rv 
w = sm sm — - cos 1)^, 

whose nodes, determined by the equation 

Fig. 88. 

. ttiju . Try TTu, tru -. 

sm — sm -^ cos — cos -^ = 0, 
a a a a 

are (in addition to the edges) the straight lines 
Fig. (33) 

x — ^a y=ia. 

[Frequency = 2*00.] 

The next case which we shall consider is obtained by ascribing 
to m, » the values 3, 1, and 1, 3 successively. We have 

(^ . ^irx . Try ^ r\ - itx , 37ry) 

w = -^1/ sm sin — ^ + i/sm — sm — - \ cos »^. 

\ a a a a } ^ 

The nodes are given by 
sin^sin ^{c(4co3«^- l) + i)(4coe»^- l)Uo, 
or, if we reject the fint two ftrCtors, which correspond to the edges. 

(7(4co8»^'^-l) + i)(4co8»^-l) = (7). 


Digitized by ' 




If (7 = 0, we have . y^^ia, y=»|a. 
If2) = 0, a? = ia, a? = Ja. 

irx try 

cos — == ± cos — ^ , 
a a 

If (7 = -D, 

whence, y = a?, y^a-^x, 

which represent the two diagonals. 

Lastly, i{ C=D, the equation of the node is 

^trx , ,7ry , 

cos* h cos* -^ = i, 

a a " 


., . 27ra: . 27ry 

1 + cos h cos — ^ s 

a a 

Fig. 84. 

Z) = 0. 0+D = 0. 


[Frequency = 2-24.] 

In case (4) when a: = ^a, y = Ja, or fa; and similarly when 
y = ^a, a? = Ja?, or fa. Thus one half of each of the lines joining 
the middle points of opposite edges is intercepted by the curve. 

[The diameters of the nodal curve parallel to the sides of the 
square are thus equal to ^a. Those measured along the diagonab 
are sensibly smaller, equal to ^\/2 . a, or '471 a.] 

It should be noticed that in whatever ratio to one another 
G and D may be taken, the nodal curve always passes through 
the four points of intersection of the nodal lines of the first two 
cases, (7=0, 2) = 0. If the vibrations of these 
cases be compounded with corresponding phases, 
it is evident that in the shaded compartments of 
Fig. (35) the directions of displacement are the 
same, and that therefore no part of the nodal curve 
is to be found there ; whatever the ratio of ampli- 
tudes, the curve must be drawn through the un- 
shaded portions. When on the other hand the phases are opposed, 
the nodal curve will pass exclusively through the shaded portions. 

Fig. 95. 


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When m = 8, n = 3, the nodes are the straight lines parallel 
to the edges shewn in Fig. (36). 

The last case [Frequency = 2'56] which we 
shall consider is obtained by putting 

m==S, n=:2, or m = 2, n = 3. 

The nodal system is 

[Frequency = 3*00.] 

Cam sm — ^-^JJsm — -sin - =0, 

a a n a 

or, if the fiu;tors corresponding to the edges be rejected, 

c(4cos«^~l)cos^ + Dcos^(4co8«^-l) = (9). 

If C or i) vanish, we fall back on the nodal systems of the 
component vibrations, consisting of straight lines parallel to the 
edges. If C = J5, our equation may be written 

fcos^ + cos^)f4cos^cos^~l) = (10), 

of which the first factor represents the diagonal y + ^ = a, and 
the second a hyperbolic curve. 

If (7= — i), we obtain the same figure relatively to the other 

198. The pitch of the natural modes of a square membrane, 
which is nearly, but not quite uniform, may be investigated by 
the general method of § 90. 

We will suppose in the first place that m and n are equal. 
In this case, when the pitch of a uniform membrane is given, 
the mode of its vibration is completely determined. If we now 
conceive a variation of density to ensue, the natural type of 
vibration is in general modified, but the period may be calculated 
approximately without allowance for the change of t}rpe. 

We have 

= i ^m» |p. \ + jjSp sin' ^ 8in» ^ dxdy^ , 

I lami, Letont iwr ViUutieitf, p. 129. 

Digitized by VjOOQIC 



of which the second term is the increment of T due to ip. Hence 
if w X Qospty and P denote the value of p previously to variation, 
we have 

i>™„':P^»=l-y"r^8in.^siB«^yd.dy (1). 

where Pmm^^ — ^ , and c»= Tj -^ po. 

For example, if there be a small load M attached to the middle of 
the square, 

4tAf nr 

lW':P«.m'=l-* sin'mj (2), ; 

CL pQ ^ 

in which sin* ^tt vanishes, if m be even, and is equal to unity, if 
m be odd. In the former case the centre is on the nodal line of 
the unloaded membrane, and thus the addition of the load produces 
no result. 

When, however, m and n are unequal, the problem, though re- 
maining subject to the same general principles, presents a pecu- 
liarity diflFerent from anything we have hitherto met with. The 
natural type for the unloaded membrane corresponding to a speci- 
fied period is now to some exteut arbitrary ; but the introduction 
of the load will in general remove the indeterminate element. In 
attempting to calculate the period on the assumption of the undis- 
turbed tj^, the question will arise how the selection of the undis- 
turbed tj^ is to be made, seeing that there are an indefinite 
number, which in the uniform condition of the membrane give 
identical periods. The answer is that those types must be chosen 
which differ infinitely little from the actual types assumed under 
the operation of the load, and such a type will be known by the 
criterion of its making the period calculated from it a maximum 
or minimum. 

As a simple example, let us suppose that a small load M is 
attached to the membrane at a point lying on the line x^^^a, and 
that we wish to know what periods are to be substituted for the 
two equal periods of the unloaded membrane, found by making 

m = 2, n.= l, or m = l, n = 2. 

It is clear that the normal types to be chosen, are those whose 
nodes are represented in the first two cases of Fig. (32). In the 
first case the increase in the period due to the load is zero, which 
is the least that it can be; and in the second case the increase 

Digitized by 



is the greatest possible. If /3 be the ordinate of if, the kinetic 
energy is altered in the ratio 

2 4^f4 + 2«"^'^' 

and thus p^^ : P^«= l~^f sin*--^ (3) 

while l>ii' = Pii' = Pi,». 

The ratio characteristic of the interval between the two natural 

tones of the loaded membrane is thus approximately 

1+ - sm»-- (4). 

a^p a 

I( /3 = ^a, neither period is affected by the load. 

As another example, the case where the values of m and n 
are 3 and 1, considered in § 197, may be referred to. With a load 
in the middle, the two normal types to be selected are those 
corresponding to the last two cases of Fig. (34), in the former 
of which the load has no effect on the period. 

The problem of determining the vibration of a square mem- 
brane which carries a relatively heavy load is more difficult, and 
we shall not attempt its solution. But it may be worth while to 
recall to memory the £su;t that the actual period is greater than 
any that can be calculated from a hypothetical type, which differs 
from the actual one. 

199. The preceding theory of square membranes includes a 
good deal more than was at first intended. Whenever in a vibrat- 
ing system certain parts remain at rest, they may be supposed to 
be absolutely fixed, and we thus obtain solutions of other questions 
than those originally proposed. For example, in the present case, 
wherever a diagonal of the square is nodal, we obtain a solution 
applicable to a membrane whose fixed boundary is an isosceles 
right-angled triangle. Moreover, any mode of vibration possible to 
the triangle corresponds to some natural mode of the square, as 
may be seen by supposing two triangles put together, the vibra- 
tions being equal and opposite at points which are the images of 
each other in the common hypothenuse. Under these circum- 
stances it is evident that the hjrpothenuse would remain at rest 
without constraint, and therefore the vibration in question is in- 
cluded among those of which a complete square is capable. 

Digitized by 




The frequency of the gravest tone of the triangle is found by 
putting m s: 1, n =s 2 in the formula 

£ = Av(^.+„.) (1^ 

and is therefore equal to C'Jojia. 

The next tone occurs, when m = 3, n = 1. In this case 

JL^^lJ^ (2) 

as might also be seen by noticing that the triangle divides itself 
into two, Fig. (37), whose sides are less 
than those of the whole triangle in the ^' ^'^' 

ratio V2 : 1. 

For the theory of the vibrations of 
a membrane whose boundary is in the 
form of an equilateral triangle, the 
reader is referred to Lamp's Lefons 

8ur r^ldsticitd. It is proved that the frequency of the gravest 
J L tone is c-r-h, where h is the height of the triangle, which is the 

same as the frequency of the gravest tone of a square whose 
diagonal is h. 

200. When the fixed boundary of the membrane is circular, 
the first step towards a solution of the problem is the expression 
of the general differential equation in polar co-ordinates. This 
may be effected analytically ; but it is simpler to form the polar 
equation de novo by considering the forces which act on the polar 
element of area rdO dr. As in § 194 the force of restitution acting 
on a small area of the membrane is 


!'w _ (d^w Idw 1 d^w \ . 

i¥~^\dr^~'^rd^'^f^dS^] ^^^• 

and thus, if TJp = c* as before, the equation of motion is 
d^w . {d^w 

The subsidiary condition to be satisfied at the boundary is that 
t(; = 0, when r=^a. 

In order to investigate the normal component vibrations we 
have now to assume that w \& b, harmonic function of the tima 


Digitized by 



Thua, if w oc oob (2>^ — c), and for the sake of brevity we write 
pjc ss k, the differential equation appears in the form 

cPw Idw 1 d^w . , - ^ ,-,v 

dr- + rd7 + r«rf^ + *'«'-^ <2). 

in which k is the reciprocal of a linear quantity. 

Now whatever may be the nature of to as a function of r and 0, 
it can be expanded in Fourier's series 

w = W9 + WiCO8{0-hai) + w, cos 2 (tf + Oj) + (3), 

in which Wo, «^, &c. are functions of r, but not of 0. The result 
of substituting from (3) in (2) may be written 

the sunmiation extending to all integral values of n. If we 
multiply this equation by cos n (^ + On), and integrate with respect 
to between the limits and iir, we see that each term must 
vanish separately, and we thus obtain to determine Wn SiS sl 
function of r 

d^Wn . Idwn 

■*lt-H''-%h.-o W. 

dr» r dr \ 

in which it is a matter of indifference whether the factor 
cos h (^ + On) be supposed to be included in Wn or not. 

The solution of (4) involves two distinct functions of r, 
each multiplied by an arbitrary constant. But one of these 
functions becomes infinite when r vanishes, and the corresponding 
particular solution must be excluded as not satisfying the pre- 
scribed conditions at the origin of co-ordinate& This point may 
be illustrated by a reference to the simpler equation derived from 
(4) by making k and n vanish, when the solution in question 
reduces to w — logr, which, however, does not at the origin 
satisfy V*w =s 0, as may be seen from the value of f(dw/dn) ds, inte- 
grated round a small circle with the origin for centre. In like 
manner the complete integral of (4) is too general for our 
present purpose, since it covers the case in which the centre of 
the membrane is subjected to an external force. 

The other function of r, which satisfies (4), is the Bessel's 
function of the rfi^ order, denoted by J^ (kr), and may be expressed 
in several ways. The ascending series (obtained immediately 
from the differential equation) is 

Digitized by 





2 . 4 . 2n + 2 . 2n + 4 

2 . 4.6 . 2n + 2 . 2n + 4 . 2w + 6 "*■ 

«^»(*) = 2»r(n + l)r~2.2n + 2'''; 

..} (5X 

from which the following relations between functions of conseca 

tive orders may readily be deduced : 

/,'(*) J,{z) (6), 

2/„'(*) = J^,(«)-J„+.(z) (7). 


— /„(*) = J"^, (*) + /„+,(«) (8). 


When n is an integer, J^ {z) may be expressed by the definiU 

Jn{z) = - I cos (-e: sin fi) — no)) do) (9), 


which is Bessel's original form. From this expression it is evidenl 
that «7n <md its differential coefficients with respect to z are always 
less than unity, 
n M V The ascending series (5), though infinite, is convergent for all 

values of n and z\ but, when z is great, the convergence does not 
begin for a long time, and then the series becomes useless as a 
basis for numerical calculation. In such cases another series 
proceeding by descending powers of z may be substituted with 
advantage. This series is 

-^-(") = V^r- 1.2(8.)> + }^('-4-^2J 

/ 2 [ l«-4n' (l'-4n') (3«-4n') (5«-4n«) ) 

'^y irz\ 1.8^ 1.2.3.(8^)» "^ | 

^^(^"i"^l) .....(10); 

it terminates, if 2n be equal to an odd integer, but otherwise, it 
runs on to infinity, and becomes ultimately divergent. Nevertheless 
when z is great, the convergent part may be employed in calcula- 
tion ; for it can be proved that the sum of any number of terms 
differs from the true value of the function by less than the last 
term included. We shall have occasion later, in connection with 
another problem, to consider the derivation of this descending seriea 
As Bessel's functions are of considerable importance in theo- 
retical acoustics, I have thought it advisable to give a table foi 
the functions Jq and Ji, extracted from Lommers^ work, and due 
1 Loxnmel, Studien Hher die Be$$eV$chen Funetionen. Leipzig, 1868. 

Digitized by 





originally to Hanseu. The functions J© and Jj are connected by 
the relation Jo' = — «A • 

1 » 










00000 1 





1 01 


•0499 , 







' 0-2 


•0995 , 









•1483 ' 























































5 4 



















+ ^0270 




+ •0184 





















•5419 1 












■2767 ' 






•5699 : 












•2329 ; 









•2081 , 






•5812 1 









•5767 1 


















•5560 ' 

















+ •00-25 

•5202 ' 














•0677 • 




•4708 1 



+ •0252 


















•0826 I 


+ •0020 













•3391 , 












•1592 , 


















•2014 ' 



























•2476 , 









•2580 , 






+ -0128 





























+ •0146 

•2728 1 








- 0125 

•2697 I 









•2641 ' 












+ •0166 



Digitized by VjOOQL 


201. In accordaace with the notation for Bessers functions 
the expression for a normal oompouent vibration may therefore be 

w^PJn(kr) co8n(tf + a) co&(pt + €) (1); 

and the boundary condition requires that 

Jn{ka)^0 (2), 

an equation whose roots give the admissible values of k, and 
therefore o{ p. 

The complete expression for w is obtained by combining the 
particular solutions embodied in (1) with all admissible values of 
k and n, and is necessarily geneml enough to cover any initial 
circumstances that may be imagined. We conclude that any 
function of r and may be expanded within the limits of the 
circle r=a in the series 

w = 22 /n(*r){^ cos ntf + ^ sin n^} (3). 

For every integral value of n there are a series of values of k, 
given by (2); and for each of these the constants ^ and '^ are 

The determination of the constants is effected in the usual 
way. Since the energy of the motion is equal to 

J p r rw^rdddr (4), 

and when expressed by means of the normal co-ordinates can only 
involve their squares, it follows that the product of any two of the 
terms in (3) vanishes, when integrated over the area of the circle. 
Thus, if we multiply (3) by Jn{kr) cos nO, and integrate, we 

I / w Jn{kr) cos nOrdrdO 

^(l>jj[Jn(kr)Ycos^n0rdrd0 = <l>.irr[Jn{h')']^rdr (5). 

by which <f> is determined. The corresponding formula for ^Jr is 
obtained by 'writing sin n6 for cos nd, A method of evaluating 
the integral on the right will be given presently. Since tfe and -^ 
each contain two terms, one varying as cos^^ and the other as 
sin pt, it is now evident how the solution may be adapted so as to 
agree with arbitrary initial values of w and w. 

Digitized by 



202. Let us now examine more particularly the character of 
the fundamental vibrations. If n == 0, i«r is a function of r only, 
that is to say, the motion is symmetrical with respect to the centre 
of the membrane. The nodes, if any, are the concentric circles, 
whose equation is 

/o(A?r) = (1). 

When n has an integral value different from zero, wias, func- 
tion of d as well as of r, and the equation of the nodal system 
takes the form 

Jn{kr) cosn(tf--o) = (2). 

The nodal system is thus divisible into two parts, the first con- 
sisting of the concentric circles represented by 

Jn(kr)^0 (3), 

and the second of the diameters 

^ = a + (2m + l)7r/2w (4), 

where m is an integer. These diameters are n in number, and 
are ranged uniformly round the centre; in other respects their 
position is arbitrary. The radii of the circular nodes will be 
investigated further on. 

203. The important integral formula 
Vn(ir) J„(A:V)rdr = (1), 


where k and k' are different roots of 

Jn{ka)^0 (2), 

may be verified analytically by means of the differential equations 
satisfied by J»(fcr), t/«(A:V); but it is both simpler and more 
instructive to begin with the more general problem, where the 
boundary of the membrane is not restricted to be circular. 

The variational equation of motion is 


and therefore 

SV+pjjiuBwdxdy = (8) 

^-i''!l{&<t)h'' <*>■ 

'^-'M'^'f.wi'"' <'>• 


Digitized by VjOOQ IC 


III these equations w refers to the actual motion, and St(; to a hypo 
thetical displacement consistent with the conditions to which th( 
system is subjected. Let us now suppose that the system is exe 
cuting one of its normal component vibrations, so that w=^u, and 

u-hp^u^^O (6), 

while Sw is proportional to another normal function v. 
Since k^p/c, we get from (3) 

i-//«t;da.dy=//jg| + ||}dxdy (7> 

The integral on the right is symmetrical with respect to u and v 
and thus 

{hf^-lc'){\uvdxdy = (8), 

where h'^ bears the same relation to v that 1<^ bears to u. 

Accordingly, if the normal vibrations represented by u and v 
have different periods, 

jjuvdxdy = (9). 

In obtaining this result, we have made no assumption as to the 
boundary conditions beyond what is implied in the absence of re- 
actions against acceleration, which, if they existed, would appear 
in the fundamental equation (3). 

If in (8) we suppose k' = k% the equation is satisfied identically, 

and we cannot infer the value of jju^dxdi/. In order to evaluate 

this integral we must follow a rather diflferent course. 

If u and V be functions satisfying within a certain contour the 
equations V^w + k*u = 0, V^v + k'^v = 0, we have 

(k'-' - k^) jjuvdxdy^^l Hv V^u - u V^v^dxdy 

by Green s theorem. Let us now suppose that v is derived from 
n by slightly varying k, so that 

V = If + -IT SA-, kf =^k-\-ik) 
substituting in (10), we find 

St//..^.y./(S£-.^;U (U); 

Digitized by 



or, if u vanish on the boundary, 

a//..,l.iy-/||* (12). 

For the application to a circular area of radius r, we have 

u ^ C0& nd Jn(kr)) . ^. 

v = cosneJn(kV)] ^^"^^^ 

and thus from (10) on substitution of polar co-ordinates and integra- 
tion with respect to 0, 

(A:'* - k^) rj^ (At) J^ (AV) rdr 

^rJ^{k'r)^~Jn{kr)-rJn(kr)^^^ (^*)- 

Accordingly, if 

^^Jnik'r) : J, (*'r) = ^^Jn{M : J„(ir), 

and k and k' be different, 

fjn(kr)J^(k'r)rdr^O (15). 

an equation first proved by Fourier for the case when 
Jnikr) = Mk'r)='0. 

Again from (11) 

dJdJ , d^r 

1 UK iir iiV dk 

dashes denoting differentiation with respect to kr. Now 

and thus 

2fjn'(kr)rdr = i^J^Hkr) + 7- (l - ^f^^j Jn\kr) (16). 

This result is general ; but if, as in the application to membranes 
with fixed boundaries, /„ (kr) = 0, 

then 2['jn^{kr)rdr^r^J^^(kr) (17). 


Digitized by VjOOQIC 


201. We may use the result just arrived at to simplify the 
expressions for T and F. From 

W = 22 {^«»/n iJCwnr) cos ud + ^^^nJn i^^mnT) siu Tltf j (1), 

we find 

r«ip7ra«22J'„'»(*m«a){<^mn' + ^mn'; (2), 

F » i p7ra« Upmn^Jn'^ {Kna) {^«n' + ^mn'\ (3) ; 

whence is derived the normal equation of motion 

^+i»«„'^„-— .jr-/,'^,^-^) (4). 

and a similar equation for '^mn* The value of 4>mn is to be found 
from the consideration that ^wn^^mn denotes the work done by the 
impressed forces during a hypothetical displacement S^mn ; so that 
if Z be the impressed force, reckoned per unit of area, 

^mn^uZJn{krnnr)co^n0rdrde (5). 

These expressions and equations do not apply to the case n = 0, 
when ^ and '^ are amalgamated. We then have 

r^^pira'p„,o'Jo'{kmoa)il>mo'\ ^ ^' 


As an example, let us suppose that the initial velocities are zero, 
and the initial configuration that assumed under the influence of a 
constant pressured; thus 

^„,o = Z.2tr\ Jo {k„,or) rdr, 

Now by the differential equation, 

rJ, (kr) - - {r Jo'' (kr) + 1 Jo' (^t)}. 
and thus 

Vo(*r)rdr = -^Jo'(Jta) (8); 


80 that 4>^ ^« ZJ,' (k^a). 

Substituting this in (7), we see that the initial value of ^^o is 

— 2Z 


Digitized by 



For values of n other than zero, <t> and the initial value of ^^n 
vanisL The state of the system at time t is expressed by 

<A»n« = (^mo)e-o.COSp^e (10), 

W = 2^,«,Jo(*»nor) (11), 

the summation extending to all the admissible values o( tCm^' 

As an example o{ forced vibrations, we may suppose that Z, still 
constaut with respect to space, varies as a harmonic function of the 
time. This may be taken to represent roughly the circumstances 
of a small membrane set in vibration by a train of aerial waves. 
If Z=cos qt, we find, nearly as before, 

w^ ^cosg^Z , ,,'^^^^''L, , (12). 

The forced vibration is of course independent of 0. It will be seen 
that, while none of the symmetrical normal components are missing, 
their relative importance may vary greatly, especially if there be a 
near approach in value between q and one of the series of quanti- 
ties j[)^. If the approach be very close, the eflfect of dissipative 
forces must be included. 

[Again, suppose that the force is applied locally at the centre. 
By (5) 

4>,^ = ZiCosg^ (13), 

if Zi COS qt denote the whole force at time t From (7) 

^ ^i_??l?i nA\ 

'''"^-p7ra'(l>«o»-3«)^o'MUa) ^'*^' 

and w is then given by (11). The series is convergent, unless 
r = 0. 

But this problem would be more naturally attacked by including 
in the solutions of (4) § 200 the second BesseFs function § 341. 
In this method k—qjc\ and the ratio of constants by which the 
two functions of r are multiplied is determined by the boundary 
condition. When q coincides with one of the values of j», the 
second function disappears from the solution.] 

205. The pitches of the various simple tones and the radii of 
the nodal circles depend on the roots of the equation 

Jn(*a)-c/n(^) = 0. 

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If these (exclusive of zero) taken in order of magnitude b 

called Zn'^^^ Zn^^\ Znf^^ Zn}"^ , then the admissible values of 

are to be found by multiplying the quantities Zn^*^ by c/a. Tb 
particular solution may then be written 

W = Jn [z^^*^ -\ {^n<'> cos 1X0 + B^^*^ siu nO] cos l^^r,,^'^^ -€n <"[...(!). 

The lowest tone of the group n corresponds to ^,/** ; and since i 
this case Jn (-^n"^ rja) does not vanish for any value of r less than c 
there is no interior nodal circle. If we put « = 2, «/„ will vanisl 


that is, when 



which is the radius of the one interior nodal circle. Similarlj 
if we take the root Zn^''\ we obtain a vibration with « — 1 noda 
circles (exclusive of the boundary) whose radii are 


All the roots of the equation J^ {ka) = are real. For, \\ 
possible, let Aa = X + ifi be a root ; then A;'a = X — i^i is also a root 
and thus by (14) § 203, 

4i\/A I Jn {kr) Jn {k'r) rdr = 0. 

Now Jn (kr\ Jn (k'r) are conjugate complex quantities, whos( 
product is necessarily positive ; so that the above equation requires 
that either \ or fi vanish. That \ cannot vanish appears from 
the consideration that if ka were a pure imaginary, each term ol 
the ascending series for Jn would be positive, and therefore the 
sum of the series incapable of vanishing. We conclude thai 
/Lt = 0, or that k is reaP. The same result might be arrived at 
from the consideration that only circular functions of the time 
can enter into the analytical expression for a normal component 

The equation Jn (z) = has no equal roots (except zero). Froii 
equations (7) and (8) § 200 we get 

J'--J -7 

^ RiemaDD, PartielU DiffereniialgUichungen, Brauoschweig, 1869, p. 2C0. 

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205.] ROOTS OF bessel's functions. 329 

whence we see that if «/«, Jn vanished for the same value of z, Jn+i 
would also vanish for that value. But in virtue of (8) § 200 
this would requii-e that all the functions /„ vanish for the value 
of z in question \ 

206. The actual values of z^ may be found by interpolation 
from Hansen's tables so far as these extend ; or formulae may be 
calculated from the descending series by the method of successive 
approximation, expressing the roots directly. For the important 
case of the symmetrical vibrations (n = 0), the values of z^ may be 
found from the following, given by Stokes': 

z^^*^ ^. '050661 '053041 2 62051 .-. 

For n = 1, the formula is 

z^_ -151982 015399 _ '245270 
It -f+^^ 4«+r"^(4«-My (45+l)» ^ ^* 

The latter series is convergent enough, even for the first root, 
corresponding to « = 1. The series (1) will suffice for values of b 
greater than unity; but the first root must be calculated 
independently. The accompanying table (A) is taken from 
Stokes' paper, with a slight diflFerence of notation. 

It will be seen either from the formulae, or the table, that the 
diflference of successive roots of high order is approximately tt. 
This is true for all values of «, as is evident from the descending 
series (10) § 200. 

[The general formula, analogous to (1) and (2), for the roots of 
Jn C-^) has been investigated by Prof. M*^Mahon. If m = 4w*, and 
a = j7r(2n-l+4«) (3), 

32(»t-l)(83w''- 982ot + 3779) 

15 (8a)» 


^ Bourget, " M($moire sur le mouyement vibratoire des membranes circulaires," 
Ann, de Vecole nortnale, t. iii., 1866. In one passage M. Boarget implies that he 
has proved that no two Bessel's functions of integral order can have the same root, 
bat I cannot find that he has done so. The theorem, however, is probably true ; 
in the case of functions, whose orders differ by 1 or 2, it may be easily proved from 
the formuls of § 200. 

^ Camb, Phil, Trans. Vol. ix. ** On the numerical calculation of a class of defi- 
nite Integrals and infinite series." [In accordance with the calculation of Prof. 
M*^Mahon the numerator of the last term in (2) has been altered from '245835 
to -246270.] 

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This formula may be applied not only to integral values of n as Id 
(1) and (2), but also when n is fractional. The cases of n = 4, and 
71 == } are considered in § 207.] 

M. Bourget has given in his memoir very elaborate tables of 
the frequencies of the different simple tones and of the radii of 
the nodal circles. Table B includes the values of z, which satis^* 
*/„(-?), for w = 0,1,... 5, « = 1, 2, ... 9. 

Table A. 


-for /,(«) = 0. 


























-fory,(«) = 0. 














12 2469 

1^001 1 

When n is considerable the calculation of the earlier roots 
becomes troublesome. For very high values of n, -?»<'7^ approxi- 
mates to a ratio of equality, as may be seen from the consideration 
that the pitch of the gravest tone of a very acute sector must tend 
to coincide with that of a long parallel strip, whose width i3 equal 
to the greatest width of the sector. 

Table B. 

— \ 


n = 


n = 2 

n = 3 

n = 4 

n = 5 1 
























































31-813 , 







34-983 1 

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3.0 52 



The figures represent tlie more important normal modes of 
vibration, and the numbers affixed give the frequency referred to 

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the gravest as unity, together with the radii of the circular node 
expressed as fractions of the radius of the membrane. In the cas 
of six nodal diameters the frequency stated is the result of a rougl 
calculation by myself. 

The tones corresponding to the various fundamental modes o 
the circular membrane do not belong to a harmonic scale, bu 
there are one or two approximately harmonic relations which ma; 
be worth notice. Thus 

^ X 1-594 = 2125 = 2-136 nearly, 
f X 1-594. = 2-657 = 2-653 nearly, 
2 X 1-594 = 3188 = 3*156 nearly; 

so that the four gravest modes with nodal diameters only woul( 
give a consonant chord. 

The area of the membrane is divided into segments by thi 
nodal system in such a manner that the sign of the vibratioi 
chunges whenever a node is crossed. In those modes of vibratioi 
which have nodal diameters there is evidently no displacement o 
the centre of inertia of the membrane. In the case of symmetri 
cal vibrations the displacement of the centre of inertia is proper 
tional to 

|Vo (h-) rdr = - j^ U" (kr) + ji J^' (kr) I I'dr = - | ^o' (*«), 

iiD expression which does not vanish for any of the admissible 
values of k, since Jo (z) and J^ (z) cannot vanish simultaneously 
111 all the symmetrical modes there is therefore a displacement o 
the centre of inertia of the membrane. 

207. Hitherto we have supposed the circular area of th( 
membrane to be complete, and the circumference only to b( 
fixed; but it is evident that our theory virtually includes th( 
solution of other problems, for example — some cases of a mem 
brane bounded by two conceutric circles. The complete theorj 
for a membrane in the form of a ring requires the second Bessel't 

The problem of the membrane in the form of a serai-circle 
may be regarded as already solved, since any mode of vibration 
of which the semi-circle is capable must be applicable to the 

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207.] FIXED BADIUS. 333 

complete circle also. In order to see this, it is only necessary 
to attribute to any point in the complementary semi-circle the 
opposite motion to that which obtains at its optical image in 
the bounding diameter. This line will then require no constraint 
to keep it nodal. Similar considerations apply to any sector 
whose angle is an aliquot part of two right angles. 

When the opening of the sector is arbitrary, the problem 
may be solved in terms of Bessels functions of fractional order. 
If the fixed radii are d = 0, d = )8, the particular solution is 

w — PJ„fp(kr) sin ^ cos(2>^ — c) (1), 

where i/ is an integer. We see that if fi be an aliquot part of tt,. 
mrfff is integral, and the solution is included among those ab eady 
used for the complete circle. 

An interesting case is when fi = 2ir, which corresponds to the 
problem of a complete circle, of which the 
radius = is constrained to be nodal. ^'^8' ^®' 

We have 

w = PJ^y (kr) sin ^v0 cos (pt — e). 
When V is even, this gives, as might be 
expected, modes of vibration possible without 
the constraint; but, when v is odd, new 
modes make their appearance. In fact, in 
the latter case the descending series for / 
terminates, so that the solution is expressible in finite terms. 
Thus, when i/ = 1, 

sin fc7* 
^"^V(F)^'''*^ cos(p^-6) (2). 

The values of k are given by 

sin ka = 0, or ka = stt. 

Thus the circular nodes divide the fixed radius into equal 
parts, and the series of tones form a bar- j.j 39 

monic scale. In the case of the gravest 
mode, the whole of the membrane is at any 
moment deflected on the same side of its 
equilibrium position. It is remarkable that 
the application of the constraint to the 
radius 0^0 makes the problem easier than 

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If we take v = 3, the solution is 

In this case the nodal radii are Fig. (39) 

and the possible tones are given by the equation 

tan ka=:ka 

To calculate the roots of tan a? = a; we may assume 

a: = (* + i)7r-y = Z-y, 

where y is a positive quantity, which is small when x is large. 

Substituting this, we find cot y = X - y, 

* zv -a: Z' v 3 15 315 ••• 

This equation is to be solved by successive approximatio 
It will readily be found that 


60 that the roots of tan x^^x are given by 

• (5). 


where X = (« 4- i) tt. 

In the first quadrant there is no root after zero since tan x > 
and in the second quadrant there is none because the signs 
X and tana; are opposite. The first root after zero is thus 
the third quadra it, corresponding to « = 1. Even in this ca 
the series converges sufficiently to give the value of the ro 
with considerable accuracy, while for higher values of a it 
all that could be desired. The actual values of x/ir are 1-430 
2-4590, 3-4709, 4-4747, 5-4818, 6-4844, &c. 

208. The effect on the periods of a slight inequality in tl 
density of the circular membrane may be investigated by tl 
general method § 90, of which several examples have alread 
been given. It will be sufficient here to consider the case of 

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small load M attached to the membrane at a point whose radius 
vector is /. 

We will take first the symmetrical types (n = 0), which may 
still be supposed to apply notwithstanding the presence of M. The 
kinetic energy T is (6) § 204 altered from 

and therefore 

/>«. .i»»-i p^„.j-;,(^^„) w. 

where P^ denotes the value of je>„w'i when there is no load. 

The uns3anmetrical normal types are not fully determinate for 
the unloaded membrane ; but for the present purpose they must 
be taken so as to make the resulting periods a maximum or 
minimum, that is to say, so that the effect of the load is the 
greatest' and least possible. Now, since a load can never raise 
the pitch, it is clear that the influence of the load is the least 
possible, viz. zero, when the type is such that a nodal diameter (it 
is indifferent which) passes through the point at which the load is 
attached. The unloaded membrane must be supposed to have two 
coincident periods, of which one is unaltered by the addition of the 
load. The other type is to be chosen, so that the alteration of 
period is as great as possible, which will evidently be the case 
when the radius vector / bisects the angle between two adjacent 
nodal diameters. Thus, if r' correspond to d = 0, we are to take 

V) = ^nn Jn {Kinr) COS Yid \ 

SO that (2) § 204 

T= i pira? 4>^n' Jn' (kfnna) + i if ^mn' Jn' {KnV). 

The altered p^n' is therefore given by 

Pmn^r^n p^a« /,/« (i^„a) ^^^' 

Of course, if r' be such that the load lies on one of the nodal 
circles, neither period is affected. 

For example, let M be at the centre of th^ membrane. J^ (0) 
vanishes, except when n = 0; aud Jo(0) = l. It is only the 
symmetrical vibrations whose pitch is influenced by a central load, 
and for them by (1) 

P-^"''^^-"^^''j-^(k,^a)~^a^ (3). 

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By (6) §200 Jo(z)^-Ji{zl 

so that the application of the formula requires only a knowledge of 
the values of «7i (z), when J^ (z) vanishes, § 200, For the gravest 
mode the value of Jo (Jcm<^) is '51903*. When Ar^o^ is consider- 

t/i' (^mott) =2-5- irkmod 

approximately; so that for the higher components the influence of 
the load in altering the pitch increases. 

The influence of a small irregularity in disturbing the nodal 
system may be calculated from the formulsB of § 90. The most 
obvious effect is the breaking up of nodal diameters into curves 
of hj^rbolic form due to the introduction of subsidiary sym- 
metrical vibrations. In many cases the disturbance is favoured 
by close agreement between some of the natural perioda 

209. We will next investigate how the natural vibrations of 
a uniform membrane are affected by a slight departure from the 
exact circular form. 

Whatever may be the nature of the boundary, w satisfies the 


<Pw I dw ^ 1 d^w , ,. ^ .^^ 

d> + ;: di^+i^ d^+*'«' = o (!)• 

where ifc is a constant to be determined. By Fourier's theorem w 
may be expanded in the series 

w = Wo + Wi COS {0 + ai) •{• w^cos 2 (0 + OLt) '\- 

+Wncosn(0+an) + , 

where w©, Wi, &c. are functions of r only. Substituting in (1), we 
see that Wn must satisfy 

d^Wn 1 dwn 



of which the solution is 


for, as in § 200, the other function of r cannot appear. 

The general expression for w may thus be written 

w = AoJo{kr) + Ji{kr)(AiCO8 + Bisin0) 

+ ... + Jn(kr)(AnCO8n0 -h Bnsmn0) + (2). 

For all points on the boundary w is to vanish. 

1 The succeeding Talues are approximately -341, *271, '282, *206, -187, Ac, 

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In the case of a nearly circular membrane the radius vector is 
nearly constant. We may take r — a + Br, 8r being a small 
function of 0. Hence the boundary condition is 

• O^A,[Jo(ka) + kBrJ,'(ka)] + 

4- [Jn (lea) -{-kSr Jn (ka)] [An cos n0 + Bn sin nO] 

+ (8), 

which is to hold good for all values of 0. 

Let us coQsider first those modes of vibration which are nearly 
symmetrical, for which therefore approximately 

w = AoJo(kr). 

All the remaining coefficients are small relatively to Aq, since 
the type of vibration can only differ a little from what it would 
be, were the boundary an exact circle. Hence if the squares of 
the small quantities be omitted, (3) becomes 

A^ [Jo {ka) + ASr Jo (ka)] 4- Ji (ka) [A^ cos ^ + jBi sin 0] 

+ . . . + t/n (ka) [AnCO8n0 + BnSmn0]+ ...=0 (4). 

If we integrate this equation with respect to between the 
limits and 27r, we obtain 

27r Jo (ka) + Jo (ka) r'kBrdd = 0, 

ka + kfjSr ^1=0 (5), 

or Jo- 

which shews that the pitch of the vibration is approximately the 
same as if the radius vector had uniformly its mean value. 

This result allows us to form a rough estimate of the pitch of 
any membrane whose boundary is not extravagantly elongated. 
If a denote the area, so that pa is the mass of the whole mem- 
brane, the frequency of the gravest tone is approximately 

(27r)-^ X 2-404 x y/^> (6)^ 

In order to investigate the altered type of vibration, we may 

* [A numerical error is here corrected.] 


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multiply (4) by cos nO, or sinn^, and then integrate as before. 

/•2ir \ 

Ao Jo(ka) I k Br cos n0 dd-^irAn Jn (ka) = 




AoJo(ka)r'kBrsmn0d0 + irBnJn(ka)^O 

which determine the ratios An : Aq and Bn : Ao. 

If Sr = Sro + 5riH- ... + Srn+... 

be Fourier's expansion, the final expression for w may be writt'en, 
w iAq^Jq (kr) 

When the vibration is not approximately symmetrical, the 
question becomes more complicated. The normal modes for the 
truly circular membrane are to some extent indeterminate, but the 
irregularity in the boundary will, in general, remove the indeter- 
minateness. The position of the nodal diameters must be taken, 
so that the resulting periods may have maximum or minimum 
values. Let us, however, suppose that the approximate type is 

w^A,J^{kr)Q(^ve (9), 

and afterwards investigate how the initial line must be taken in 
order that this form may hold good. 

All the remaining coefficients being treated as small in com- 
parison with ^^, we get from (4) 

Aq Jq (ka) + ... + Ay[J^ (ka) + kirJJ (4a)] cos vd 

'\-B^J,(ka)8iav0 •{• 

'\-Jn{ka)[AnCiysn0'\'BnCosnd] + .,.^0 (10). 

Multiplying by cos v0 and integrating, 


IT J, (ka) + k J/ (ka) Br cos* v0d0 = 0, 

J^ pa + Ar I Sr cos* i/^ — I = 0, 

which shews that the effective radius of the membrane is 

a4-/>cos.^f (IIX 

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The ratios of An and Bn to Ay may be found as before by in- 
tegrating equation (10) after multiplication by cos nO, sin nd. 

But the point of greatest interest is the pitch. The initial line 
is to be so taken as to make the expression (11) a maximum or 
minimum. If we refer to a line fixed in space by putting d — a 
instead of 0, we have to consider the dependence on a of the 

' 5rcos« !/(<?-- a) dd, 



which may also be written 

cos* va I Sr cos^ i0d0 + 2 cos i/a sin va j Br cos i^O sin v0d0 

-hsin^vaj Srsm^v0d0 (12), 

and is of the form 

A cos* va 4- 25 cos va sin va + C sin* i/a, 

A, B, C being independent of a. There are accoi-dingly two 
admissible positions for the nodal diameters, one of which makes 
the period a maximum, and the other a minimum. The diameters 
of one set bisect the angles between the diameters of the other 

There are, however, cases where the normal modes remain inde- 
terminate, which happens when the expression (12) is independent 
of a. This is the case when Br is constant, or when Br is propor- 
tional to cos v0. For example, if Br were proportional to cos 20, 
or in other words the boundary were slightly elliptical, the nodal 
system corresponding to n = 2 (that consisting of a pair of per- 
pendicular diameters) would be arbitrary in position, at least to 
this order of approximation. But the single diameter, correspond- 
ing to n = l, must coincide with one of the principal axes of 
the ellipse, and the periods will be different for the two axes. 

210. We have seen that the gravest tone of a membrane, 
whose boundary is approximately circular, is nearly the same as 
that of a mechanically similar membrane in the form of a circle of 
the same mean radius or area. If the area of a membrane be 
given, there must evidently be some form of boundary for which 
the pitch (of the principal tone) is the gravest possible, and this 


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form can be no other than the circle. In the ca^e of approximat 
circularity an analytical demonstration may be given, of which th 
following is an outline. 

The general value of w being 

u; = ilot/o(^)4- ... + Jn(AT) (-4nC08 7i^4-5sinn6?) + (1), 

in which for the present purpose the coeflScients A^B^,... are smal 
relatively to -4©, we find from the condition that w vanishe 
when r = a-\-tr, 

A,J,{ka) + kA,J,'{ka)Zr + \l^A,J^\ka),{h^)''^ 

+ 2 [[Jn{ka) + 1cJn{ka) 8r + ...}{ilHCOsn^ + JBnsin n^}] = 0...(2). 

Hence, if 

8r = a, cos ^ + /8i sin d + . . . + a„ cos n^ + )8„ sin wd + (3), 

we obtain on integration with respect to from to 27r, 

2A, Jo + i k^A, Jo" 2^]* «•• + Pn^) 

+ A:2^^J(a,,4n + /3nfin)Jn'] = (4). 

from which we see, as before, that if the squares of the smal 
quantities be neglected, Jo (ka) = 0, or that to this order of ap 
proximation the mean radius is also the eflfective radius. Ii 
order to obtain a closer approximation we first determine A^ : A 
and Bn : -4© by multiplying (2) by cos nO, sin nd, and then in 
tegrating between the limits and 27r. Thus 

AfiJn = "■ kanA Jo , Bf^Jn = " kpf^ AqJo (5). 

Substituting these values in (4), we get 

J, (ka) = i *» t^ ^(a„^ + /3„') 1*^' - i J,' jl (6). 

Since Jo satisfies the fundamental equation 

Jo" + j^Jo' + Jo = (7), 

and in the present case Jo = approximately, we may replac 
Jo" '^y ~ IT *^o'- Equation (6) then becomes 

/,(A:a) = U-^/„'2;:;[(«..' + /3,.'){^' + 2j-}] (8). 

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Let us now suppose that a + cia is the equivalent radius of the 
membrane, so that 

Jo [* (a + da)] = Jo (lea) + Jo (ka) kda = 0. 

Then by (8) we find 

'^=-**ch'-»-^-'){^'-*-2y] <^>- 

Again, if a + da' be the radius of the truly circular membrane 
of equal area, 

A»' = ^X^"(a„» + /9„') (10); 

SO that 

The question is now as to the sign of the right-hand member. 
If n = 1, and z be written for ka, 

vanishes approximately by (7), since in general J^^ — J^\ and 
in the present case Jo {z) = nearly. Thus da' — da = 0, as should 
evidently be the case, since the term in question represents merely 
a displacement of the circle without an alteration in the form of 
the boundary. When n = 2, (8) § 200, 

t/2 — — t/i — t/oi 

from which and (7) we find that, when Jo = 0, 


J, 2z 



da'-da = ^(a,«+A»)g'-l) (13), 

which is positive, since -» — 2*404. 
We have still to prove that 


is positive for integral values of n greater than 2, when z » 2*404. 

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For this purpose we may avail ourselves of a theorem given i 
Riemann's Partielle Differentialgleichungen, to the effect thi 
neither «/» i^or J^ has a root (other than zero) less than n. Tt 
differential equation for Jn may be put into the form 


+ (^-n»)/„(^)=t); 

while initially Jn and Jn (as well as dJn/d log z) are positive. A( 
cordingly dJn/d log z begins by increasing and does not cease to d 
so before z = n, from which it is clear that within the range z = 
to ^ = n, neither Jn nor Jn can vanish. And since Jn and /«' ai 
both positive until z^n/it follows that, when n is an integer greats 
than 2*404, da' — da is positive. We conclude that, unless o,, )8 
a„ ... all vanish, da' is greater than da, which shews that in tb 
case of any membrane of approximately circular outline, the circl 
of equal area exceeds the circle of equal pitch. 

We have seen that a good estimate of the pitch of an approx 
mately circular membrane may be obtained from its area alon< 
but by means of equation (9) a still closer approximation may b 
effected. We will apply this method to the case of an elh*ps( 
whose semi-axis major is R and eccentricity e. 

The polar equation of the boundary is 

r^R {l-Je>-^e* + +Je«cos2d + } (14); 

so that in the notation of this section 

a = /i(l-ie»-^e*), Oa^ie^iJ. 

Accordingly by (9) 

*^=-w-*^-{:^V) + 2.}' 

or by (12), since A:iJ = -a: = 2*404, 


Thus the radius of the circle of equal pitch is 
^, i>fi 1^ 9-779 e*) 

in which the term containing e* should be correct. 


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The result may also be expressed in terms of e and the area <r. 
We have 

and thus 

from which we see how small is the influence of a moderate eccen- 
tricity, when the area is given. 

211. When the fixed boundary of a membrane is neither 
straight nor circular, the problem of determining its vibrations 
presents difficulties which in general could not be overcome 
without the introduction of functions not hitherto discussed or 
tabulated. A partial exception must be made in favour of an 
elliptic boundary ; but for the purposes of this treatise the im- 
portance of the problem is scarcely sufficient to warrant the 
introduction of complicated analysis. The reader is therefore 
referred to the original investigation of M. Mathieu^ 

[The method depends upon the use of conjugate functions. If 

a? + iy = 6Cos(f + ii;) (1), 

then the curves tf = const, are confocal ellipses, and f = const, are 
confocal hjrperbolas. In terms of f , i; the fundamental equation 
(V* + A*)tt = becomes 

^ + g+A;''(co8h«i,-co8«f)tt = (2). 

where k^ =« ke. 

The solution of (2) may be found in the form 

u.H(f).H(i,) (3), 

in which H is a function of f only, and H a function of tf only, 

^-(i'»cos»f-.a)H = (4), 

J" + (Jb'»cosh>i;-a)H = (5), 

a being an arbitrary constants 

^ LiouTille, xm., 1S6S; Cour$ de physique mathimatique^ 1878, p. 122. 
' Pockels, Oher diepartielle DifferentiaXgleichung ^u-k-l?u^Of p. 114. 

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Michell* has shewn that the elliptic transformation (1) is tl 
only one which yields an equation capable of satisfiewtion in tl 
form (3).] 

Soluble cases may be invented by means of the gener 

w = AoJo(kr)'\- .,.+{AnCosn0 + BnSinn6)Jn(kr)+ 

For example we might take 

w = Jo (kr) — \ J"i (At) cos 0, 

and attaching different values to \, trace the various forms 
boundary to which the solution will then apply. 

Useful information may sometimes be obtained from tl 
theorem of § 88, which allows us to prove that any contraction < 
the fixed boundary of a vibrating membrane must cause an elevj 
tion of pitch, because the new state of things may be conceived 1 
differ from the old merely by the introduction of an addition 
constraint. Springs, without inertia, are supposed to urge tl 
line of the proposed boundary towards its equilibrium positio 
and gradually to become stiffer. At each step the vibratioi 
become more rapid, until they approach a limit, corresponding 
infinite stiffness of the springs and absolute fixity of their poin 
of application. It is not necessary that the part cut off shou 
have the same density as the rest, or even any density at all. 

For instance, the pitch of a regular polygon is intermedia 
between those of the inscribed and circumscribed circles. Clas 
limits would however be obtained by substituting for the circur 
scribed circle that of equal area according to the result of § 21 
In the case of the hexagon, the ratio of the radius of the circle 
equal area to that of the circle inscribed is I'OoO, so that the m« 
of the two limits cannot differ from the truth by so much as 2^ p 
cent. In the same way we might conclude that the sector of 
circle of 60° is a graver form than the equilateral triangle obtaini 
by substituting the chord for the arc of the circle. 

The following table giving the relative frequency in certa 
calculable cases for the gravest tone of membranes under simil 
mechanical conditions and of eqiial area (or), shews the effect of 
greater or less departure from the circular form. 

* Messenger of Mathematics, vol. xix. p. 86, 1890. 

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Circle 2404 . a/tt « 4-261. 

Square ^2 . tt = 4*443. 

Qaadrant of a circle -^— . \/w = 4'551. 

Sector of a circle 6(y> 6-379 a/| = 4*616. 

Rectangle 3x2 a/^ . tt = 4624. 

Equilateral triangle 27r . Vtan 30* = 4-774. 

Semicircle 3-832 W ^ = 4-803. 

1 = 4-967. 

Rectangle 2 x 1 

Right-angled isosceles triangle 

Rectangle 3 X 1 w- A/-n- = 5-736. 

For instance, if a square and a circle have the same area, the 
former is the more acute in the ratio 4*443 : 4*261, or 1*043 : 1. 

For the circle the absolute frequency is 

(2^)-^x2-404c>y/^, where c=-^/T^^^p, 

In the case of similar forms the frequency is inversely as the 
linear dimension. 

[From the principle that an extension of boundary is always 
accompanied by a fall of pitch, we may infer that the gravest 
mode of a membrane of any shape, and of any variable density, is 
devoid of internal nodal lines.] 

212. The theory of the free vibrations of a membrane was 
first successfully considered by Poisson^ His theory in the 
case of the rectangle left little to be desired, but his treatment 
of the circular membrane was restricted to the sjonmetrical 
vibrations. Kirchhoff's solution of the similar, but much more 
difficult, problem of the circular plate was published in 1850, 
and Clebsch's Theory of EUtstidty (1862) gives the general theory 
of the circular membrane including the effects of stiffness and 

1 M6m. de VAcadSmie, t. vin. 1829. 

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of rotatory inertia^ It will therefore be seen that there was not 
much left to be done in 1866 ; nevertheless the memoir of Bourget 
already referred to contains a useful discussion of the problem 
accompanied by very complete numerical results, the whole of 
which however were not new. 

213. In his experimental investigations M. Bourget made use 
of various materials, of which paper proved to be as good as any. 
The paper is immersed in water, and after removal of the superfluous 
moisture by blotting-paper is placed upon a frame of wood whose 
edges have been previously coated with glue. The contraction of the 
paper in dr3ring produces the necessary tension, but many fidlures 
may be met with before a satisfactory result is obtained. Even 
a well stretched membrane requires considerable precautions in 
use, being liable to great variations in pitch in consequence of the 
varying moisture of the atmosphere. The vibrations are excited 
by organ-pipes, of which it is necessary to have a series proceeding 
by small intervals of pitch, and they are made evident to the eye 
by means of a little sand scattered on the membrane. If the 
vibration be sufficiently vigorous, the sand accumulates on the 
nodal lines, whose form is thus defined with more or less precision. 
Any inequality in the tension shews itself by the circles becoming 

The principal results of experiment are the following : — 

A circular membrane cannot vibrate in unison with every sound. 
It can only place itself in unison with sounds more acute than 
that heard when the membrane is gently tapped. 

As theory indicates, these possible sounds are separated by less 
and less intervals, the higher they become. 

The nodal lines are only formed distinctly in response to 
certain definite sounds. A little above or below confusion ensues, 
and when the pitch of the pipe is decidedly altered, the membrane 
remains unmoved. There is not, as Savart supposed, a continuous 
transition from one system of nodal lines to another. 

The nodal lines are circles or diameters or combinations of 
circles and diameters, as theory requires. However, when the 

^ [The reader who wishes to pursue the subject from a mathematical poiDt of 
view is referred to an excellent discussion by Pockels (Leipzig, 1891) of Uh 
di£Ferential equation \i^u-\-kHmOJ] 

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number of diameters exceeds two, the sand tends to heap itself 
confusedly towards the middle of the membrane, and the nodes 
are not well defined. 

The same general laws were verified by MM. Bernard and 
Bourget in the case of square membranes^; and these authors 
consider that the results of theory are decisively established in 
opposition to the views of Savart, who held that a membrane 
was capable of responding to any sound, no matter what its pitch 
might ba £ut I must here remark that the distinction between 
forced and free vibrations does not seem to haTe been sufficiently 
borne in mind. When a membrane is set in motion by aerial 
waves having their origin in an organ-pipe, the vibration is 
properly speaking forced. Theory asserts, not that the membrane 
is only capable of vibrating with certain defined frequencies, but 
that it is only capable of so vibrating freely. When however the 
period of the force is not approximately equal to one of the 
natural periods, the resulting vibration may be insensible. 

In Savart's experiments the sound of the pipe was two or three 
octaves higher than the gravest tone of the membrane, and was 
accordingly never far from unison with one of the series of over- 
tones. MM. Bourget and Bernard made the experiment under 
more &vourable conditions. When they sounded a pipe somewhat 
lower in pitch than the gravest tone of the membrane, the sand 
remained at rest, but was thrown into vehement vibration as unison 
was approached. So soon as the pipe was decidedly higher than the 
membrane, the sand returned again to rest. A modification of the 
experiment was made by first tuning a pipe about a third higher 
than the membrane when in its natural condition. The membrane 
was then heated until its tension had increased sufficiently to 
bring the pitch above that of the pipe. During the process of 
cooling the pitch gradually fell, and the point of coincidence 
manifested itself by the violent motion of the sand, which at the 
beginning and end of the experiment was sensibly at rest. 

M. Bourget found a good agreement between theory and obser- 
vation with respect to the radii of the circular nodes, though the 
test was not very precise, in consequence of the sensible width of 
the bands of sand ; but the relative pitch of the various simple 
tones deviated considerably from the theoretical estimates. The 

^ Am. de Ghim. lx. 449—479. 1860. 

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committee of the French Academy appointed to report 
M. Bourget's memoir suggest as the explanation the want 
perfect fixity of the boundary. It should also be remembered tl 
the theory proceeds on the supposition of perfect flexibility- 
condition of things not at all closely approached by an ordina 
membrane stretched with a comparatively small force. B 
perhaps the most important disturbing cause is the resistance 
the air, which acts with much greater force on a membrane th 
on a string or bar in consequence of the large surface expose 
The gravest mode of vibration, during which the displacement 
at all points in the same direction, might be affected ve 
differently from the higher modes, which would not require 
great a transference of air from one side to the other. 

[In the case of kettle-drums the matter is further complicat 
by the action of the shell, which limits the motion of the air up 
one side of the membrane. From the fact that kettle-drums i 
struck, not in the centre, but at a point about midway betwe 
the centre and edge, we may infer that the vibrations which it 
desired to excite are not of the symmetrical class. The sound 
indeed but little affected when the central point is touched wi 
the finger. Under these circumstances the principal vibration {I] 
that with one nodal diameter and no nodal circle, and to tl 
corresponds the greater part of the sound obtained in the nom 
use of the instrument. Other tones, however, are audible, whi 
correspond with vibrations characterized (2) by two nodal diamet 
and no nodal circle, (3) by three nodal diameters and no no< 
circles, (4) by one nodal diameter and one nodal circle. " 
observation with resonators upon a large kettle-drum of 25 incl 
diameter the pitch of (2) was found to be about a fifth above ( 
that of (3) about a major seventh above (1), and that of (4) a lit 
higher again, forming an imperfect octave with the principal to 
For the corresponding modes of a uniform perfectly flexible me 
brane vibrating in vdcuo, the theoretical intervals are th« 
represented by the ratios 1-34, 1'66, 1*83 respectively \ 

The vibrations of soap films have been investigated by Meld 
The frequencies for surfaces of equal area in the form of the cin 
the square and the equilateral triangle, were found to be 

if — 

1 Phil Mag., vol. vii., p. 160, 1879. ^ 

a Pogg. Ann,, 169, p. 275, 1876. Akustik, p. 131, 1883. 


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1*000 : 1'049 : 1'175. In membranes of this kind the tension is 
due to capillarity, and is independent of the thickness of the film.] 

213 a. The forced vibrations of square and circular membranes 
have been further experimentally studied by Elsas^ who has 
confirmed the conclusions of Savart as to the responsiveness of a 
membrane to sounds of arbitrary pitch. In these experiments the 
vibrations of a fork were communicated to the membrane by means 
of a light thread, attached normally at the centre ; and the position 
of the nodal curves and of the maxima of disturbance was traced 
in the usual manner by sand and lycopodium. A series of figures 
accompanies the memoir, shewing the effect of sounds of pro- 
gressively rising pitch. 

In many instances the curves found do not exhibit the 
symmetries demanded by the supposed conditions. Thus in 
the case of the square membrane all the curves should be similarly 
related to the four comers, and in the case of the circular mem- 
brane all the curves should be circles. The explanation is probably 
to be sought in the difficulty of attaining equality of tension. If 
there be any irregularity, the effect will be to introduce modes of 
vibration which should not appear, as having nodes at the point of 
excitation, and this especially when there is a near agreement of 
periods. Or again, an irregularity may operate to disturb the 
balance between two modes of theoretically identical pitch, which 
should be excited to the same degree. Indeed the passage through 
such a- point of isochronism may be expected to be highly unstable 
in the absence of moderate dissipative forces. 

The theoretical solution of these questions has already (§§ 196, 
204) been given, but would need much further development for 
an accurate determination of the nodal curves relating to periods 
not included among the natural periods. But the general course 
of the phenomenon can be traced without difficulty. 

If the imposed frequency be less than the lowest natural 
frequency, the vibration is devoid of (internal) nodes. For a nodal 
line, if it existed, being of necessity either endless or terminated 
at the boundaiy*, would divide the membrane into two parts. Of 

^ Nova Acta der K$l. Leap. Carol. Deutschen Akademie^ Bd. xlv. Kr. 1. Halle, 

' Otherwise the extremity would have to remain at rest under the action of 
component tensions from the surrounding parts which are all in one di^ction. 

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these one part would be vibrating freely with a frequency 
than the lowest natural to the whole membrane, an imposs 
condition of things (§ 211). The absence of nodal curves under 
above-mentioned conditions is one of the conclusions drawn 
Elsas from his observations. 

As the frequency of the imposed vibration rises through 
lowest natural frequency, a nodal curve manifests itself round 
point of excitation, and gradually extends. The course of thi 
is most easily followed in the case of the circular membn 
excited at the centre. The nodal curves are then of necessity i 
circles, and it is evident that the first appearance of a nodal ci] 
can take place only at the centre. Otherwise there would b 
circular annulus of finite internal diameter, vibrating freely wit 
frequency only infinitesimally higher than that of the entire cir 
At first sight indeed it might appear that even an infinitely sn 
nodal circle would entail a finite elevation of pitch, but a c 
sideration of the solution (§ 204) as expressed by a combinatioi 
Bessel's functions of the first and second kinds, shews that thi 
not the case. At the point of isochronism the second funct 
disappears, and immediately afterwards re-enters with an infinit 
small coefficient. But inasmuch as this function is itself infio 
when r = 0, a nodal circle of vanishing radius is possible. Acco 
ingly the fixation of the centre of a vibrating circular membrs 
does not alter the pitch, a conclusion which may be extended 
the fixation of any number of detached points of a membrane 
any shape. 

The eflfect of gradually increasing frequency upon the na 
system of a circular membrane may be thus summarized. Bel 
the first proper tone there is no internal node. As this point 
reached, the mode of vibration identifies itself with the cor 
sponding free mode, and then an infinitely small nodal cir 
manifests itself. As the frequency further increases, this cir 
expands, until when the second proper tone is reached, it coinci( 
with the nodal circle of the free vibration of this frequen 
Another infinitely small circle now appears, and it, as well as 1 
first, continually expands, until they coincide with the nodal spt 
of a free vibration in the third proper tone. This process c< 
tinues as the pitch rises, every circle moving continually outwar 
At each coincidence with a natural frequency the nodal syst< 
identifies itself with that of the free vibration, and a new cir 
begins to form itself at the centre. 

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213 a.] 



The behaviour of a square membrane is of course more difficult 
to follow in detail. The transition fjx)m Fig. (34) case (4), corre- 
sponding to m = 3, n = 1, and m = 1, n = 3, to Fig. (36) where m = 3, 
n = 3, can be traced in Elsas's curves through such forms as 

Fig. 39 a. 



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214. In order to form according to Green's method the equ 
tions of equilibrium and motion for a thin solid plate of unifor 
isotropic material and constant thickness, we require the expressi( 
for the potential energy of bending. It is easy to see that for ea 
unit of area the potential energy F is a positive homogeneo 
symmetrical quadratic function of the two principal curvaturi 
Thus, if pu Pihe the principal radii of curvature, the expressii 
for V will be 

Aa^\^^) (1). 

where A and /i are constants, of which A must be positive, ai 
fM must be numerically less than unity. Moreover if the materi 
be of such a character that it undergoes no lateral contracti* 
when a bar is pulled out, the constant /i must vanish. Tl 
amount of information is almost all that is required for o 
purpose, and we may therefore content oiu*selves with a me 
statement of the relations of the constants in (1) with those 1 
means of which the elastic properties of bodies are usually d 

From Thomson and Tait s Natural Philosophy, §§ 639, 64 
720, it appears that, if 2A be the thickness, q Youngs moduli 

^ [This Chapter deals only with flexural vibrations. The extensional vibratio 
of an infinite plane plate are briefly considered in Chapter X.a, as a particoi 
case of those of an infinite cylindrical shell. They are not of much acoustic 

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aod fi the ratio of lateral contraction to longitudinal elongation 
when a bar is pulled out, the expression for V is 

gA' ffi , ly 2(1-/*) ) .2V 

[Equation (2) gives the interpretation of the constants of (1) 
in its application to a homogeneous plate of isotropic material ; 
.but the expression (1) itself is of far wider scope. The material 
composing the plate may vary from layer to layer, and the elastic 
chiEuracter of any layer need not be isotropic, but only symmetrical 
with respect to the normal. As a particular case, the middle 
layer, or indeed any other layer, may be supposed to be physically 

Similar remarks apply to the investigations of the following 
chapter relating to curved shells.] 

If w be the small displacement perpendicular to the plane 
of the plate at the point whose rectangular coordinates in the 
plane of the plate are x, y, 

11-^ 1 d^wd^w fd^wy 

Pi pi ' Pipi dx" df \dxdy) ' 

and thus for a unit of area, we have 


which quantity has to be integrated over the surfa<^ {S) of the 

^ The foUowiDg comparison of the notations used by the principal writers may 
save trouble to those who wish to consult the original memoirs. 

Rigidity =n (Thomson) =^ (Lam6). 

Young's modulus =£ (Clebsch) =3f (Thomson) = -^ - (Thomson) 

O/C + H 

^ n(8TO~n) (Thomson) =g (Kirchhoflf and Donkin)=2JS:^^ (Kirchhoff). 
Ratio of lateral contraction to longitudinal elongation =/x (Clebsoh and Donkin) 
=ir (Thomson) =!^'* (Thomson) = ^-J^^ (Kirchhoff) r:^-^^^ (Lam6). 
Poiseon assumed this ratio to be }, and Wertheim |. 

R- 23 

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216. We proceed to find the variation of V, but it Bhould 

previously noticed that the second term in F, namely (I- 

represents the total curvature of the plate, and is therefore d 
pendent only on the state of things at the edge. 

80 that we have to consider the two variations 

jjV^w.V^iw.dS and jjS(pipt)-'dS. 
Now by Green's theorem 
jh^w . V^Sw . dS = jh*w ,&w,dS 

-J-d^r-^-^+r'^^*' <2> 

in which ds denotes an element of the boundary, and d/dn denoi 
differentiation with respect to the normal of the boundary dra? 

The transformation of the second part is more difficult. ^ 


d^ivd^Sw d}wd}ho ^^ d}w cPStt^l ,„ 
(ic* dy^ dy* da^ dxdy dxdy] 

The quantity under the sigu of iutegratiou may be put ii 
the form 

, d^ /dSw d^w _ d8w d^w \ d_ /dSw d^w _ d£w d^w \ 
dy \ dy da? dx dxdy) dx\dx dy* dy dxdy) ' 
Now, if -f be any function of x and y, 

//^^dy = /^sin^d.| 

||^(irdy = jVcos^cfej 

where 6 is the angle between x and the normal drawn outwaK 
and the integration on the right-hand side extends round t 
boundary. Using these, we find 

^ rr^- f^ • g{d£wdhv ^d^ d?w) 
J J PiRi ~ i \dy da? dx (}xdy) 


+ Id^cos^l 

diw d?w ^ dSw d^w ) 
{da? dy^ dy dxdy)' 


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If we substitute for dSw/dx, dBw/dy their values in terms 
dSw/dfiy d^/ds, from the equations (see Fig. 40) 

dSw dSw ^ dhv . ^ 
- = _— cos ^ — J— sin d 
dx an as 

dSw dSw . >, . dSw ^ 

dy dn as 

Fig. 40. 


we obtain 

^ffdS [jdBwi.^^d^w^ 8/)^'^ o- D n<^'^] 

+ |i.^jco8^sin^(^-^)+(3m»^-cos'^)^-f...(o). 

The second integral by a partial integration with respect to 
8 may be put into the form 

Ck>llecting and rearranging our results, we find 


+ (cos..-sin«.)||)} 


-^{1." + 


^ ^ . ^ d^w \ ) ' 
+ 2cos^sm^ 1— ^j[ 



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There will now be no difficulty in forming the equation 
motion. If p be the volume density, and Z,p,7Ji,dS the transv 
force acting on the element dS, 

BV " jf 2ZphBwdS+ if 2phivBwd&=0 (7 

is the general variational equation, which must be true whati 
function (consistent with the constitution of the system) Sw i 
be supposed to be. Hence by the principles of the Calculu 



at every point of the plate. 

If the edges of the plate be free, there is no restriction on 
hypothetical boundary values of Sw and dSw/dn, and therefore 
coefficients of these quantities in the expression for S Fmust vao 
The conditions to be satisfied at a free edge ai'e thus 


+ (cos«^.sin«^)|^}=0 


;xV^ + (l-M){cos«5^ + sin«<?*^ 

+ 2co8^sind:^^l=0 

If the whole circumference of the plate be clamped, iw- 
dSw/dn = 0, and the satis&ction of the boundary conditioDi 
already secured. If the edge be ' supported'*, Sw == 0, but diw 
is arbitrary. The second of the equations (9) must in this case 
satisfied by w, 

216. The boundary equations may be simplified by gett 
rid of the extrinsic element involved in the use of Cartes 
coordinates. Taking the axis of x parallel to the normal of 
bounding curve, we see that we may write 



COS* d j-r + sm* ^ 3-^ + 2 COS ^ sm ^ ^—5- - 
dx^ d'if dxdy 

— - cPw . d^w 
dn" dc^ 


* The rotatoiy inertia is here neglected. 

* Compare § 163. 

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where <risA fixed axis coinciding with the tangent at the point 
under consideration. In general d^w/da* differs fix)m d^wjdsK 
To obtain the relation between them, we may proceed thus. 
Expand w by Maclaurin's theorem in ascending powers of the 
small quantities n and <r, and substitute for n and a their values 
in terms of «, the arc of the curve. 

Thus in general 

dw dw , ^w , d^w , d^w , 

(Wio da-o ^ dn^ dfiodco ^da^^ 

while on the curve o- = « + cubes, n = — ^ «*//> -»- . ., , where p is 
the radius of curvature. Accordingly for points on the curve, 

, dw ^ dw . d?w . . , J. 
t(; = Wo — ij + j— * + i J— ¥ ^ + cubes of *, 

and therefore j-. * j~v 3- (2); 

cw" At* P dn '^ ' 

whence from (1) 

— , d^w \dw . cPw ,„. 

^**""d;^+p5;^ + d«» <«)• 

We conclude that the second boundary condition in (9) § 215 
may be put into the form 

d^w , (IdAV ^d?w\ ^ ,.. 

d^+^ipdi^-^SF)'^ <*)• 

In the same way by putting ^ == 0, we see that 

^ . >, fd^w d^w\ . .^ . _ ^. d^w 

18 equivalent to d^w/dndc, where it is to be understood that 
the axes of n and <r are fixed. The first boundary condition now 

l'--<>-''>5(il)- <«> 

If we apply these equations to the rectangle whose sides are 
parallel to the coordinate axes, we obtain as the conditions to be 
satisfied along the edges parallel to y, 

^{S"-*-")^"}-") ,,, 

d^w d^w ^ 

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In this case the distinction between o- and 8 disappears, and p, the 
radius of curvature, is infinitely great The conditioos for the 
other pair of edges are found by interchanging x and y. These 
results may be obtained equally well from (9) § 215 directly, with- 
out the preliminary transformation. 

217. If we suppose Z = 0, and write 

3p(l-/.»r^ ^^^' 

the general equation becomes 

ib + c'V^w^O (2), 

or, if w oc cos(p^ — e), 

V*u; = A*t(; (3X 

where k^^p'/c^ (4). 

Any two values of w, u and v, corresponding to the same 
boundary conditions, are conjugate, that is to say 


uvdS^O (5), 

provided that the periods be different. In order to prove this 
from the ordinary differential equation (3), we should have to 
retrace the steps by which (3) was obtained. This is the method 
adopted by Kirchhoff for the circular disc, but it is much simpler 
and more direct to use the variational equation 

SV'\'2phjfw&ivdS=-0 (6X 

in which w refers to the actual motion, and £u; to an arbitrazy 
displacement consistent with the nature of the system. SFis a 
symmetrical function of w and Sw, as may be seen fix)m § 215, or 
from the general character of V (§ 94). 

If we now suppose in the first place that w = u, Sw^v, we 


and in like manner if we put w=^v,Sw — u, which we are equally 
entitled to do, 


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This demonstration is valid whatever may be the form of the 
boundary, and whether the edge be clamped, supported, or free, in 
whole or in part 

As for the case of membranes in the last Chapter, equation 
(7) may be employed to prove that the admissible values of p^ are 
real ; but this is evident frx)m physical considerations. 

218. For the application to a circular disc, it is necessary to 
express the equations by means of polar coordinates. Taking the 
centre of the disc as pole, we have for the general equation to be 
satisfied at all points of the area 

(V*-/fc*)w = (1), 

1 _d 1 d« 
rdr r" 5^ ' 

where (§ 200) 

V*= 7, + -^ + ^ 

To express the boundary condition (§ 216) for a free edge 
(r = a), we have 

dn dr 

§LV^ ^/d*w^\ d d^(dw\ d^w _ d^w 
dr ^' d8\dnd^)~'~adddr\rd0)' d^^oH^' 

p ss radius of curvature = a ; and thus 

dr\dr^ r dr) dd^ \ a* dr a* 

'd}w 1 dmA ^ / 2-^ 
\d7^ rdr) de\ a« 

dr^'^^\id^'^ a^de^) 


After the diflferentiations are performed, r is to be made equal 
to a. 

If w be expanded in Fourier's series . 

w = Wo + Wi + ...H-t(;„ + ..., 
each, term separately must satisfy (2), and thus, since 

Wn X cos {nO — a), 

d_ [d*Wn 1 dWfa\ 

dr \ dr^ r dr 


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A I 



The superficial differential equation may be written 
(V» + i*)(V«-i*)w = 0, 
which becomes for the general term of the Fourier expansion 
/# Id n*^\fd^ Id w' ^\ _^ 

shewing that the complete value of Wn will be obtained by adding 
together, with arbitrary constants prefixed, the general solations of 

(£-?^-"*'-)»-<' <*^ 

The equation with the upper sign is the same as that which 
obtains in the case of the vibrations of circular membranes, and 
as in the last Chapter we conclude that the solution applicable 
to the problem in hand is WnOcJn (At), the second function of r 
being here inadmissible. 

In the same way the solution of the equation with the lower 
sign iawnocjn (tAr), where « s ^ (. 1) as usual. [See § 221 a] 

The simple vibration is thus 
Wn = cos ntf {aJn (At) + fiJn (ikr)] + sin n0 {yJn (At) + SJn (ikr)}. 

The two boundary equations will determine the admissible 
values of k and the values which must be given to the ratios 
a : fi and 7 : S. From the form of these equations it is evident 
that we must have ol : fi^y : S, 

and thus Wn may be expressed in the form 

Wn-PcosinO'-a) {Jn(kr)'\'\Jn(ikr)} cos (pt-e) (0). 

As in the case of a membrane the nodal system is composed of 
the n diameters symmetrically distributed rotind the centre, but 
otherwise arbitrary, denoted by 

cos(n^-a) = (6), 

together with the concentric circles, whose equation is 

Jn(AT) + XJn(tAT) = (7). 

219. In order to determine \ and A; we must introduce the 
boundary conditions. When the edge is free, we obtain from 
(3) § 218 

nV-1) likaJn\ika)-'Jni%ka)} + %lifa*Jn'i%ka) 

_^_ ifi-l){kaJn'(ka)^n*Jn{ka)}-'k'a*Jn{ka) 
(/* - 1) {ikaJn' (ika) - w« /« (ika)} + A"a« /« {ika) ) 


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in which use has been made of the differential equations satisfied 
by Jn(kr), Jn(ikr). In each of the fractions on the right the 
denominator may be derived from the numerator by writing ik in 
place of k. By elimination of X the equation is obtained whose 
roots give the admissible values of k. 

When n » 0, the result assumes a simple form, viz. 

2(i-.)t«.i^.*.J^!-o., <.). 

This, of course, could have been more easily obtained by neglecting 
n from the beginning. 

The calculation of the lowest root for each value of n is trouble- 
some, and in the absence of appropriate tables must be effected 
by means of the ascending series for the frmctions Jn{kr), Jn(ikr). 
In the case of the higher roots recourse may be had to the semi- 
convergent descending series for the same functions. Kirchhoff 

tan(A:a-in7r) ^-^^^^^--^-^—^^ (3). 



(7=7(1 -4n«) (9 -4»«) + 48(l + 4n«), 

D = - 7 J {(1 - 4n«) (9 - 4m') (13 - 4n«)} + 8 (9 + 136n« + SOn'). 

When ka is great, 

tan (ka - ^ nw) = approx. ; 

ia = i'7r(n + 2A) (4), 

where h is an integer. 

It appears by a numerical comparison that h is identical with 
the number of circular nodes, and (4). expresses a law discovered 
by Chladni, that the frequencies corresponding to figures with a 
given number of nodal diameters are, with the exception of the 
lowest, approximately proportional to the squares of consecutive 
even or uneven numbers, according as the number of the diameters 
is itself even or odd. Within the limits of application of (4), we 
see also that the pitch is approximately unaltered, when any 
number is subtracted from h, provided twice that number be 

Digitized by 





added to n. This law, of which traces appear in the following table, 
may be expressed by saying that towards raising the pitch nodal 
circles have twice the effect of nodal diameters. It is probable, 
however, that, strictly speaking, no two normal components have 
exactly the same pitch. 


»» = 









• • • 




* • • 

1 Ois 

QiB + 

A + 




2 gui' + 




e" + 


fi»" + 



n = 3 

, Ch. 






1 C 






1 g' 

gi8' + 



di8" + 


The table, extracted from Eirchhoff's memoir, gives the pitch 
of the more important overtones of a free circular plate, the gravest 
being assumed to be C^ The three columns under the heads 
Ch, P, W refer respectively to the results as observed by Chladni 
and as calculated from theory with Poisson's and Wertheim's 
values of ffr. A pltLS sign denotes that the actual pitch is a little 
higher, and a mimts sign that it is a little lower, than that written. 
The discrepancies between theory and observation are considerable, 
but perhaps not greater than may be attributed to irregularity in 
the plate. 

220. The radii of the nodal circles in the symmetrical case 
(n = 0) were calculated by Foisson, and compared by him with 
results obtained experimentally by Savart. The following numbers 
are taken from a paper by Strehlke^ who made some careful 
measurements. The radius of the disc is taken as unity. 

ObseiTation. Galcalation. 
. 0-67816 0-68062. 
fO-39133 0-39151. 
|0-84!l49 0-84200. 
[o-25631 0-25679. 
Three circles |o-59107 0-59147. 
io-89360 0-89381. 

^ Gifl correspondB to G^ of the English notation, and hiob nataral. 
« Pogg. Ann. xcv. p. 677. 1866. 

One circle . 
Two circles. 

Digitized by 





The calculated results appear to refer to Foisson's value of /i, but 
would vary very little if Wertheim's value were substituted. 

The following table gives a comparison of Eirchhofifs theory 
(n not zero) with measurements by Strehlke made on less accurate 

Radii of Circular Nodes. 


« = !, A=l 

n = 2, A=l 

» = 3, A=l 

n=l, h^2 



The most general motion of the uniform circular plate is 
expressed by the superposition, with arbitrary amplitudes and 
phases, of the normal components already investigated. The 
determination of the amplitude and phase to correspond to 
arbitraiy initial displacements and velocities is effected precisely 
as in the corresponding problem for the membrane by the aid of 
the characteristic property of the normal functions proved in § 217. 

221. When the plate is truly symmetrical, whether uniform 
or not, theory indicates, and experiment verifies, that the position 
of the nodal diameters is arbitrary, or rather dependent only on 
the manner in which the plate is supported, and excited. By 
vaiying the place of support, any desired diameter may be made 
nodal It is. generally otherwise when there is any sensible 
departure fix)m exact symmetry. The two modes of vibration, 
which originally, in consequence of the equality of periods, could 
be combined in any proportion without ceasing to be simple 
harmonic, are now separated and affected with different periods. 
At the same time the position of the nodal diameters becomes 
determinate, or rather limited to two alternatives. The one set is 
derived from the other by rotation through half the angle included 
between two adjacent diameters of the same set. This supposes 
that the deviation from uniformity is small ; otherwise the nodal 
system will no longer be composed of approximate circles and 
diameters at all The cause of the deviation may be an irregu- 
larity either in the material or in the thickness or in the form of 

Digitized by 





the boundary. The effect of a small load at any point may 1 
investigated as in the parallel problem of the membrane § 20 
If the place at which the load is attached does not lid on a nod 
circle, the normal types are made determinate. The diameti 
system corresponding to one of the types passes through the f\m 
in question, and for this type the period is unaltered. The peri( 
of the other type is increased. 

[The divergence of free periods, which is due to slight i 
equalities, would seem to afford an explanation of some curioi 
observations by Savart^ When a circular plate, vibrating wil 
nodal diameters, is under the influence of the bow applied at ai 
part of the circumference, the nodal diameters indicated by sand a 
so situated that the bow lies in the middle of a vibrating segmei 
If, however, the bow be suddenly withdrawn, the nodal syste 
oscillates, or even revolves, during the subsidence of the motio 
It is evident that no such displacement could be expecte 
were the plate absolutely symmetrical. The same would be tn 
even in the cas6 of asymmetry, if the bow were so applied as 
excite one only of the two determinate vibrations then possib 
But in general the effect of the bow must be to excite both kin 
of vibrations, and then the matter is more complicated. It won 
seem that so long as the constraining action of the bow lasts, bo 
vibrations are forced to keep the same time, and the effect 
much the same as in the case of symmetry. But on withdraw 
of the bow the free vibrations which then ensue take place each 
its proper frequency, and a phase difference soon arises by whi 
the effects are modified. 

Let us suppose that the origin of ^ is so chosen in relati 
to the irregularities that the types of vibration are represent 
by cos 710, sin n0. Then in general the free vibrations, result! 
from the action of the bow at an arbitrary point of the circu 
ference, may be taken to be 

cosna 8mn0 COS pt -- sin na cosnd coa(pt + e) (1), 

where e is the difference of phase which has accumulated sii 
the commencement of the fi^e vibrations. In the case 
symmetry e « 0, and (1) becomes 

sin n(0 — a) cos pt (2), 

1 Ann. Chim,f toI. 86, p. 257, 1827. 


Digitized by 



which represents a fixed nodal system 

0^a + m{v/n) (3), 

in any arbitrary position depending upon the point of application 
of the bow. A similar fixity of the nodal system occurs, in spite 
of the variable €, when a is so chosen that cos na » or sin na =s 0. 
But in general there is no fixed nodal system. When e is a 
multiple of 2v, that is when the two vibrations are restored to 
the same phase, there is a nodal system represented by (3). And 
when € is an odd multiple of v, so that the two vibrations are in 
opposite phases, we have in place of (2) 

8inn(tf +a)cosp^ (4), 

with a nodal system 

^ = -.a + m('7r/n) (5). 

In these cases there is a nodal system, and in a sense the system 
may be said to oscillate between the positions given by (3) and (5) ; 
but it must not be overlooked that at intermediate times there is 
no true nodal system at all Thus, when e = Jtt, (1) becomes 

cos na sin nO co& pt + sin na cos nO sin pt 

The squared amplitude of this motion is 

cos' na sin' n0 + sin* na cos* nO, 

a quantity which does not vanish for any value of 0. In general 
the squared amplitude is 

cos* na sin* nO -f sin* na cos* wtf - 2 cos na sin na cos n0 sin n0 cos 6, 

or, as it may also be written, 

^ — ^cos2na cos'2n0 — ^sin2na sin 2n0 cose (6). 

This quantity is a maximum or a minimum when 

tan 2n0 = cos€ tan2na (7). 

The minimum of motion thus oscillates backwards and forwards 
between tf = + a and 5 « — a ; but as we have seen, it is only in 
these extreme positions that the minimum is zero. 

A like phenomenon occurs during the fi^ee vibrations of a 
circular membrane, or in fact of any system of revolution such 
that the position of nodal lines is arbitrary so long as the 
symmetry is complete.] 

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The two other cases of a circular plate in which the edge 
is either clamped or supported would be easier than the preceding 
in their theoretical treatment, but are of less practical interest on 
account of the difficulty of experimentally realising the conditions 
assumed The general result that the nodal system is composed 
of concentric circles, and diameters symmetrically distributed, is 
applicable to all the three cases. 

221a. The use in the telephone of a thin circular plate 
clamped at the edge lends a certain interest to the calculation of 
the periods and modes of vibration W such a plate. It will suffice 
to consider the symmetrical modes. 

By (5) § 218 we may take as representing the motion in 
this case 

w = Jo(*r) + \Jo(i*r) = Jp(tr) + \7o(A?r)^ (1), 

from which 

^^Jo'{kr) + %\J,'{ikr)^^J,(kT) + \I,(kr) (2>, 

where we write 

/oW = /oW = l+| + 2rV» + W. 

z ^ ^ 
Ii{z) =iJo'(tz) = 2 ■*" 2«T4 ■*■ 2«T4V:5 "*" ^^^ 

Since the plate is clamped at r^a, both w and dw/dr must 
there vanish. Hence, writing ka — z, we get as the frequency 

^i^U[^^,^0 (5). 

In (5) /i and Iq are both positive, so that the signs of Ji and J^ 
must be opposite. Hence by Table B § 206 the first root most 
lie between 2*4 and 3*8, the second between 5*5 and 7*0, and 
so on. The values of the earlier roots might be obtained without 
much difficulty from the series for /© and /i by using the table 
§ 200 for Jo and Ji ; but it will be convenient for the present and 
further purposes to give a short table ^ of the functions /« and /i 
themselves. For large values of the argument descending series, 
analogous to (10) § 200, may be employed. 

1 Calculated by A. Lodge, Brit. Ass. Rep., 18S9. 

Digitized by 










AW ' 





0-0000 1 






-1005 , 


















•4329 ; 






•5662 ' 


















1-0848 ' 






1-3172 , 






1-5906 ' 


















2-7554 , 















The first root of (o) is z = 3-20. This then is the value of ka 
for the gravest symmetrical vibration. The next value of 2^ is 
about 6*3. Since the fi-equency varies as A;* (§ 217), the interval 
between the tones is nearly two octaves. 

Returning to the first root, we have for the frequency (n) 


^ p ^ (3-2)«c' ^ (3-2) V g. A 

27r 27ra* 2iraW3p (1 - /a«) ^^^' 

This is the general formula. For rough calculations fi* in the 
denominator may be omitted. If for the case of iron we take 

p = 7-7, gr = 20xlOi«, 

2-4xlO».2A _ 

— r 0)> 

we find 

n = 

2A and a being expressed in centimetres. 

A telephone plate measured by the author gave 

a = 2-2, 2A = -020. 
According to these values 

n = 991 vibrations per second 

222. We have seen that in general Chladni's figures as traced 
by sand agree very closely with the circles and diameters of 
theory; but in certain cases deviations occur, which are usually 
attributed to irregularities in the plate. It must however be re- 

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membered that the vibrations excited by a bow are not Btrictif 
speaking free, and that their periods are therefore liable to a 
certain modification. It may be that under the action of the bow 
two or more normal component vibrations coexist. The whole 
motion may be simple harmonic in virtue of the external force, 
although the natural periods would be a little different. Such an 
explanation is suggested by the regular character of the figures 
obtained in certain cases. 

Another cause of deviation may perhaps be found in the 
manner in which the plates are supported. The requirementB of 
theory are often difficult to meet in actual experiment When 
this is so, we may have to be content with an imperfect compari- 
son ; but we must remember that a discrepancy may be the fiuilt 
of the experiment as well as of the theory. 

[In the ordinary use of sand to investigate the vibratioDS of 
flat plates and membranes the movement to the nodes is irregular 
in its character. If a grain be situated elsewhere than at a node, 
it is made to jump by a sufficiently vigorous transverse vibration. 
The result may be a movement either towards or from a node; 
but after a succession of such jumps the grain ultimately finds its 
way to a node as the only place where it can remain undisturbed. 
Grains which have already arrived at a node remain there, while 
others are constantly shifting their position. 

It was found by Savart that very fine powder, such as lyoo- 
podium, behaves differently from sand. Instead of collecting at 
the nodes, it heaps itself up at the places of greatest motion. 
This effect was traced by Faraday^ to the influence of currents of 
air, themselves the result of the vibration. In a vacuum all 
powders move to the nodes. 

In some cases the movement of sand to the nodes, or to some 
of them, takes place in a more direct manner as the result of 
friction. Thus, in his investigation of the longitudinal vibrations 
of thin narrow strips of glass, held horizontally, Savart' observed 
the delineation of nodes apparently dependent upon an aooom- 
paniment of vibrations of a transverse character. The special 
peculiarity of this phenomenon was the non-correspondence of the 
lines traced by sand upon the two faces^ of the glass when tested 

^ On a Peoaliar CIebb of Aconstioal Figures, Phil. Trcau., ISSl, p. 299. 
s Ann. d. Chim,, vol. 14, p. 118, 1820. 

Digitized by 




222.] SAV art's obsebvations. 369 

in succession, a fistct sufficient to shew that the transverse motion 
was connected with a failure of uniformity. In consequence of 
this there are developed transverse vibrations of the same (high) 
pitch as that of the principal longitudinal motion, and therefore 
attended with many nodes. These nodes are of course the same 
whichever &ce of the glass is uppermost, and it might be supposed 
that they would all be indicated by the sand, as would happen if 
the transverse vibrations existed alone. But the combination of 
the two kinds of motion causes a creeping of the sand towards the 
alternate nodes, the movements of the sand at corresponding 
points on the two sides of the plate being always in opposite 
directions. On the one side an inwards longitudinal motion (for 
example) is attended by an upwards transverse motion, but when 
the plate is reversed the same inwards longitudinal motion is 
associated with a transverse motion directed downwards. If there 
were no transverse motion, the longitudinal force upon any 
particle resulting from friction would vanish in the long run, but 
in consequence of the transverse motion this balance is upset, and 
in a manner different upon the two sides of the plate. The above 
considerations appear to afford sufficient ground for an explanation 
of the remarkable phenomenon observed by Savart, but an attempt 
to follow the matter further into detail would lead us too 

223. The first attempt to solve the problem with which we 
have just been occupied is due to Sophie Germain, who succeeded 
in obtaining the correct differential equation, but was led to 
erroneous boundary conditions. For a free plate the latter part of 
the problem is indeed of considerable difficulty. In Poisson's 
memoir 'Sur T^uilibre et le mouvement des corps ^lastiquesV 
that eminent mathematician gave three equations as necessary to be 
satisfied at all points of a free edge, but Eirchhoff has proved that 
in general it would be impossible to satisfy them alL It happens, 
however, that an exception occurs in the case of the symmetrical 
vibrations of a circular plate, when one of the equations is true 
identically. Owing to this peculiarity, Poisson's theory of the 
symmetrical vibrations is correct, notwithstanding the error in his 
view as to the boundary conditions. In 1850 the subject was 

^ See Terqnem, (7. R., xlyi., p. 776, 185S. 
' MSm. de VAcad. d. Sc. ft Par. 1829. 

B. 24 

Digitized by VjOOQIC 




resumed by Kirchhoff ^ who first gave the ttvo equations approprii 
to a free edge, and completed the theory of the vibrations ol 
circular disc. 

224. The correctness of Elirchhoff's boundary equations 1 
been disputed by Mathieu*, who, without explaining where 
considers KirchhoflTs error to lie, has substituted a different set 
equations. He proves that if u and u be two normal functions, 
that w = u cos pt, w = u'co9p't are possible vibrations, then 

(p^ — p'*) 1 1 uu'dxdy 

, dV^u -, du* ^^ ,du ^ dV»w' 
an dn an a< 



This follows, if it be admitted that u, u ssatisfy respectiv< 
the equations 

Since the left-hand member is zero, the same must be true 
the right-hand member; and this, according to Mathieu, cani 
be the case, unless at all points of the boundai^ both u and 
satisfy one of the four following pairs of equations : 

u «0 



V»tt =0 



u =0 

P ^0 


dn " 

The second pair would seem the most likely for a free edge, b 
it is found to lead to an impossibility. Since the first and thi 
pairs are obviously inadmissible, Mathieu concludes that the foui 
pair of equations must be those which really express the conditi 
of a free edge. In his belief in this result he is not shaken by t 
fact that the corresponding conditions for the free end of a I 
would be duldx = 0, d^u/da:^ = Oj the first of which is contradict 
by the roughest observation of the vibration of a large tunin 

^ Crelle, t. xl. p. 51. Ueber das Gleichgewicbt und di« Bewegang eiuer eli 
tiscben Scheibe. 

' LiouviUe, t. xiv. 1S69. 

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The &^t is that although any of the four pairs of equations 
would secure the evanescence of the boundary integral in (1), it 
does not follow conversely that the integral can be made to vanish 
in no other way; and such a conclusion is negatived by KirchhofiTs 
investigation. There are besides innumerable other cases in 
which the integral in question would vanish, all that is really 
necessary being that the boundary appliances should be either at 
rest, or devoid of inertia. 

226. The vibrations of a rectangular plate, whose edge is 
supported^ iMiy be easily investigated theoretically, the normal 
functions being identical with those applicable to a membrane of 
the same shape, whose boundary is fixed. If we assume 

w = sm- sm -r^ (io^pt (1), 

we see that at all points of the boundary, 

w = 0, d^wlda^ « 0, d^wfdf = 0, 

which secure the fulfilment of the necessary conditions (§ 215). 
The value of p, found by substitution in c^V^w^^p^w^ 

- ^-«^nf + (2). 

shewing that the analogy to the membrane does not extend to the 
sequence of tones. 

It is not necessary to repeat here the discussion of the primary 
and derived nodal systems given in Chapter ix. It is enough to 
observe that if two of the fundamental modes (1) have the same 
period in the case of the membrane, they must also have the same 
period in the case of the plate. The derived nodal systems are 
accordingly identical in the two cases. 

The generality of the value of w obtained by compounding 
with arbitrary amplitudes and phases all possible particular solu- 
tions of the form (1) requires no fresh discussion. 

Unless the contrary assertion had been made, it would have 
seemed unnecessary to say that the nodes of a supported plate 
have nothing to do with the ordinary Chladni's figures, which 
belong to a plate whose edges are free. 


Digitized by VjOOQ IC 




The realization of the conditions for a supported edge 
scarcely attainable in practice. Appliances are required capa 
of holding the boundary of the plate at rest, and of such a nat 
that they give rise to no couples about tangential axes. We u 
conceive the plate to be held in its place by friction against 
walls of a cylinder circumscribed closely round it. 

The problem of a rectangular plate, whose edges 
free, is one of great difficulty, and has for the moiSt part resis 
attacks If we suppose that the displacement w is indepeud 
of y, the general diflferential equation becomes identical with tl 
with which we were concerned in Chapter vrii. If we take 
solution corresponding to the case of a bar whose ends are ii 
and therefore satisfying dhu/da^^O, d*w/dx^ = 0, when ^ = * 
when a? = a, we obtain a value of w which satisfies the gene 
di£ferential equation, as well as the pair of boundary equatious 


d^w .« .d^w] ^\ 


d^w ^ \ 


which are applicable to the edges parallel to y ; but the sect 
boundary condition for the other pair of edges, namely 

d^w d*w ^ 



will be violated, unless /a==0. This shews that, except in 
case reserved, it is not possible for a free rectangular plate 
vibrate after the manner of a bar; unless indeed as an approxii 
tion, when the length parallel to one pair of edges is so great t 
the conditions to be satisfied at the second pair of edges may 
left out of account. 

Although the constant fi (which expresses the ratio of lat< 
contraction to longitudinal extension when a bar is drawn c 
is positive for every known substance, in the case of a few s 
stances — cork, for example — it is comparatively verj* smalL Th 
is, so far as we know, nothing absurd in the idea of a subsU 

* [The oase where two opposite edges are firee while the other two edges 
supported, has been diaoussed by Voigt {Gdttingen Nachncht^n, 1893).] 

Digitized by 



for which /a vanishes. The investigation of the problem under 
this condition is therefore not devoid of interest, though the results 
will not be strictly applicable to ordinary glass or metal plates, 
for which the value of /i is about ^} 

If 111, t£„ &c. denote the normal functions for a free bar inves- 
tigated in Chapter viiL, corresponding to 2, 3, nodes, the 

vibrations of a rectangular plate will be expressed by 

w^Ui {xja), w = U2 (x/a), &c., 

or w = Ml (y/6), w = ii, (y/6), &c. 

In each of these primitive modes the nodal system is composed 
of straight lines parallel to one or other of the edges of the 
rectangle. When b^a, the rectangle becomes a square, and the 

w = Un (x/a), w^Un (jz/a), 

having necessarily the same period, may be combined in any pro- 
portion, while the whole motion still remains simple harmonic. 
Whatever the proportion may be, the resulting nodal curve will of 
necessity pass through the points determined by 

Un {xja) = 0, On (y/a) = 0. 

Now let us consider more particularly the case of n = 1. The 
nodal system of the primitive mode, w — u^ (xja), consists of a 
pair of straight lines parallel to y, whose distance from the nearest 
edge is '2242 a. The points in which these lines are met by the 
corresponding pair for w = tij (y/a), are those through which the 
nodal curve of the compound vibration must in all cases pass. It 
is evident that they are symmetrically disposed on the diagonals 
of the square. If the two primitive vibrations be taken equal, 
but in opposite phases (or, algebraically, with equal and opposite 
amplitudes), we have 

w= t*i (x/a) - Ui (y/a) (3), 

^ In order to make a plate of material, for which ft is not zero, vibrate in the 
manner of a bar, it would be necessary to apply constraining couples to the edges 
parallel to the plane of bending to prevent the assumption of a contrary curvature. 
The effect of these couples would be to raise the pitch, and therefore the calcu- 
lation founded on the type proper to /tsQ would give a result somewhat higher in 
pitch than the truth. 

Digitized by 





from which it is evident that w vanishes when a? = y, that is alo 

the diagonal which passes through the origin. f%, n. 

That w will also vanish along the other diagonal 

follows from the symmetry of the functions, and 

we conclude that the nodal system of (3) comprises 

both the diagonals (Pig. 41). This is a well-known 

mode of vibration of a square plate. 

A second notable case is when the amplitudes are equal ai 
their phases the same, so that 

w = Ui{x/a)'^tti(y/a) ,„(4). 

The most convenient method of constructing graphical 
the curves, for which t(; = const., is that employed by Maxwi 
in similar cases. The two systems of curves (in this install 
straight lines) represented by t^ (x/a) = const., t(i (yfa) = canst,, a 
first laid down, the values of the constants forming an arit 
metical progression with the same common diflFerence in the u 
cases. In this way a network is obtained which the requir 
curves cross diagonally. The execution of the proposed pb 
requires an inversion of the table given in Chapter VUL, § 17 
expressing the march of the function Ui, of which the lesult is 
follows : — 


X : a 


X : a 

+ 1O0 


- -25 




















The system of lines represented by the above values of jr (C4)i] 
pleted symmetrically on the ftirther side of the central line) an 
the corresponding system for y are laid down in Fig. 42, Froi 
these the curves of equal displacement are deduced; At tl 
centre of the square we have w a maximum and equal to 2 on tl 
scale adopted. The first curve proceeding outwards is the locits < 
points at which w = 1. The next is the nodal line, separating th 
regions of opposite displacement. The remaining curves taken i 

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order give the displacements — 1, — 2, — 3. The numerically great- 
est negative displacement occurs at the comers of the square, 
where it amounts to 2 x 1-645 = 3-290.* 

The nodal curve thus constructed agrees pretty closely with the 
observations of Strehlke '. His results, which refer to three care- 
fully worked plates of glass, are embodied in the following polar 
equations : 

-40143 01711 00127^ 

r = -40143 + -01721 cos 4t + '00127 > cos 8i, 
-4019 -Oiesj '0013 J 





- -■ J2 _,Z 


^ !i- '/\ 

- A^ -,Z 

N. W 

.-Zt JZ. 


V- ^ ^ 



\/ \/ 

T ^'^~ 7^ 

S. Z^^ 7^ 

5/ S/ - 

7 2\~" 


_7S^ /S^. 

7 J- ^- 



Z H \ 

f 1 7 



\ /\ c 

I ' 



^ Y 



}\ A 

s___S_ S 


Z \Z..v 

.S± ^ 1 



\. Z\ Ti 

- S S^ 


\^ ^^ - 

- s^^zS^ 

-S2.\ J2S . 

V 5^ ^ 

Z :^7 "S,i 

-S zs 



yv y^ 

- ^2 S^ 


JZ. SZ . 

.J2.\^ S_ 

-^Z ^1\ 





the centre of the square being pole. From these we obtain for 
the radius vector parallel to the sides of the square (t = 0) -41980, 

1 On the nodal lines of a sqoare plate. Phil. Mag. Angast, 1878. 
« Pogg. Ann, Vol. cxlvi. p. 819, 1872. 

Digitized by 



'419S1, '4200, while the calculated result b '4154. The rs 
vector measured along a diagonal is '3856, ^S855, '3864, an* 
calculation 3900* 

By crossing the network in the other direction we ohtaiE 
locus of points for which w^ (^r/a) — lii (y/a) is constant, which 

the curves of constant displacement for that mode in which 
diagonals are nodal. The pitch of the vibration is (accordit 
theory) the aame in both cases. 

Fig* 43. 


















The primitive modes represented by w — w^ (jaja) or w = «, 
may be combined in like manner. Fig 43 shews the nodal c 
for the vibration 

m - n^ixfa) ± u^ (y/a) .,•*,.,*....., ,.( 

The form of the curve is the same relatively to the other dia^ 
if the sign of the ambiguity be altered. 

Digitized by 


227.] wheatstone's figures. 377 

227. The method of superposition does not depend for its 
application on any particular form of normal function. Whatever 
the form may be, the mode of vibration, which when /a = 
passes into that just discussed, must have the same period, 
whether the approximately straight nodal lines are parallel to 
a? or to y. If the two synchronous vibrations be superposed, 
the resultant has still the same period, and the general course 
of its nodal system may be traced by means of the considera- 
tion that no point of the plate can be nodal at which the 
primitive vibrations have the same sign. To determine exactly 
the line of compensation, a complete knowledge of the primitive 
normal functions, and not merely of the points at which they 
vanish, would in general be necessary. Doctor Young and the 
brothers Weber appear to have had the idea of superposition as 
capable of giving rise to new varieties of vibration, but it is to Sir 
Charles Wheatstone ^ that we owe the first systematic application 
of it to the explanation of Chladni's figures. The results actually 
obtained by Wheatstone are however only very roughly applicable 
to a plate, in consequence of the form of normal function implicitly 
assumed. In place of Fig. 42 (itself, be it remembered, only an 
approximation) Wheatstone finds for the node of the compound 
vibration the inscribed square shewn in Fig. 44. 
This form is really applicable, not to a plate vi- 
brating in virtue of rigidity, but to a stretched 
membrane, so supported that every point of the 
circumference is firee to move along lines perpen- 
dicular to the plane of the membrane. The 
boundary condition applicable under these circumstances is 

, «s ; and it is easy to shew that the normal functions which 

involve only one co-ordinate are 

w = cos (mTTir/a), or w^ cos (wiry /a), 

the origin being at a comer of the square. Thus the vibration 

2'n'X 2'7rt/ ,,. 

WssCOS +COS — ~ (1) 

has its nodes determined by 

7r(a?H-y) 'rr{x — y) ^ 

cos ^ cos ^- = 0, 

a a 

1 PUL Trans. 1838. 

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whence X'\-y = ^a or |a, or x — y=^±^a, equations whi( 
represent the inscribed square. 


2irx 2iry 

= ooa — nna — ^ 

t(; = cos 



the nodal system is composed of the two diagouals. This resu 
which depends only on the symmetry of the normal functions, 
strictly applicable to a square plate. 

When m = 3, 

w =5 cos h cos — ^ 

a a 

and the equations of the nodal lines are 


^ + y=g, a, g, 

^-y = ±g, 

Fig. 4^, 

shewn in Fig. 45. If the other sign be taken, we 
obtain a similar figure with reference to the other 

When m = 4, 

4BTrx 4nry 

w = cos + cos — ~ . 

a a 


giving the nodal lines 
_a 3a ba 7a 

"^^^""4' T' T' T' 

a.-y = ±i, ±x(Fig^*C). 

With the other sign 

we obtain 

w =s cos cos — - 

a a 

a;+y = |. a.^, ar-y = 0, ± | (Fig. 47) 

representing a system composed of the diagonals, 
together with the inscribed square. 

These forms, which are strictly applicable to the membran 
resemble the figures obtained by means of sand on a square pkl 
more closely than might have been expected. The sequence ( 
tones is however quite different. From § 176 we see that, if fi wei 
zero, the interval between the form (43) derived from thre 
primitive nodes, and (41) or (42) derived from two, would b 


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1"4629 octaves; and the interval between (41) or (42) and (46) or 
(47) would be 2*4358 octaves. Whatever may be the value of jj, the 
forms (41) and (42) should have exactly the same pitch, and the 
same should be true of (46) and (47). With respect to the first- 
mentioned pair this result is not in agreement with Chladni's 
observations, who found a difference of more than a whole tone, 
(42) giving the higher pitch. If however (42) be leffc out of 
account, the comparison is more satisfactory. According to theory 
(m = 0), if (41) gave d, (43) should give ^r'-, and (46), (47) 
should give /' + . Chladni found for (43) g't + , and for (46), 
(47) g'% and ^'t-^ respectively. 

2128. The gravest mode of a square plate has yet to be consi- 
dered The nodes in this case are the two lines drawn through the 
middle points of opposite sides. That there must be such a mode 
will be shewn presently from considerations of symmetry, but 
neither the form of the normal function, nor the pitch, has yet 
been determined, even for the particular case of /Li => 0. A rough 
calculation however may be -founded on an assumed tjrpe of 

If we take the nodal lines for axes, the form w^xy satisfies 
V^w = 0, as well as the boundary conditions proper for a free edge 
at all points of the perimeter except the actual comers. This is 
in fact the form which the plate would assume if held at rest by 
four forces numerically equal, acting at the comers perpendicu- 
larly to the plane of the plate, those at the ends of one diagonal 
being in one direction, and those at the ends of the other diagonal 
in the opposite direction. From this it follows that w^xycospt 
would be a possible mode of vibration, if the mass of the plate 
were concentrated equally in the four comers. By (3) § 214, we 
see that 

^-30T^)'''P' ^^>' 

inasmuch as 

d^w/dx^ = cPw/dy^ = 0, d^wjdxdy = cos^^^ 

For the kinetic energy, if p be the volume density, and M the 
additional mass at each comer, 

T=^f sin*^ U^ ""T " iphahj^dxdy + Jifa*l 

■.W^.^pt[^\ + %M] (2). 


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l_p(l +M)a «/, ^qM\ 


where J/' denotes the mass of the plate without the loads. Th 
result tends to become accurate when M is relatively great ; othe 
wise by § 89 it is sensibly less than the truth. But even whi 
M — Q, the error is probably not very great. In this case s 
should have 

,^ 96qh^ 

p(l+M)a* " 



giving a pitch which is somewhat too high. The gravest mo 
next after this is when the diagonals are nodes, of which the pitx 
if ^ = 0, would be given by 

,,_qh^ (4-7300y 

|)- = 

(see §174). 



We may conclude that if the material of the plate were su 
that ft=0, the interval between the two gravest tones woi 
be somewhat greater than that expressed by the ratio VZ 
Chladni makes the interval a fifth. 


Fig. 48. 

229. That there must exist modes of vibration in whi 
the two shortest diameters are nodes may be 
inferred from such considerations as the following. 
In Fig. (48) suppose that GH is a plate of which 
the edges HO, GO are supported, and the edges 
QC, GH free. This plate, since it tends to a 
definite position of equilibrium, must be capable 
of vibrating in certain fundamental modes. Fixing 
our attention on one of these, let us conceive a 
distribution of w over the three remaining quadrants, such that 
any two that adjoin, the values of w are equal and opposite 
points which are the images of each other in the line of separati 
If the whole plate vibrate according to the law thus deterrain 
no constraint will be required in order to keep the lines GE, i 
fixed, and therefore the whole plate may be regarded 2^ free. T 
same argument may be used to prove that modes exist in whi 
the diagonals are nodes, or in which both the diagonals and t 
diameters just considered are together nodal. 

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The principle of symmetry may also be applied to other forms 
of plate. We might thus infer the possibility of nodal diameters 
in a circle, or of nodal principal axes in an ellipse. When the 

Fig. 49. Fig. 50. Fig. 51. 

boundary is a regular hexagon, it is easy to see that Figs. (49), 
(50), (51) represent possible forms. 

It is interesting to trace the continuity of Chladni's figures, as 
the form of the plate is gradually altered. In the circle, for 
example, when there are two perpendicular nodal diameters, it is a 
matter of indifference as respects the pitch and the type of vibra- 
tion, in what position they be taken. As the circle develops into 
a square by throwing out comers, the position of these diameters 
becomes definite. In the two alternatives the pitch of the vibra- 
tion is different, for the projecting comers have not the same effi- 
dencj in the two cases. The vibration of a square plate shewn in 
Fig. (42) corresponds to that of a circle when there is one circular 
node. The correspondence of the graver modes of a hexagon or 
an ellipse with those of a circle may be* traced in like manner. 

230. For plates of uniform material and thickness and of 
invariable shape, the period of the vibration in any fundamental 
mode varies as the square of the linear dimension, provided of 
course that the boundary conditions are the same in all the cases 
compared. When the edges are clamped, we may go further 
and assert that the removal of any external portion is attended 
by a rise of pitch, whether the material and the thickness be 
uniform, or not. 

Let AB be a part of a clamped edge (it is of no consequence 
whether the remainder of the boundary be clamped, or not), and 

Fig. 52. 

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let the piece ACBD be removed, the new edge ADB being also 
clamped. The pitch of any fundamental vibration is sharper 
than before the change. This is evident, since the altered 
vibrations might be obtained from the original system by the 
introduction of a constraint clamping the edge ADB. The effect 
of the constraint is tq raise the pitch of every component, and 
the portion ACBD being plane and at rest throughout the motion, 
may be removed. In order to follow the sequence of changes 
with greater security from error, it is best to suppose the line 
of clamping to advance by stages between the two positions 
ACB, ADB. For example, the pitch of a uniform clamped plate 
in the form of a regular hexagon is lower than for the inscribed 
circle and higher than for the circumscribed circle. 

When a plate is free, it is not true that an addition to 
the edge always increases the period. In proof of this it may be 
sufficient to notice a particular case. 

AB IB B, narrow thin plate, itself without inertia but carrying 
loads B,t A, By C. It is clear that the addition to the breadth 

Fig. 58. 

•A •€ B* 

indicated by the dotted line would augment the stiffness of the 
bar, and therefore lessen the period of vibration. The same 
consideration shews that for a uniform free plate of given area 
there is no lower limit of pitch ; for by a sufficient elongation 
the period of the gravest component may be made to exceed 
any assignable quantity. When the edges are clamped, the 
form of gravest pitch is doubtless the circle. 

If all the dimensions of a plate, including the thickness, be 
altered in the same proportion, the period is proportional to the 
linear dimension, as in every case of a solid body vibrating in 
virtue of its own elasticity. 

The period also varies inversely as the square root of Young s 
modulus, if /^ be constant, and directly as the square root of the 
mass of unit of volume of the substance. 

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231.] CYLINDER OF RING. 383 

231. Experimenting with square plates of thin wood whose 
gfain ran parallel to one pair of sides, Wheatstone^ found that 
the pitch of the vibrations was different according as the ap- 
proximately straight nodal lines were parallel or perpendicular 
to the fibre of the wood. This effect depends on a variation 
in the flexural rigidity in the two directiona The two sets of 
vibrations having different periods cannot be combined in the 
usual manner, and consequently it is not possible to make such 
a plate of wood vibrate with nodal diagonals. The inequality 
of periods may however be obviated by altering the ratio of the 
sides, and then the ordinary mode of superposition giving nodal 
diagonals is again possible. This was verified by Wheatstone. 

A further application of the principle of superposition is due 
to Eonigl In order that two modes of vibration may combine, 
it is only necessary that the periods agree. Now it is evident 
that the sides of a rectangular plate may be taken in such a 
ratio, that (for instance) the vibration with two nodes parallel 
to one pair of sides may agree in pitch with the vibration having 
three nodes parallel to the other pair of sides. In such a case 
new nodal figures arise by composition of the two primary modes 
of vibration. 

232. When the plate whose vibrations are to be considered 
is naturally curved, the difficulties of the question are generally 
much increased. But there is one case in which the complication 
due to curvature is more than compensated by the absence of a 
free edge ; and this case happens to be of considerable interest, as 
being the best representative of a bell which admits of simple 
analjrtical treatment. 

A long cylindrical shell of circular section and uniform thick- 
ness is evidently capable of vibrations of a fiexural character 
in which the axis remains at rest and the surface cylindrical, 
while the motion of every part is perpendicular to the generating 
lines. The problem may thus be treated as one of two dimensions 
only, and depends upon the consideration of the potential and 
kinetic energies of the various deformations of which the section 
is capable. The same analysis also applies to the corresponding 
vibrations of a ring, formed by the revolution of a small closed 
area about an external axis (§ 192 a). 

1 Phil Trans. 1833. 

> Pogg. Ann. 1884, cxzn. p. 238. 

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The cylinder, or ring, is susceptible of two classes of vibrati< 
depending respectively on extensibility and flexural rigidity, b 
analogous to the longitudinal and lateral vibrations of strai^ 
bars. When, however, the cylinder is thin, the forces resisti 
bending become small in comparison with those by which < 
tension is opposed; and, as in the case of straight bars, 1 
vibrations depending on bending are graver and more imports 
than those which have their origin in longitudinal rigidi 
In the limiting case of an infinitely thin shell (or ring), i 
flexural vibrations become independent of any extension of 1 
circumference as a whole, and may be calculated on the s\ 
pasition that each part of the circumference retains its nain 
length throughout the motion. 

But although the vibrations about to be considered 
analogous to the transverse vibrations of sti-aight bars in resp 
of depending on the resistance to flexure, we must not fall i 
the common mistake of supposing that they ai-e exclu&iv 
normal. It is indeed easy to see that a motion of a cylinder 
ring in which each particle is displaced in the direction of 
radius would be incompatible with the condition of no extensi 
In order to satisfy this condition it is necessary to ascribe 
each part of the circumference a tangential as well as a non 
motion, whose relative magnitudes must satisfy a certain diri 
ential equation. Our first step will be the investigation of i 

233. The original radius of the circle being a, let the eq 
librium position of any element of the circumference be defii 
by the vectorial angle 0. During the motion let the polar 
oi-dinates of the element become 

If da represent the arc of the deformed curve corresponding to a 
we have 

(ds)» = (ad0y = (dSry + r« (dtf + dhOy ; 

^vhence we find, by neglecting the squares of the small quanti 
Si , B0, 

Sr dh0 ^ 

7 + W=^- (^ 

as the required relation. 

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In whatever manner the original circle may be deformed at 
time t, Sr may be expanded by Fourier's theorem in the series 

-^ A,coa 80 '\- B,8m 80 + ...} (2), 

and the corresponding tangential displacement required by the 
condition of no extension will be 

A B 
B0 ==-Aiam0 + B,co80 +...--- sin 80 -¥ — coa 80 - (3), 


the constant that might be added to S0 being omitted. 

If (rad0 denote the mass of the element ad0, the kinetic 
energy T of the whole motion will be 

+ (l + i)(i/ + 5/) + ...| (4). 

the products of the co-ordinates A,, B, disappearing in the 

We have now to calculate the form of the potential energy V. 
Let p be the radius of curvature of any element ds ; then for the 
corresponding element of V we may take i^Bds {S (1/p)}*, where 
£ is a constant depending on the material and on the thickness. 


r=^Bar(B-yd0 (5). 

u =s - =3 - {1 — ilj cos ^ — 5i sin ^ — ... }, 

for in the small terms the distinction between ^ and may be 


8 - = - 2 {(«» - 1) {A, cos 8^ + B, sin a<^)}, 


B. 25 

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F= ^ p {2 («» - 1) {A, COS80 + B, sin s$}Y d6 

= ^^2(«'-l)'(^' + 5.') (6 

in which the summation extends to all positive integral val 
of 8. 

The term for which « = 1 contributes nothing to the poten 
energy, as it corresponds to a displacement of the cLrcIe as a wh 
without deformation. 

We see that when the configuration of the system is defined 
above by the co-ordinates -4i, -Bi, &c., the expressions for Taiic 
involve only squares; in other words, these are the n&ritwl 
ordinates, whose independent harmonic variation expresses 
vibration of the system. 

If we consider only the terms involving cos s8, sin s8, we hi 
by taking the origin of 6 suitably, 


8r = ail. cos «tf, Stf = -misd (7) 


while the equation defining the dependence of A^ upon 
time is 

<ra'(l+^)i>^(«'-l)'A = (8J 

from which we conclude that, if A, varies as cos (pi — c)» 

P^ = ^-«'T1- <^' 

This result was given by Hoppe for a ring in a memoir p 
lished in Crelle, Bd. 63, 1871. His method, though more conipl 
than the preceding, is less simple, in consequence of his not 
cognising explicitly that the motion contemplated corresponds 
complete inextensibility of the circumference. 

[In the application of (9) to a ring we have, § 192 a, 

^-p.... ...(10) 

where q is Young's modulus, p the volume density, and c i 

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radius of the circular section. For the cylindrical shell, (18) 
§ 235 g, 

a '*3(m + n)p ^ ^' 

2h denoting the thickness, and m, n the elastic constants in 
Thomson and Tait's notation.] 

According to Chladni the firequencies of the tones of a ring 
are as 

3» : 5» : 7« : 9« 

If we refer each tone to the gravest of the series, we find for 
the ratios characteristic of the intervals 

2-778, 5-446, 9, 13-44, &c. 

The corresponding numbers obtained from the above theoretical 
formula (9), by making 8 successively equal to 2, 3, 4, &c., are 

2-828, 5-423, 8-771, 1287, &c., 

agreeing pretty nearly with those found experimentally. 

[Observations upon the tones of thin metallic cylinders, open 
at one end, have been made by Fenkner \ Since the pitch proved 
to be very nearly independent of the height of the cylinders, the 
vibrations may be regarded as approximately two-dimensional. 
In accordance with (9), (11), Fenkner found the frequency propor- 
tional to the thickness directly, and to the square of the radius 
inversely. As regards the sequence of tones from a given 
cylinder *, the numbers, referred to the gravest (« = 2) as unity, 
were 2*67, 5-00, 800, 1200, &c. The agreement with (9) would 
be improved if these numbers were raised by about -j^ part, 
equivalent to an alteration in the pitch of the gravest tone. 

The influence of rotation of the shell about its axis has been 
examined by Bryan*. It appears that the nodes are carried 
round, but with an angular velocity less than that of the rotation. 
If the latter be denoted by o), the nodal angular velocity is 

^-1 T 

1 Wied, Arm. vol. S, p. 186, 1879. 

s Melde, Akustih, Leipzig, 1883, p. 228. 

8 Proc. Camb. Phil. Soc. vol. vn. p. 101, 1890. 


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234. When s^l, the frequency is zero, as might have been 
anticipated. The principal mode of vibration corresponds to ^^2, 
and has four nodes, distant from each other by 90^. These so- 
called nodes are not, howeyer, places of absolute rest, for the 
tangential motion is there a maximum. In fact the tangential 
vibration at these points is half the maximum normal motion. 
In general for the ^ term the maximum tangential motion is 
(l/s) of the maximum normal motion, and occurs at the nodes of 
the latter. 

When a bell-shaped body is sounded by a blow, the point of 
application of the blow is a place of maximum normal motion 
of the resulting vibrations, and the same is true when the 
vibrations are excited by a violin-bow, as generally in lecture- 
room experiments. Bells of glass, such as finger-glasses, are 
however more easily thrown into regular vibration by friction with 
the wetted finger carried round the circumference. The pitch of 
the resulting sound is the same as of that elicited by a tap with 
the soft pait of the finger; but inasmuch as the tangential motion 
of a vibrating bell has been very generally ignored, the production 
of sound in this manner has been felt as a difficulty. It is now 
scarcely necessary to point out that the effect of the friction is in 
the first instance to excite tangential motion, and that the point 
of application of the friction is the place where the tangential 
motion is greatest, and therefore where the normal motion 

236. The existence of tangential vibration in the case of a bell 
was verified in the following manner. A so-called air-pump re- 
ceiver was securely fastened to a table, open end uppermost, and set 
into vibration with the moistened finger. A small chip in the rim, 
reflecting the light of a candle, gave a bright spot whose motion 
could be observed with a Coddington lens suitably fixed. As the 
finger was carried round, the line of vibration was seen to in- 
volve with an angular velocity double that of the finger; and 
the amount of excursion (indicated by the length of the line of 
light), though ^'ariable, was finite in every position. There was, 
however, some difficulty in observing the correspondence between 
the momentary direction of vibration and the situation of the point 
of excitement. To effect this satisfactorily it was found necessair 
to apply the friction in the neighbourhood of one point It then 
became evident that the spot moved tangentially when the bell was 

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excited at poiDts distant therefrom 0, 90, 180, or 270 degrees ; and 
normally when the friction was applied at the intermediate points 
corresponding to 45, 135, 225 and 315 degrees. Care is sometimes 
required in order to make the bell vibrate in its gravest mode 
without sensible admixture of overtones. 

If there be a small load at any point of the circumference, 
a slight augmentation of period ensues, which is different accord- 
ing as the loaded point coincides with a node of the normal or 
of the tangential motion, being greater in the latter case than 
in the former. The sound produced depends therefore on the 
place of excitation; in general both tones are heard, and by 
interference give rise to beats, whose frequency is equal to the 
difference between the frequencies of the two tones. This phe- 
nomenon may often be observed in the case of large bells. 

236 a. In determining the number of nodal meridians (2^) 
corresponding to any particular tone of a bell, advantage may be 
taken of beats, whether due to accidental irregularities or intro- 
duced for the purpose by special loading (compare §§ 208, 209). By 
tapping cautiously round a circle of kUitude the places may be in- 
vestigated where the beats disappear, owing to the absence of one 
or other of the component tones. But here a decision must not 
be made too hastily. The inaudibility of the beats may be &voured 
by an unsuitable position of the ear or of the mouth of the re- 
sonator used in connection with the ear. By travelling round, 
a situation is soon found where the observation can be made to 
the best advantage. In the neighbourhood of the place where the 
blow is being tried there is a loop of the vibration which is most 
excited and a (coincident) node of the vibration which is least 
excited. When the ear is opposite to a node of the first vibration, 
and therefore to a loop of the second, the original inequality is 
redressed, and distinct beats may be heard even though the 
deviation of the blow from a nodal point may be very small. The 
accurate determination in this way of two consecutive places where 
no beats are generated is all that is absolutely necessary for the 
purpose in view. The ratio of the entire circumference of the 
circle of latitude to the arc between the points in question is in 
fact 48. Thus, if the arc between consecutive points proved to 
be 45'', we bhould infer that we were dealing with the case of « = 2, 
in which the deformation is elliptical. As a greater security 
against error, it is advisable in practice to determine a larger 

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number of points where no beats occur. Unless the deviation 
from symmetry be considerable, these points should be uniformly 
distributed along the circle of latitude \ 

In the above process for determining nodes we are supposed to 
hear distinctly the tone corresponding to the vibration under 
investigation. For this pui-pose the beats are of assistance in 
directing the attention; but in dealing with the more difficult 
subjects, such as church bells, it is advisable to have recourse to 
resonators. A set of v. Helmholtz s pattern, as manufactured bj 
K5nig, are very convenient. The one next higher in pitch to 
the tone under examination is chosen and tuned by advancing the 
finger acrdss the aperture. Without the security afforded by 
resonators, the determination of the octave is very uncertain. 

The only class of bells, for which an approximate theory can 
be given, are those with thin walls, §§ 233, 235 c. Of such the 
following glass bells may be regarded as examples : — 

I. c', g"b, c'"«. 

II. a, c'% V\ 
III. f% V\ 

The value of s for the gravest tone was 2, for the second 3, 
and for the third tone 4. 

Similar observations have been made upon a so-called hemi- 
spherical bell, of nearly uniform thickness, and weighing about 3 
cwt. Four tones could be plainly heard, 

the pitch being taken from a harmonium. The gravest tone has a 
long duration. When the bell is struck by a hard body, the 
higher tones are at first predominant, but after a time they die 
away, and leave eb in possession of the field. If the striking body 
be soft, the original preponderance of the higher elements is less 

By the method described there was no difficulty in shewing 
that the four tones correspond respectively to s = 2, 3, 4, 5. Thus 
for the gravest tone the vibration is elliptical with 4 nodal meri- 
dians, for the next tone there are 6 nodal meridians, and so on. 

^ The beUs, or gongs, as they are sometimes caUed, of striking clocks often giro 
disagreeable beats. A remedy may be found in a suitable rotation of the beU roond 
its axis. 

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235 <X.] BELLS. 391 

Tapping along a meridian shewed that the sounds became less 
clear as the edge was departed from, and this in a continuous 
manner with no suggestion of a nodal circle of latitude. A question 
to which we shall recur in connection with church bells here 
suggests itself. Which of the various coexisting tones characterizes 
the pitch of the bell as a whole ? It would appear to be the third 
in order, for the founders gave the pitch as E natural. 

In church bells there is great concentration of metal at the 
" sound-bow " where the clapper strikes, indeed to such an extent 
that we can hardly expect much correspondence with what occurs 
in the case of thin uniform bells. But the method already 
described suffices to determine the number of nodal meridians for 
all the more important tones. From a bell of 6 cwt. by Mears 
and Stainbank 6 tones could be obtained, viz. : 

e', c", r+, h"\^, d!'\ r\ 

(4) (4) (6) (6) (8) 

The pitch of this bell as given by the makers is d!\ so that it 
is the fifth in the above series of tones which characterizes the 
bell. The number of nodal meridians in the various components 
is indicated within the parentheses. Thus in the case of the tone 
e' there are 4 nodal meridians. A similar method of examination 
along a meridian shewed that there was no nodal circle of latitude. 
At the same time differences of intensity were observed. This 
tone is most fully developed when the blow is delivered about 
midway between the crown and the rim of the bell. 

The next tone is c". Observation shewed that for this vibra- 
tion also there are four, and but four, nodal meridians. But now 
there is a well-defined nodal circle of latitude, situated about a 
quarter of the way up from the rim towards the crown. As heard 
with a resonator, this tone disappears when the blow is accurately 
delivered at some point of this circle, but revives with a very small 
displacement on either side. The nodal circle and the four meri- 
dians divide the surface into segments, over each of which the 
normal motion is of one sign. 

To the tone /" correspond 6 nodal meridiana There is no 
well-defined nodal circle. The sound is indeed very faint when 
the tap is much displaced from the sound-bow; it was thought 
to fall to a minimum when a position about half-way up was 

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The three graver tones are heard loudly from the sound-bow. 
But the next in order, ft'^l?, is there scarcely audible, unless the 
blow is delivered to the rim itself in a tangential direction. The 
maximum effect occurs about half-way up. Tapping round the 
circle revealed 6 nodal meridians 

The fifth tone, d'", is heard loudly from the sound-bow, but 
soon falls off when the locality of the blow is varied, and in the 
upper three-fourths of the bell it is very faint. No distinct circular 
node could be detected. Tapping round the circumference shewed 
that there were 8 nodal meridians. 

The highest tone recorded, /'", was not easy of observation, 
and the mode of vibration could not be fixed satisfisustonly. 

Similar results have been obtained from a bell of 4 cwt, cast 
by Taylor of Loughborough for Ampton church. The nominal 
pitch (without regard to octave) was d, and the following were the 
tones observed : — 

el? -2, d"-6, /"-h4, 6'1?— 6", d'\ f, 
(4) (4) (6) (6) (8) 

In the specification of pitch the numerals following the note 
indicate by how much the frequency for the bell differed fix)m 
that of the harmonium employed as a standard. Thus the gravest 
tone e^ gave 2 beats per second, and was flat. When the number 
exceeds 3, it is the result of somewhat rough estimation, and 
cannot be trusted to be quite accurate. Moreover, as has been 
explained, there are in strictness two firequencies under each 
head, and these often differ sensibly. In the case of the 4th tone, 
6"b — 6" means that, as nearly as could be judged, the pitch of the 
bell was midway between the two specified notes of the 

Observations in the laboratory upon the above-mentioned bells 
having settled the modes of vibration corresponding to the five 
gravest tones, other bells of the church pattern could be sufficiently 
investigated by simple determinations of pitch. The results are 
collected in the following tabled and include, besides those already 
given, observations upon a Belgian bell, the property of Mr 
Haweis, and upon the five bells of the Terling peal. As regank 

1 On Bells, PWZ. Uag.y vol. 29, p. 1, 1890. 

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235 cl] 

the nominal jHtch of the latter bells, several observers concurred 
in fixing the Dotes of the peal as 

/#» 5*' «ft ^ ^' 

no attention being paid to the question of the octave. 





Terling (5),|Terlmg (4), Terling (8), Terling (2), Teriing (1), 

Osborn, Hears, Graye, Gardner, Warner, 

1788. ' 1810. 1628. 1728. 1868. 

Actual Pitch by Harmonium. 



























a"-6 1 ef'-3 














Pitch referred to fifth tone as c. 















*l? + 




cb + 4 




at? -a 













Examination of the table reveals the remarkable fact that 
in every case of the English bells it is the 5th tone in order 
which agrees with the nominal pitch, and that, with the exception 
of Terling (4), no other tone shews such agreements Moreover, 
as appeared most clearly in the case of the bell cast by Mears and 
Stainbank, the nominal pitch, as given by the makers, is an octave 
below the only corresponding tone. 

The highly composite, and often discordant, character of the 
sounds of bells tends to explain the discrepancies sometimes 
manifested in estimations of pitch. Mr Simpson, who has devoted 
much attention to the subject, has put forward strong arguments 
for the opinion that the Belgian makers determine the pitch of 
their bells by the tone 2nd in order in the above series, so that 
for instance the pitch of Terling (3) would be a and not at. In 
subordination to this tone they pay attention also to the next 
(the 3rd in order), classifying their bells according to the character 

^ In this comparison the gravest tone is disregarded. 

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Google — 



[235 a. 

of the third, whether major or minor, so compounded. Thus 
in Terling (3) the interval, a' to c" , is a major third. The com- 
parative neglect with which the Belgians treat the 5th tone, 
regarded almost exclusively by English makers, may perhaps be 
explained by a less prominent development of this tone in Belgian 
bells, and by a difference in treatment. When a bell is sounded 
alone, or with other bells in a comparatively slow succession, 
attention is likely to concentrate itself upon the graver aud more 
persistent elements of the souud rather than upon the acnter 
and. more evanescent elements, while the contrary may be 
expected to occur when bells follow one another rapidly in a peaL 

In any case the false octaves with which the Table abounds 
are simple facts of observation, and we may well believe that their 
correction would improve the genei*al effect. Especially should 
the octave between the 2nd tone and the 5th tone be made true. 
Probably the lower octave of the gravest, or hum-note, as it is 
called by English founders, is of less importance. The same may 
be said of the fifth, given by the 4th tone of the series, which 
is much less prominent. The variations recorded in the Table 
would seem to shew that no insuperable obstacle stands in the 
way of obtaining accurate harmonic relations among the various 

No adequate explanation has been given of the form adopted 
for church bells. It appears both from experiment and from the 
theory of thin shells that this form is especially stiff, as regards the 
principal mode of deformation (s = 2), to forces applied normally 
and near the rim. Possibly the advantage of this form lies in its 
rendering less prominent the gravest component of the sound, 
or the hum-note. 

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236 6. In the last chapter (§§ 232, 233) we have considered 
the comparatively simple problem of the vibration in two dimen- 
sions of a cylindrical shell, so far at least as relates to vibrations 
of a flexural character. The shell is supposed to be thin, to be 
composed of isotropic material, and to be bounded by infinite 
coaxal cylindrical surfaces. It is proposed in the present chapter 
to treat the problem of the cylindrical shell more generally, and 
further to give the theory of the flexural vibrations of spherical 

In considering the deformation of a thin shell the most 
important question which presents itself is whether the middle 
surface, viz. the surface which lies midway between the boundaries, 
does, or does not, undergo extension. In the former case the 
deformation may be called extensionaX, and its potential energy is 
proportional to the thickness of the shell, which will be denoted 
by 2A. Since the inertia of the shell, and therefore the kinetic 
energy of a given motion, is also proportional to A, the frequencies 
of vibration are in this case independent of A, § 44. On the 
other hand, when no line traced upon the middle sur&ce under- 
goes extension, the potential energy of a deformation is of a 
higher order in the small quantity h. If the shell be conceived 
to be divided into laminse, the extension in any lamina is pro- 
portional to its distance from the middle surface, and the con- 
tribution to the potential energy is proportional to the square 
of that distance. When the integration over the thickness 
is carried out, the whole potential energy is found to be propor- 
tional to h\ Vibrations of this kind may be called inextensional, 

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[235 6. 

or flexural, and (§ 44) their frequencies are proportional to A, so 
that the sounds become graver without limit as the thickness is 

Vibrations of the one class may thus be considered to depend 
upon the term of order A, and vibrations of the other class upon 
the term of order A', in the expression for the potential energy. 
In general both terms occur ; and it is only in the limit that the 
separation into two classes becomes absolute. This is a question 
which has sometimes presented difficulty. That in the case of 
extensional vibrations the term in A' should be negligible in 
comparison with the term in h seems reasonable enough. But 
is it permissible in dealing with the other class of vibrations to 
omit the term in h while retaining the term in A* ? 

The question may be illustrated by considei-ation of a statical 
problem. It is a general mechanical principle (§ 74) that, if given 
displacements (not sufficient by themselves to determine the 
configuration) be produced in a system originally in equilibrium 
by forces of corresponding tjrpes, the resulting deformation \& 
determined by the condition that the potential energy shall be 
as small as possible. Apply this principle to the case of an elastic 
shell, the given displacements being such as not of themselves to 
involve a stretching of the middle surface. The resulting defor- 
mation will, in general, include both stretching and bending, and 
any expression for the energy will be of the form 

Ah (extension)* + Bh^ (bending)' (1). 

This energy is to be as small as possible. Hence, wlien the 
thickness is diminished without limit, the actual displacement 
will be one of pure bending, if such there be, consistent with 
the given conditions. 

At first sight it may well appear strange that of the two terms 
the one proportional to the cube of the thickness is to be retained, 
while that proportional to the first power may be neglected. The 
fact, however, is that the large potential energy that would 
accompany any stretching of the middle surface is the very reason 
why such stretching does not occur. The comparative laigeness 
of the coefficient (proportional to h) is more than neutralized by 
the smallness of the stretching itself, to the square of which the 
energy is proportional. 


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An example may be taken from the case of a rod, clamped at 
one end A, and deflected by a lateral force ; it is required to trace 
the effect of constantly increasing stiffness of the part included 
between A and a neighbouring point B, In the limit we may 
regard the rod as clamped at By and neglect the energy of the 
part AB, in spite of, or rather in consequence of, its infinite 

It would thus be a mistake to regard the omission of the term 
in A as especially mysterious. In any case of a constraint which 
is supposed to be gradually introduced (§ 92 a), the vibrations 
tend to arrange themselves into two classes, in one of which the 
constraint is observed, while in the other, in which the constraint 
is violated, the frequencies increase without limit. The analogy 
with the shell of gradually diminishing thickness is complete if 
we suppose that at the same time the elastic constants are in- 
creased in such a manner that the resistance to bending remains 
unchanged. The resistance to extension then becomes infinite, 
and in the limit one class of vibrations is purely inextensional, or 

In the investigation which we are about to give of the 
vibrations of a cylindrical shell, the extensional and the in- 
extensional classes will be considered separately. It would 
apparently be more direct to establish in the first instance a 
general expression for the potential energy complete as far as 
the term in A*, from which the whole theory might be deduced. 
Such an expression would involve the extensions and the curva- 
tures of the middle surface. It appears, however, that this method 
is difficult of application, inasmuch as the potential energy (correct 
to A') does not depend only upon the above-mentioned quantities, 
but also upon the manner of application of the normal forces, 
which are in general implied in the existence of middle surface 

236 c. The first question to be considered is the expression of 
the conditions that the middle surface remain unextended, or if 
these conditions be violated, to find the values of the extensions in 
terms of the displacements of the various points of the smface. 

^ On the Uniform Deformation in Two Dimensions of a Cylindrical Shell, with 
Application to the General Theory of Deformation of Thin Shells. Proe. Math, 
Soe., vol. XX. p. 872, 18S9. 

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We will suppose in the first instance merely that the surface is of 
revolution, and that a point is determined by cylindrical co-ordi- 
nates z, r, <l>. After deformation the co-ordinates of the above 
point become Z'\-Sz, r'\-Sr, ^ + S^ respectively. If ds denote 
an element of arc traced upon the surface, 

(ds + dB&y = (dz + dSzy + (r + Sr)« (d4> + dS<^)« + (dr + dSry, 

so that 

dadBd^dzdSz + r'd^dSit) + rSr {d4>y + dr dSr (1). 

In this we regard z and (f) as independent variables, so that, for 

while ^^^(F^^dS ^^' 

in which by hypothesis dr/d<l> = 0. Accordingly 

dB8_(dzy(dSz drdSrj {d^^f ( dSif> I 

ds "{dayidz ^dz dz)^{dsy X d<t> ^ ^) 

dzd<f> ( dSz dS^ dr dSr ) .a\ 

"^ (ds)> \d<l>^ dz'^dzd<f>) ^ ^' 

in which dSs/ds represents the extension of the element ds. If 
there be no extension of any ai'c traced upon the surface, (2) must 
vanish independently of any relations between dz and d^. Hence 

diz dr d£r _ .^. 

dz dz dz 

r^ + Sr = (4), 

dSz d5^ ^^^ — Ci) 

d<f> dz dz d<f> 

From these, by elimination of Sr, 

dSz^drd^r dB(f> \ ^ 
dz dzdz\ d<f> J ' 

dBz dS<l> ^drd^B<t>^Q^ 
d<f> dz dz d<f>^ ' 

and again, by elimination of iz^ 

£(r^m_r^d'^^0 (6). 


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235 c] 



If the distribution of thickness and the form of the boundary 
or boundaries be symmetrical with respect to the axis, the normal 
functions of the system are to be found by assuming S<f> to be 
proportional to cos 9^, or sin 8(f>. The equation for B<l> may then 
be put into the form 


«.r^ga0 = O 


It will be seen that the conditions of inextension go a long way 
towards determining the form of the normal fonctions. 

The simplest application is to the case of a cylinder for which 
r is constant, equal say to o. Thus (3), (4), (5), (7) become simply 

_=0. Sr + a^ = 0. 5^ + a'-^ = (8). 



By (9), if S^ oc cos 8<l>, we may take 

aB<l>=:{Ata + Btz) cos 8<f> (10), 

and then, by (8), Sr = 8 (Aga + Bgz) sin 8<l> (11), 

Sz = - 8"^ B^a sin 8<f> (12). 

Corresponding terms, with fresh arbitrary constants, obtained by 
writing 8(t> + Jtt for 8<f>, may of course be added. If 5, = 0, the 
displacement is in two dimensions only (§ 233). 

If an inextensible disc be attached to the cylinder at j? =r 0, so 
as to form a kind of cup, the displacements Sr and Btj) must vanish 
for that value of z, exception being made of the case « = 1. Hence 
Ag = 0, and 

aS<l> = BtZ cos 8<f>, Sr = 8 BfZ sin 8<l>, Sz = — «~*-B,a sin s^... (13). 

Again, in the case of a cone, for which r = tan 7 . z, the equa- 
tions (3), (4), (5), (7) become 

dBz ^ ^ dBr ^ , dB<l> ^ ^ ^ 
d^+^^'^d^^^' ;.tan7^+Sr=0 



+ z^ tan*7 ^^ + tan 7 ^ = 



U-^)'" a^'- 

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If we take, as usual, 3^ oc cos 8^, we get as the solution of (15) 

S<^ = (^ + 5,-er-i)cos«<^ (16), 

and corresponding thereto 

Br = 8 tan y(AtZ'\-Bg)am8<f> (17), 

Sz = tan« 7 [s'^ 3,-8 {A^z + S,)] sin «^ (18). 

If the cone be complete up to the vertex at jgr = 0, -B, = 0, so that 

S^ = -4,cos«^ (19), 

Sr = tfil, rsin«^ (20), 

8^ = — «-4,tan7rsin«^ (21). 

For the cone and the cylinder, the second term in the general 
equation (7) vanishes. We shall obtain a more extensive class of 
soluble cases by supposing that the surface is such that 

r*-T-5 = constant (22), 

an equation which is satisfied by sur&ces of the second degree in 
general. If 

z^ r^ 

^ + 6i = l (23). 

we shall find 7^-=-^ = — r (24); 

dz^ a» "^ ^' 

and thus (7) takes the form 

d^-^«* = (25). 

if i<f> X cos 8^t Aiid a is defined by 

a^jr^dz (26), 

or in the present case 

' = W>«^-z <27). 

The solution of (25) is 

^♦-Ksr-K:-^r]-*- (»> 

The corresponding values of Br and S^ are to be obtained from (4) 
and (5). 


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235 c] NORMAL MODES. 401 

If the surface be complete through the vertex z^a, the term 
multiplied by B must disappear. Thus, omitting the constant 
multiplier, we may take 

^ = (Sr^'* <29); 

whence, by (4), (5), 

*"-a(^T^""'* <3^>' 

*"=(**+"> SStS^'"^'* •^^'>- 

If we measure / from the vertex, z ^a — z^ and we may write 
S* = .(^)'co8*^ (32), 

Sr=«r(^ysin«<^ (33), 

Sz = -g/=:^I(jj + l)a-«/U^ysin«<^ (34). 

For the parabola, a and 6 are infinite, while b^/a^2a\ and 
r*=^4ia'z\ Thus we may take* 

S^ = r»cos«^, Sr = ^+i8in«<^, S-2' = -2(« + l)aV8in^...(35). 

We will now take into consideration the important case of the 
sphere, for which in (23) b = a. Denoting by the angle between 
the radius vector and the axis, we have z^^a cos 0,r^a sin 0, and 
thus from (29), (30), (31) 

S<^ = co8«<^tan'i^ (36), 

Sr/a = « sin «<^ sin ^tan'i^ (37), 

Sz/a = {1'\- 8 cos 0) sin 84i ton' i0 (38). 

The other terms of the complete solution, corresponding to 
(28), are to be obtained by changing the sign of «. 

In the above equations the displacements are resolved parallel 
and perpendicular to the axis 0-0, It would usually be more 
convenient to resolve along the normal and the meridian. If the 
components in these directions be denoted by w and aS0, we have 

w==Brsm0'\-Sz cos 0, aS0 ^ Br cos — Sz sin 0; 

1 On the Infinitesimal Bending of Sorfaces of Bevolution. Proc, Math. Soc., 
vol. xui. p. 4, 1S81. 

R, 26 

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SO that altogether 

S<^ = co8d<^[^,tan'i^ + 5,cot«itf] (39), 

S0 = - sin 8(f> sin [A, tB.n' ^0 -- B,cof ^0] ..(40), 

w/a = sin 8<f) [Ag {s + cos 0) tan* ^0 + 5, (« - cos 0) cot' ^0] . . .(41). 

To the above may be added terms derived by writing «^ + fir 
for 8<f>, and changing the arbitrary constants. 

235 d. We now proceed to apply the equations of § 235 c to 
the principal extensions of a cylindrical surface, with a view to the 
formation of the expression for the potential energy. The axial 
and circumferential extensions will be denoted respectively by €i, 
€2, and the shear by w. The first of these is given by (2) § 235 c, 
if we suppose that d<f> = 0, dz/ds = 1. Since in the case of a 
cylinder dr/dz = 0, we find 

dSz . 

'^-Tz <^^ 

In like manner 

'^-H^'dif, ^'^ 

The value of the shear may be arrived at by considering the 
diflference of extensions for the two diagonals of an infinitesimal 
square whose sides are dz and ad<f>. It is 

1 d8z , dS<^ ,^. 

'' = ad<l>+''-di ^^^ 

The next part of the problem, viz. the expression of the potential 
energy by means of €1, Cj, bt, appertains to the general theory of 
elasticity, and can only be treated here in a cursory manner. But 
it may be convenient to give the leading steps of the investigation, 
referring for further explanations to the treatises of Thomson and 
Tait and of Love. In thfe notation of the former {Natural 
Philosophy, § 694) the general equations in three dimensions are 

na=^S, nb = T, nc=U (4), 

Jlfe=P-c^(Q + i^)^ 

Mf^ Q^a(R + P)[ (5), 

Mg = R-a{P + Q)) 

where <^ — -a — (6)*- 

2m ' 

1 M is Young's modulus, 0- is Poisson's ratio, n is the constant of rigidity, and 
(m - ^n) that of compressibility. 

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The energy lu, corresponding to unit of volume, is given by 

+ 2(m-n)(/5r + 5'«+e/) + n(a^ + 6» + c») (7). 

In the application to a lamina, supposed parallel to the plane 
ary, we are to take -R = 0, iS = 0, T = 0, so that 

g <^f^> « = 0, 6 = (8). 

Thus in terms of the extensions e, f, parallel to x, y, and of the 
shear c, we get 

«, = „|e. + /. + ^--^(e+/)» + ic'| (9). 

This is the energy reckoned per unit of volume. In oixier to 
adapt the expression to our purposes, we must multiply it by the 
thickness {2h), Hence as the energy per unit area of a shell 
of Ihickness 2A, we may take in the notation adopted at the com- 
mencement of this section, 

2nA|e,» + e,» + iw> + ^^(6, + 6,)j (10). 

This expression may be applied to curved as well as to plane 
plates, for any modification due to curvature must involve higher 
powers of h. The same is true of the energy of bending. 

235 e. We are now prepared for the investigation of the 
extensional vibrations of an infinite cylindrical shell, assumed to 
be periodic with respect both to z and to ^. It will be convenient 
to denote by single letters the displacements parallel to z, if>,r\ 
we take 

Sz^u, aB<l> = v, hr^w (1). 

These functions are to be assumed proportional to the sines or 
cosines o( jz/a and «^. Various combinations may be made, of 
which an example^ is 

u=U cos 8<l> cos jz/Uj t; = F sin 8<l> sin jz/a, 

w = TT cos s4> sin jz/a (2) ; 

so that (1), (2), (3), § 235 d 

a. €i^— jU cos 8<t) sin jz/a (3), 

a,€i^(W + sV)cos8<l>sinjz/a (4), 

a.w = (— sU -\- jV) sin 8<l> cos jz/a (5). 

^ Additions of Jt to $</>, or io jz/a, or to both, may of coarse be made at pleasure. 


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The potential energy per unit area is thus (10) § 235 d 
2n/ia-»reos«5^sin«j^/a|j»Cr>+(Tr + «F)« + ^^(Tr + «F-jir^ 

+ ^Qm^8<l> coa^jz/ai-sU + jVy] (6). 

Again, if p be the volume density, the kinetic energy per unit 
of area is 

ph\ (-it) cos!^ s<I> cos* jz/a-^(-jT-] sin^ 86 sin* jz/ a 

8<f> sin*jz/a , 


In the integration of (6), (7) with respect to z and 0, ^ is the 
mean value of the square of each sine or cosine.* We may then 
apply Lagrange's method, regarding [7, F, TT as independent 
generalized co-ordinates. If the type of vibration he cospt, 
and p*p/n = A;^, the resulting equations may be written 

{2(iV + l)j« + 5»-Ar^a«}Cr-(2iV + l)>F-2i\rjTr = 0...(8), 


where N ^"^ (11). 

The frequency equation is that expressing the evanescence of 
the determinant of this triad of equations. On reduction it may 
be written 

[ifc^a* - j» - «*] {^^a« [^^a« - 2 (iV^ + 1) (j» + fi« + 1)] 

+ 4(2i\r + l)j^} + 4 (2iVr+ i)jV = (12).* 

These equations include of course the theory of the extensional 
vibrations of a plane plate, for which a = oo . In this application 
it is convenient to write o^ = y, s/a = /9, jja = 7. The displace- 
ments are then 

w= UcosPyc6syz, v = Vsmfiysinyz, w — W cos fiysinyz 


^ In the physical problem of a simple cylinder the range of integration for ^ is 
from to 2t ; but mathematicaUy we are not confined to one reTolation. We may 
conceiye the sheU to consist of several superposed conYolations, and then s is not 
limited to be a whole number. 

' Note on the Free Vibrations of an infinitely long Cylindrical Shell. Proc. 
Ray, Soc„ vol. 46, p. 446, 1889. 

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235 e. J PLANE PLATE, 405 

When a is made infinite while i8, 7 remain constant, the 
equations (10), (8), (9) ultimately assume the form TT «= 0, and 

{2(2«r+i)y + ^-.A;»}[r-(2iV^4.1)^y9F=0...(14), 

-(2iV^ + l)7/9l7 + {7« + 2(iV^+l)/3»-A»)F-0...(15); 

and the determinantal equation (12) becomes 

^[*'-y-/9*][**-2(iV^H-l)(7» + )S«)]«0 (16). 

In (16), as was to be expected, 1^ appears as a function of 
(i8* + 7^). The first root A:» = relates to flexural vibrations, 
not here regarded. The second root is 

A'^/S' + T^ (17), 

or l>^ = ^08«+y) (18). 

At the same time (14) gives 

7l7-/8F=rO (19). 

These vibrations involve only a shearing of the plate in its own 
plane. For example, if 7 = 0, the vibration may be repre- 
sented by 

tt = cos)9y cosp^, t;=«0, t£; = (20). 

The third root of (16) 

A:» = 2(i\r+l)(;8« + y) = ^(/8» + y) (21) 

gives p> = J^?!^^±0^ (22). 

The corresponding relation between U and V is 

^t7 + 7F=0 (23). 

A simple example of this case is given by supposing in (IS), 
(23), )8 = 0. We may take 

14 = 00872: coQptf v = 0, w = (24), 

the motion being in one dimension. 

Reverting to the cylinder we will consider in detail a few 
particular cases of importance. The first arises when j = 0, that is, 
when the vibrations are independent of z. The three equations 
(8), (9), (10) then reduce to 

(«*-A:»a«)Cr=0 (26), 

{2(iV + l)««-A;«a»}F+2(iV+l)«TF = (26), 

2(JV'+l)«F+12(i\r + l)-A«a«}Tr = (27); 

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and they may be satisfied in two ways. First let F= Tr = ; then 
U may be finite, provided 

fi»-jfc»a» = (28). 

The corresponding type for u is 

tt =cos«0 co^pt (29), 

where p' = — ^ (30). 

In this motion the material is sheared without dilatation of area 
or volume, every generating line of the cylinder moving along 
its own length. The frequency depends upon the circumferential 
wave-length, and not upon the curvature of the cylinder. 

The second kind of vibrations are those for which {7=0, so 
that the motion is strictly in two dimensions. The elimination of 
the ratio VjW from (26), (27) gives 

A»a«{Jfc»a»-2(iV^ + l)(l+«»)}=0 (31). 

as the frequency equation. The first root is A:* = 0, indicating 
infinitely slow motion. The modes in question are flexural* for 
which, according to our present reckoning, the potential eneigy 
is evanescent. The corresponding relation between V and W is 
by (26) 

«F+ Tr = (32). 

giving in (3), (4), (5), 

€i = 0, €, = 0, «r = 0. 
The other root of (31) is 

A;«a» = 2(iV + l)(l+5») (33), 

or ;)» = — ; (34) ; 

while the relation between V and W is 

F-«TF«0 (36). 

The type of the motion may be taken to be 

u ss 0, v « « sin tf cos pty w = cos 8<fi cos pt (36). 

It will be observed that when 8 is very large, the flexural 
vibrations (32) tend to become exclusively radial, and the exten- 
sional vibrations (35) tend to become exclusively tangential. 

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Another important class of vibrations are those which are 
characterized by symmetry round the axis, for which accordingly 
« = 0. The general frequency equation (12) reduces in this case to 

{ifc«a«-j«}{ifc»a«[ifc«a«-2(iV^+l)(i«+l)] + 4(2iV+l)j'}=0 


Corresponding to the first root we have 17=0, TT^O, as is 
readily proved on reference to the original equations (8), (9), (10) 
with « = 0. The vibrations are the purely torsional ones repre- 
sented by 

w = 0, v = sin {jzja) cos p^, w; = (38), 

where 1>" = ^! (39). 

The frequency depends upon the wave-length parallel to the 
axis, and not upon the radius of the cylinder. 

The remaining roots of (37) correspond to motions for which 
F=:0, or which take place in planes passing through the axis. 
The general character of these vibrations may be illustrated by 
the case where j is small, so that the wave-length is a large 
multiple of the radius of the cylinder. We find approximately 
from the quadratic which gives the remaining roots 

3m-' + (ir-+l> <«)• 

>^a>-^-^i^- ,«> 

The vibrations of (40) are almost purely radial. If we suppose 
that j actually vanishes, we fall back upon 

A«o' = 2(iyr+l) (42), 

and p. = i-^«-l_ (43)S 

obtabable from (33), (34) on introduction of the condition «=s0. 
The type of vibration is now 

wrsO, t; = 0, w^cospt (44). 

1 This eqaation was first given by Love in a memoir *'0n the small Free 
Yibrations and Deformation of a thin Elastic Shell," Phil. Trans., vol. 179 (18S8), 
p. 528. 

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On the other hand, the vibrations of (41) are ultimately purely 
axial. As the type we may take 

u = 008 jz I a . cos pty t; = 0, w =* -= — j sin jz/a .cospt... (45), 

where »^ = —^ (461 

Now, if q denote Young's modulus, we have, § 214, 
q = n (3m — n)/m, 

80 that ;>»=^ (47). 

Thus u satisfies the equation 

d*u _ q d^u 
dt*'"p d?' 

which is the usual formula (§ 150) for the longitudinal vibrations 
of a rod, the fact that the section is here a thin annulus not 
influencing the result to this order of approximation. 

Another particular case worthy of notice arises when « = 1, so 
that (12) assumes the form 

Jk^a«(ifc»a«-j«-l)[ifc»a«-2(iV'+l)(j« + 2)] 

+ 4j»(ifc»a»-jO(2iV+l) = 0...(48). 

As we have already seen, if j be zero, one of the values of jfc* 
vanishes. If j be small, the corresponding value of A:' is of the 
order J*. Equation (48) gives in this case 

^""'"W+i^* <*^^' 

or in terms of p and g, 

^' = 2$ (^«)- 

The type of vibration is 

M = ^ 

t; = 8in^8inJ2:/a.co8jt>t \ (51)^ 

w = — cos <l> sin jz/a . cos pt j 

and corresponds to the flexural vibrations of a rod (§ 163). In 
(51) t; satisfies the equation 


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in which J a* represents the square of the radius of gyration of the 
section of the cylindrical shell about a diameter. 

This discussion of particular cases may sufSce. It is scarcely 
necessary to add, in conclusion, that the most general deformation 
of the middle surface can be expressed by means of a series of such 
as are periodic with respect to z and ^, so that the problem con- 
sidered is really the most general small motion of an infinite 
cylindrical shell 

The extensional vibrations of a cylinder of finite length have 
been considered by Love in his Theory of Elasticity^ (1893), where 
will also be found a full investigation of the general equations of 
extensional deformation. 

235/ When a shell is deformed in such a manner that no 
line traced upon the middle surface changes in length, the term of 
order h disappears from the expression for the potential energy, 
and unless we are content to regard this function as zero, a 
further approximation is necessary. In proceeding to this the 
first remark that occurs is that the quality of inextension attaches 
only to the central lamina. Consider, for example, a portion of a 
cylindrical shell, which is bent so that the original curvature is 
increased. It is evident that while the middle lamina remains 
nnextended, those laminae which lie externally must be stretched, 
and those that lie internally must be contracted. The amount of 
these stretchings and contractions is proportional in the first place 
to the distance from the middle surface, and in the second place to 
the change of curvature which the middle surface undergoes. The 
potential energy of bending is thus a question of the curooJtures of 
. the middle surface. Displacements of translation or rotation, such 
as a rigid body is capable of, may be disregarded. 

In order to take the question in its simplest form, let us refer 
the original surface to the normal and principal tangents at any 
point P as axes of co-ordinates, and let us suppose that after 
deformation the lines in the sheet originally coincident with the 
principal tangents are brought back (if necessary) so as to occupy 
the same positions as at first. The possibility of this will be 
apparent when it is remembered that, in virtue of the inexten- 
sion of the sheet, the angles of intersections of all lines traced 

1 Also ¥m. Trans, vol. 179 a, 188S. 

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upon it remain unaltered. The equation of the original surface in 
the neighbourhood of the point being 

\pi pJ 

\PI P2 

that of the deformed surface may be written 


^"■*i>i + Sp/ 



Pi + Bp^ 

In strictness (pi + Spi)""S (p^ + Bp-)"^ are the curvatures of the 
sections made by the planes a:, y ; but since the principal curvatures 
are a maximum and a minimum, they represent in general with 
sufficient accuracy the new principal curvatures, although these 
are to be found in slightly different planes. The condition of 
inextension shews that points which have the same x, y in (1) 
and (2) are corresponding points ; and by Gauss's theorem it is 
further necessary that 

^^i + ^* = (3). 

Pi P2 

It thus appears that the energy of bending will depend in 
general upon two quantities, one giving the alterations of principal 
curvature, and the other r depending upon the shift (in the 
material) of the principal planes. 

The case of a spherical surface is in some respects exceptional 
Previously to the bending there are no planes marked out as 
principal planes, and thus the position of these planes after 
bending is of no consequence. The energy depends only upon 
the alterations of principal curvature, and these by Gauss's theorem 
are equal and opposite, so that, if a denote the radius of the 
sphere, the new principal radii are a + Sp, a — Bp. If the equation 
of the deformed surface be 

Zz^Ax' + iBxy-k^Cy- (4), 

(a + Sp)-i + (a-Sp)-» = il + C, 

(a + Sp)-^(a-Sp)-* = il(7-5*; 

{s^y^H^-cy+B^ (5). 

we have 

so that 

We have now to express the elongations of the various laminff 
of a shell when bent, and we will begin with the case where t = 0, 

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that is, when the prmcipal planes of curvature remain unchanged. 
It is evident that in this case the shear c vanishes, and we have to 
deal only with the elongations e and /parallel to the axes, § 235 d. 
In the section by the plane of zx, let s, s' denote corresponding 
infinitely small arcs of the middle surface and of a lamina distant 
h from it. If -^ be the angle between the terminal normals, 
s = pi^^, s' = (/?! + A) -^j s' — s = A-^. In the bending, which leaves 
8 unchanged, 

Ss'«ASn^ = AsS(l/pi). 

Hence e = Ss'/s' = AS(l/pi), 

and in like manner /= AS(l/pj). Thus for the energy U per unit 
area we have 

[\ pJ \ pJ m + 71 \ pi p,/ ) 
and on integration over the whole thickness of the shell (2A) 

This conclusion may be applied at once, so as to give the result 
applicable to a spherical shell; for, since the original principal 
planes are arbitrary, they can be taken so as to coincide with the 
principal planes after bending. Thus t = 0; and by Gauss's 

S(l/pOi-S(l/p,) = 0, 

so that u^^^B-J (7), 

where S(l/p) denotes the change of principal curvature. Since 
c = — / 5r = 0, the various laminae are simply sheared, and that in 
proportion to their distance from the middle surface. The energy 
is thus a function of the constant of rigidity only. 

The result (6) is applicable directly to the plane plate; but 
this case is peculiar in that, on account of the infinitude o( pi, p^ 
(3) is satisfied without any relation between Bpi and Sp,. Thus for 
a plane plate 

'^-r\^--h^i^.{y^'} ""■ 

where l/pi, l/ps, are the two independent principal curvatures after 

1 This wOl be found to agree with the value (2) § 214, expressed in a different 

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We have thus far considered r to vanish; and it remains to 
investigate the effect of the deformations expressed by 

S^ = T^y = iT(p-i7') (9), 

where f, 17 relate to new axes inclined at 45*^ to those of x, y. The 
curvatures defined by (9) are in the planes of f, rj, and are equal 
in numerical value and opposite in sign. The elongations in these 
directions for any lamina within the thickness of the shell are At, 
- At, and the corresponding energy (as in the case of the sphere 
just considered) takes the form 

U'=^*^ (10). 

This energy is to be added ^ to that already found in (6) ; and 
we get finally 

as the complete expression of the energy, when the deformation is 
such that the middle surface is unextended. We may interpret r 
by means of the angle x* through which the principal planes are 
shifted; thus 

-^<-p-.) • *"'■ 

235 g. We will now proceed with the calculation of the 
potential energy involved in the bending of a cylindrical shell 
The problem before us is the expression of the changes of prin- 
cipal curvature and the shifts of the principal planes at any point 
P (z, <l>) of the cylinder in terms of the displacements u, v,w. As in 
§ 235 /, take as fixed co-ordinate axes the principal tangents and 
normal to the undisturbed cylinder at the point P, the axis of s 
being parallel to that of the cylinder, that of y tangential to the 
circular section, and that of ^ normal, measured inwards. If, as it 
will be convenient to do, we measure z and <f} fix)m the point P, we 
may express the undisturbed co-ordinates of a material point Q in 
the neighbourhood of P, by 

x^z, y=^a<l>, ?=ia0' (1). 

I There are clearly no terms involving the products of r with the cfaanges of 
principal curvature d {pi~^)t S {p2'^^) ; for a change in the sign of r can have so 
influence upon the energy of the deformation defined by (2). 

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During the displacement the co-ordinates of Q will receive the 

u, to8m<f>-\-vcos<f}, — i(;cos0 + t;sin^;. 

so that after displacement 

or, if u,v,whe expanded in powers of the small quantities z, <f>, 

du du , ,^. 

.=. + «.+ ^^. + ^^+ (2). 

dv dv , ,^. 

y = a<f> + w,<l> + v, + ^^z + ^^^<f>+ (3), 

. , ., 1 dhu , dhu . . dhv ., 
dv . dv ., ... 

+d./*+d^/ W' 

i£o, Vo, . . . being the values of u, v at the point P. 

These equations give the co-ordinates of the various points of 
the deformed feheet. We have now to suppose the sheet moved as 
a rigid body so as to restore the position (as far as the first power 
of small quantities is concerned) of points infinitely near P. A 
purely translatory motion by which the displaced P is brought 
back to its original position will be expressed by the simple 
omission in (2), (3), (4) of the terms Uq, v©, w^ respectively, which 
are independent of z, <f>. The effect of an arbitrary rotation is 
represented by the additions to x, y, f respectively of yoa^ — (Icdj, 
(Joh — ^o>8» xto^ — ytoi ; where for the present purpose Wi, Wj, ©3 are 
small quantities of the order of the deformation, the square of 
which is to be neglected throughout. If we make these additions 
to (2), &c., substituting for x, y, f in the terms containing d their 
approximate values, we find so far as the first powers of z, ^ 

du du 
. , , dv , dv . 

^ dw dw . , . ^ , 

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[235 ()f. 

Now, since the sheet is assumed to be unextended, it must be 
possible so to determine cdi, Wji ©s that to this order a? = z, y = a^, 
f=0. Hence 

du ^ 

dv ^ dv 


— Vo + axoi = 0. 

The conditions of inextension are thus (if we drop the suflSces 
iij^ BO longer requii-ed) 



^ , dv ^ du ^ dv ^ 


which agree with (8) § 235 c. 

Returning to (2), &c., as modified by the addition of the trans- 
latory and rotatory terms, we get 

x^z + terms of 2nd order in z, ^, 


, d^w ,^dv . dv .. 
or yince by (5) d^w/dz^ = 0, and dv/d<l> = — «;, 

The equation of the deformed surface after transference is thus 
y- (1 dp 1 (^ ) f 1 1 _l_dHo) 

Comparing with (2) § 235/ we see that 

fin s 1 1 / j_ <^'«'^ 1 /d» d»w \ ,_. 

^^ = ^' ^^=-^r + df'J' "^^afc-did^j-^^)' 

so that by (11) §235/ 

'^ ~ 3a» ti^^Mi a? V ■•" d<^V "'' \dz dzd<f,) J ^^ 

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This is the potential energy of bending reckoned per unit of 
area. It can, if desired, be expressed by (5) entirely in terms of v\ 

We will now apply (8) to calculate the whole potential energy 
of a complete cylinder, bounded by plane edges z^±l, and of 
thickness which, if variable at all, is a function of z only. Since 
u, V, w are periodic when 4> increases by 2'7r, their most general 
expression in accordance with (5) is [compare (10), &c., § 235 c] 

t; = 2 [(il,a + B,z) cos 8^ - {A,' a + B^z) sin «^] (9), 

w = 2 [« {A^a + Bgz) sin «^ + « {A^a + B^z) cos 8^] .... (10), 

tf — 2[— «~^5#asin«<^ — «~^5/acos«<^] (11), 

in which the summation extends to all integral values of 8 from 
to ». But the displacements corresponding to « = 0, 5=1 are 
such as a rigid body might undergo, and involve no absorption of 
energy. When the values of u, v, w are substituted in (8) all the 
terms containing products of sines or cosines with different values 
of 8 vanish in the integration with respect to <^, as do also those 
which contain cos 8if> sin 8<fi. Accordingly 

Jo - 3a [_m + na* ^ 

{{A,a + B,zy -f (A/ a + B.^zf] + 2 («^ - 1)» (5,« + 5/»)1 . . .(12). 

Thus far we might consider A to be a function of z ; but we will 
now treat it as a constant. In the integration with respect to z 
the odd powers of z will disappear, and we get as the energy of the 
whole cylinder of radius a, length 21, and thickness 2h, 

+ ^,(5.»+5;«)|+£.^+£;»] (13), 

in which «=2, 3, 4,.... 

The expression (13) for the potential energy suflBces for the 
solution of statical problems. As an example we will suppose 
that the cylinder is compressed along a diameter by equal forces 
F, applied at the points z^Zi, ^ = 0, <^ = 7r, although it is true 
that so highly localised a force hardly comes within the scope of 

1 From the general equations of Mr Love's memoir already cited a concordant 
result may be obtained on introduction of the appropriate conditions. 

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[235 g. 

the investigation, in consequence of the stretchings of the middle 
surface, which will occur in the immediate neighbourhood of the 
points of application ^ 

The work done upon the cylinder by the forces F during the 
hjrpothetical displacement indicated by SAg, &c., will be by (10) 

- Fls (a£A/ + zMs) (1 + cos sir), 
so that the equations of equilibrium are 

-rj-i = -(l + cos 8ir) saF, 

dB. ^' 


V = — (1 4- COS 87r) 8ZiF. 

Thus for all values of s, 

and for odd values of 5, 
But when s is even, 

m + n 

^' = - 




\m + n 3a« ■** j ' SirnhH («^ - 1)* 
and the displacement w at any point (z, <f>) is given by 

w^2(A^'a-\- B^z) cos 2^ + 4 {A^a + B^z) cos 4<^ + . . .(16), 
where A^, JS/, -4/,... are determined by (14), (15). 

A further discussion of this solution will be found in the 
memoir' from which the preceding results have been taken. 

We will now proceed with the calculation for the frequencies 
of vibration of the complete cylindrical shell of length 21, If the 
volume-density' be p, we have as the expression of the kinetic 
energy by means of (9), (10), (11), 

T=i.2V.[j(i' + t)» + w»)arf^d-2 

= 2TrpUa 2 {a» (1 + s") {A, + i/') 

+ [i^ni +«') + «-*«'] W + ^/')} (17). 

^ Whatever the corvature of the surface, an area upon it may be taken so small 
as to behave like a plane, and therefore bend, in violation of Gauss's conditioD, 
when subjected to a force which is so nearly discontinuous that it varies sensibly 
within the area. 

9 Proc. Roy, Soc, vol 45, p. 105, 1888. 

' This can scarcely be confused with the notation for the ourvatore in the 
preceding parts of the investigation. 


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From the expressions for V and T in (13), (17) the types and 
frequencies of vibration can be at once deduced. The fact that 
the squares, and not the products, of A,, B,, are involved, shews 
that these quantities are really the normal co-ordinates of the 
vibrating system. If -4„ or ^/, vary as cosp^, we have 

P''^^m-f~n'^^ ^TT ^^^>- 

This is the equation for the frequencies of vibration in two 
dimensions, § 233. For a given material, the frequency is pro- 
portional directly to the thickness and inversely to the square 
on the diameter of the cylinder*. 

In like manner if Bg, or B,, vary as co&pt% we find 

8a' m -f n 

^' ^m+npa* «» + l , 3a' ^^^^- 

(«* + ««)? 

If the cylinder be at all long in proportion to its diameter, the 
difference between p/ and p, becomes very small. Approximately 
in this case 

,, - 3a' /m + n 1 \ ,^^^ 

P./i>.=i+2^(---^ (20); 

or, if we take m — 2n, « = 2, 

236 A. We now pass on to the consideration of spherical 
shells. The general theory of the extensional vibrations of a 
complete shell has been given by Lamb', but as the subject is 
of small importance from an acoustical point of view, we shall 
limit our investigation to the veiy simple case of Sjrmmetrical 
radial vibrations. 

If w be the normal displacement, the lengths of all lines upon 
the middle surface are altered in the ratio (a + w): a. In calcu- 
lating the potential energy we may take in (10) § 235 d 

6i = €a = w/a, w = ; 

1 There is nothing in these laws special to the cylinder. In the case of similar 
shells of any form, vibrating by pore bending, the frequency will be as the thick- 
nesses and inversely as corresponding areas. If the similarity extend also to the 
thickness, then the f^qnency is inversely as the linear dimension, in accordance 
with the general law of Cauchy. 

* Proe, Land. Math, 8oe. xiv. p. 50, 1882. 

R. 27 

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80 that the energy per unit area is 

. , 3m — n w* 
4fnh ; 1, 

or for the whole sphere 

F=47ro».4nA?''^^^ (1). 

ni + n a' 

Also for the kinetic energy, if p denote the volume density, 

T^^.*7ra'.2h.p.w' (2). 

Accordingly if w = TT cos pt, we have 


^ a^p m + n ^ ^' 

as the equation for the frequency (p/^ir). 

As regards the general theory Prof. Lamb thus summarizes his 
results. "The fundamental modes of vibration fall into two 
classes. In the modes of the First Class, the motion at every 
point of the shell is wholly tangential. In the nth species of 
this class, the lines of motion are the contour lines of a surface 
harmonic Sn (Ch. xvii.), and the amplitude of vibration at any 
point is proportional to the value of dSn/de, where de is the angle 
subtended at the centre by a linear element drawn on the surface 
of the shell at right angles to the contour line passing through the 
point. The frequency {p/^ir) is determined by the equation 

k»a» = (w-l)(rH-2) (i), 

where a is the radius of the shell, and k"=p*/o/n, if p denote the 
density, and n the rigidity, of the substance." 

" In the vibrations of the Second Class, the motion is partly 
radial and partly tangential. In the nth species of this class the 
amplitude of the radial component is proportional to 5^, a surface 
harmonic of order n. The tangential component is everywhere at 
right angles to the contour lines of the harmonic Sn on the surface 
of the shell, and its amplitude is proportional to AdSn/de, where 
A is a certain constant, and de has the same meaning as before." 
Prof. Lamb finds 

. k^a»-47 .... 

^ = -2ri(n + l)7 ^""^^ 

where k retains its former meaning, and 7 = (1 + <r)/(l — <r), a 

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235 A.] 



denoting Poisson's ratio. " Corresponding to each value of n there 
are two values of k*a*, given by the equation 

k* a*- k»a*{(n« + nH-4)7H-n«H-n- 2} +4 (n» + n- 2)7 = 0.. .(iii). 

Of the two roots of this equation, one is < and the other > 47. It 
appears, then, firom (ii) that the corresponding fundamental modes 
are of quite diflferent characters. The mode corresponding to the 
lower root is always the more important." 

" When n =s 1, the values of k»a* are and 67. The zero root 
corresponds to a motion of translation of the shell as a whole 
parallel to the axis of the harmonic Si. In the other mode the 
radial motion is proportional to cos d, where is the co-latitude 
measured from the pole of Si ; the tangential motion is along the 
meridian, and its amplitude (measured in the direction of in- 
creasing) is proportional to i sin 0." 

*' When n = 2, the values of ka corresponding to various values 
of a are given by the following table : — 

<r = 

<r = J 

<^ = A 

«r = ^ 

«r = i 






The most interesting variety is that of the zonal harmonic. 
Making 5=^(3 cos' 6^—1), we see that the polar diameter of 
the shell alternately elongates and contracts, whilst the equator 
simultaneously contracts and expands respectively. In the mode 
corresponding to the lower root, the tangential motion is towards 
the poles when the polar diameter is lengthening, and vice versd. 
The reverse is the case in the other mode. We can hence under- 
stand the great diflFerence in frequency." 

Prof. Lamb calculates that a thin glass globe 20 cm. in 
diameter should, in its gravest mode, make about 5350 vibrations 
per second. 

As re^rds inextensional modes, their form has already been 
determined, (39) &c. § 235 c, at least for the case where the 
bounding curve and the thickness are sjrmmetrical with respect 
to an axis, and it will further appear in the course of the present 
investigation. What remains to be effected is the calculation of 

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the potential energy of bending corresponding thereto, as depend- 
ent upon the alterations of curvature of the middle surfSaoe. The 
process is similar to that followed in § 235^ for the case of the 
cylinder, and consists in finding the equation of the deformed 
surface when referred to rectangular axes in and perpendicular 
to the original surface. 

The two systems of co-ordinates to be connected are the usual 
polar co-ordinates r, 0, ^, and rectangular co-ordinates a?, y, j; 
measured from the point P, or (a, 0o, ^o)i on the undisturbed 
sphere. Of these x is measured along the tangent to the 
meridian, y along the tangent to the circle of latitude, and ^ 
along the noimal inwards. 

Since the origin of ^ is arbitrary, we may take it so that 
^0 — 0. The relation between the two systems is then 

a? = r {— sin (d - ^o) + sin cos 0o (1 — cos ^)} (4). 

ysrsindsin^ (5), 

?= — r {cos (0 — ^o) — sin dosin d (1 — cos ^)} + a ....(6). 

If we suppose r = a, these equations give the rectangular 
co-oitlinates of the point (a, 0, <f>) on the undisturbed sphere. 
We have next to imagine this point displaced so that its polar 
co-ordinates become a + Sr, + h0, 4> + ^> ^^^ to substitute these 
values in (4), (5), (6), retaining only the first power of Sr, S0, S^ 

a?=:(a + Sr) {— mi (0 — 0o) + sin cos 0q{1 — cos^)} 
H- aB0 {- co8{0 - 0o) + coa0 cos 0o (I - cos <^)} 
+ aS^ sin 5 cos do sin ^ (7), 

y = (a H- Sr) sin d sin ^ 

-{■ aB0 COB sin <f> + aB^ sin 0co8(f> (8), 

^^a-ia + Sr) [qos(0 - do) -sin 0o sin d (1 - cos <^)} 

+ aB0 {sin (0 - 0^) + sin do cos d (1 - cos if>)} 

+ aS^sindosindsin^ (9X 

These equations give the co-ordinates of any point Q of the sphere 
after displacement ; but we shall only need to apply them in the 
case where Q is in the neighbourhood of P, or (a, do, 0), and then 
the higher powers of (d — d©) and <f> may be neglected. 

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In pursuance of our plan we have now to imagine the displaced 
and deformed sphere to be brought back as a rigid body so that 
the parts about P occupy as nearly as possible their former 
positions. We are thus in the first place to omit from (7), (8), 
(9) the terms (involving S) which are independent of {6 — d©), ^• 
Further we must add to each equation respectively the terms 
which represent an arbitrary rotation, viz. 

determining to^, a>„ co, in such a manner that, so far as the first 
powers of {0 — do), ^, there shall be coincidence between the original 
and displaced positions of the point Q, 

If we omit all terms of the second order m {0 — 0q) and ^, we 
get ft^m (7) &c. 

a; = - a (d - do) - ^o(0- Oo) 

-a|[S«o] + ^(d-do)-h^<^| + aS^8indoC08do.*... (10), 
y = a sin do- ^ + 8n sin 0o.<f> + aB0o cos 0o . ^ 

+ a sin d< 


+ aB<l>, COB 0,(0-0,) (11), 


+ a80o{0-0o) + aBif>oBm*0o.if> (12), 

Sto &C. representing the values appropriate to P, where (0 — 0o) 
and <f> vanisL The translation of the deformed surface necessary 
to bring P back to its original position is represented by the 
omission of the terms included in square brackets. The arbitrary 
rotation is represented by the additions respectively of 

a sin do . ^ . 0),, a (d — d©) co,, — a (d — do) a)j — a sin do . ^ . c»i ; 
and thus the destruction of the terms of the first order requires 

Sr/a + dSd/dd = (13), 

-dSd/d<^ + 8indcosdS^+sindo), = (14); 

sin d dS<^/dd + COB dS<^ + 0)5 = (15), 

(Sr/a) sin d + Sd cos d + sin dd8^/d^«0 (16); 

-d8(r/a)/dd + Sd-a), = (17), 

- dS (r/a)/d<^ H-8in«d8<^- sin d 0)1=0 (18); 

the suffixes being omitted. 

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These six equations determine c^i, 6),, co,, giving as the three 
conditions of inextension 

Br/a + dS0/d0^O (19), 

dB0/d<f> + sin^edB<l>/de^O (20), 

Br/a + cote 80 + ^ld(l>=^0 (21). 

From (19), (20). (21), by elimination of Br, 

»(^.)--*w-° <^>. 

^«*--'a(^)'« <^>^ 

or, since sin 6 djdd = djd log tan i^, 

d^Un^y^dlogtanid'"" ^^*^' 

d<f> dlogtani^Und/ ^ ^ 

From (24), (25) we see that both B^ and B6/sin satisfy an 
equation of the second order of the same form, viz. 

d^U . *^ _ A /«fiX 

diiogtan^ey'^ d4>^^ ^ ^• 

If the material system be symmetrical about the axis, ti is a 
periodic function of ^, and can be expanded by Fourier's theorem 
in a series of sines and cosines of ^ and its multiples. Moreover 
each term of the series must satisfy the equations independentlj. 
Thus, if t* varies as cos«0, (26) becomes 

diio^lw -'''''' ^''^'' 

whence u = A'taa*^e + B'cof^ (28). 

where A' and R are independent of 0. If we take 

S^ = co8«<^[il,tan'id + 5,cot»i^] (29), 

we get for the corresponding value of Sd from (24) 

S^/sin ^ = - sin «0 [A, tan* ^6 - B, cot* ^ef\ (30) ; 

and thence from (21) 
h-ja = sin «0 [A, (« + cos d) tan' ^d + B,{8-ws 0) cot* i^. . .(31), 
as in (39), (40), (41) § 235 c. 

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The second solution (in Bg) may be derived from the first (in Ag) 
in two ways which are both worthy of notice. The manner of deri- 
vation from (27) shews that it is sufficient to alter the sign of s, 
tan* ^6 becoming cot*^^, sin*^ becoming — sin*^, while cos«^ 
remains unchanged. The other method depends upon the con- 
sideration that the general solution must be similarly related to 
the two poles. It is thus legitimate to alter the first solution by 
writing throughout (tt — 0) in place of 0, changing at the same 
time the sign of hd. 

If we suppose « = 1, we get 

sin 0hit> = cos ^ [ill + 5i - (^1 - A) cos 0\ 

Sd = - sin <^ [ill - jBj - (ill + 50 cos ^], 

Sr/a = sin <^ [(^i + B^) sin 0], 

The displacement proportional to (ilj — B^ is a rotation of the 
whole surface as a rigid body round the axis — ^, ^ = ; and 
that proportional to {Ai + Bi) represents a translation parallel to 
the axis — \ir, ^ = ^7r. The complementary translation and 
rotation with respect to these axes is obtained by substituting 
^ + |7r for ^. 

The two other motions possible without bending correspond to 
a zero value of 8, and are readily obtained from the original 
equations (19), (20), (21). They are a rotation round the axis 
^ = 0, represented by 

Sd = 0, S^ = const., Sr = 0, 

and a displacement parallel to the same axis represented by 

or S^ = 0, S^ssysind, Sr = — yacos^. 

If the sphere be complete, the displacements just considered, 
and corresponding to « = 0, 1, are the only ones possible. For 
higher values of 8 we see frt>m (31) that Sr is infinite at one or 
other pole, unless Ag and Bg both vanish. In accordance with 
Jellet's theorem^ the complete sphere is incapable of bending. 

If neither pole be included in the actual surface, which for 
example we may suppose bounded by circles of latitude, finite 

1 «<0n the Properties of Ineztensible Surfaces/* Irith Acad, Tram.^ vol. 22, 
p. 179, 1855. 

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values of both A and B are admissible, and therefore necessary for 
a complete solution of the problem. But if, as would more often 
happen, one of the poles, say ^ = 0, is included, the constants B 
must be considered to vanisL Under these circumstances the 
solution is 

S^=sil«tan'^^cos«^ \ 

Sd = -il,sindtan'idsin5^ I (32), 

Sr = ^,a (« H- cos ^) tan* ^^ sin «^ J 

to which is to be added that obtained by writing %^ + \ir for «^, 
and changing the arbitrary constant 

From (32) we see that, along those meridians for which 
sin 8^ = 0, the displacement is tangential and in longitude only, 
while along the intermediate meridians for which cos«^ = 0, there 
is no displacement in longitude, but one in latitude, and one 
normal to the surface of the sphere. 

Along the equator » ^, 

S^ = Ag cos 8<^, BO — '-Aa sin 8(f>, &r/a = AgS sin 8^, 

so that the maximum displacements in latitude and longitude are 

Reverting now to the expressions for x, y, f in (7), (8), (9), 
with the addition of the translatory and rotatory terms by which 
the deformed sphere is brought back as nearly as possible to its 
original position, we know that so fiu* as the terms of the first 
order in (d — 0o) and <f> are concerned, they are reduced to 

a? = -a(d-^o), y = asindo.^, ?=0 (33). 

These approximations will suffice for the values of x and y ; but 
in the case of (f we require the expression complete so as to 
include all terms of the second order. The calculation is straight- 
forward For any displacement such as Br in (9) we write 

The additional rotatory terms are by (17), (18) 

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In these we are to retain only those terms in x, y, which are of the 
second order and independent of B, so that we may write 

X = ia^» sin do cos ^o, y = a(0- 0^) if> cos 0^. 

In the complete expression for f as a quadratic function of 
{0 — 0^) and ^ thus obtained, we substitute x and y from (33). 
The final equation to the deformed surfiwe, after simplification by 
the aid of (19), (20), (21), may be written 

r= — II- — -1*^4-— ^J-1 ^^ cotddSr| 
^ 2a( a ad^J asindj ad0d4 » #J 

y^L_Sr_cotddSr_ I cP8r ] 
'^2a( a a" dd asin»d d<^»J ^"^ ^' 

the suffixes being now unnecessary. 

Taking the value of ^/a from (32) we get 

"a~ad^~=^"8i5^^'*^^*^«"^^* (3o), 

1 (?8r , cosd dSr «•-« . , .,^ 
^/i T/ijvH- . i/i-Ti =— .-^r7i-^,tan'+dcos«<p ....(36), 

Sr cotddSr 1 d^hr «»-* . ^ .,^. ^ .^^^ 

- -J/, 7-T-^ ,—- = -.— ^ il, tan* \0 sm «6. ..(37). 

a a d0 a sm* d d^» sm* ' ^ i' \ / 

To obtain the more complete solution corresponding to (31), we 
have only to add new terms, multiplied by B„ and derived from 
the above by changing the sign of 8. As was to be expected, the 
values in (35) and (37) are equal and opposite. 

Introducing the values now found into (5) § 235/, we obtain 
as the square of the change of principal curvature at any point 

' ^^f ^ [Af tan" ^0 + 5,» cot" \0 - iA,B, cos 28if>] . . .(38). 

It should be remarked that, if either A^ or B, vanish, (38) is 
independent of ^, so that the change of principal curvature is the 
same for all points on a circle of latitude, and that in any case 
(38) becomes independent of the product AtB^ after integration 
round the circumference. The change of curvature vanishes if 
« = 0, or 8 » 1, the displacement being that of which a rigid body 
is capable. 

Equations (35) &c shew that along the meridians where S^ 
vanishes (cos^^^sO) the principal planes of curvature are the 


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meridian and its perpendicular, while along the meridians where 
Sr vanishes, the principal planes are inclined to the meridian at 
angles of 45^ 

The value of the square of the change of curvature obtained in 
(38) corresponds to that assumed for the displacements in (29) &c., 
and for some purposes needs to be generalised We may add 
terms with coefficients Ai and Bi corresponding to a change 
of 8^ to (^^ + ^), and there is further to be considered the 
summation with respect to s. Putting for brevity i in place of 
tan^d, we may take as the complete expression for [£(1/^)]*, 

[2^*^ {{A,i? + 5.rO sin s^ + {Aii? + 5;r») sin («^ + }9r)} j" 

+ [2 ~^-Q K^.** - 5«^~0 cos 8^ + {Ai^ - £/r*) COS («<^ + i^)l I* . 

When this is integrated with respect to ^ round the entire 
circumference, all products of the generalised co-ordinates A^^Bt^ 
Ai, Bi disappear, so that (7) § 235/ we have as the expression for 
the potential energy of the surface included between two parallels 
of latitude 

F = 27r 2 («» - bJ (h sin-» {(A,^ + A/^) t« 

+ {B.' + B.'*)tr^}d0 (39), 

where H^^nh^ (40). 

In the following applications to spherical surfaces where the 
pole d = is included, we may omit the terms in B; and, if 
the thickness be constant, H may be removed from under the 
integral sign. We have 

dO — ^ — -, sm^ = ; 

so that 


In the case of the hemisphere ^=1, and (41) assumes the value 

2«» — 1 

4^ <*2). 

Hence for a hemisphere of uniform thickness 

F=fn-fr2(«'-«)(2««-l)(^« + ^'») (43). 

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If the extreme value of d be 60°, instead of 90°, we get in 
place of (42) 

S^ + ^8-3 .... 


and V = iyrHl. 3-<'+») («» - «) (8«« + 4« - 3) (^l,* + ^;«). . .(45). 

These expressions for F, in conjunction with (32), are suflScient 
for the solution of statical problems, relative to the deformation of 
infinitely thin spherical shells under the action of given impressed 
forces. Suppose, for example, that a string of tension F connects 
the opposite points on the edge of a hemisphere, represented by 
d = ^, ^ = i^ or fw, arid that it is required to find the deforma- 
tion. It is evident from (32) that all the quantities A/ vanish, 
and that the work done by the impressed forces, corresponding to 
the deformation BAg, is 

— SAgOS {sin ^STT + sin ^sir} F. 

If 8 be odd this vanishes, and if 8 be even it is equal to 

— 2SAga8 sin ^87r.F. 

Hence if « be odd Ag vanishes ; and by (43), if 8 be even, 


whence ^, = _ _^___^__^ (46). 

By (46) and (32) the deformation is completely determined. 

If, to take a case in which the force is tangential, we suppose 
that the hemisphere rests upon its pole with its edge horizontal, 
and that a rod of weight W is laid symmetrically along the 
diameter 0'^^v, we find in like manner 

A _ aW sin ^87r ..^ 

^•"7rff(^-5)(2^-l) ^*'^ 

for all even values of 8, and Ag^O for all odd values of 8. 

We now proceed to evaluate the kinetic energy as defined by 
the formula 

in which <r denotes the surface density, supposed to be uniform. 

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If we take the complete value of S<f> from (29), as supplemented by 
the terms in A/, £/, we have 

^^^ = 2 [cos 8if> (A,if + Bstr*) + cos (««^ + ^w) (A/f + £/(-•)]. 

When this expression is squared and integrated with respect 
to <f> round the entire circumference, all products of letters with a 
different sufiSx, and all products of dashed and undashed letters 
even with the same suflSx, will disappear. Hence replacing cofi**^ 
&c. by the mean value' i, we may take 

sin»d(^^*y = isin»dS(i,» + i/0«»' 

+ isin»d2W + B;»)r« + 8in»d2(i,5. + i;5,'). 

The mean value (30) of {dZOjdty is the same as that just 
written with the substitution throughout of — B for B, so that we 
may take 

^?^|^y = sin«^2(4.»-h^'»)^« 

H-sin»d2(4' + Mt-^ (*9), 

as the mean available for our present purpose. In (49) the 
products of the symbols have disappeared, and if the expression 
for the kinetic energy were as yet fully formed, the co-ordinates 
would be shewn to be nomud. But we have still to include that 
part of the kinetic energy dependent upon d8r/dt As the mean 
value, applicable for our purpose, we have from (31) 

+ J 2 (4' + 5.'') (» - COS d)* r" 

+ 2 (A.B, + A,'B,') («» - cos' e) (50). 

The expressions (49) and (oO) have now to be added. If we set 
for brevity 

jtaa''^0{(8 + co6ey + 2Bia'0] sin edd=/(8) (51), 

or putting x — l + cos 0, 

f{8)^j*(^)'{(8-iy + 2x(s + l)-a*}dx (52), 

Digitized by VjOOQ IC 


we get 

T = i^cra* {2/(«) (i.« + i/«) + 2/(- 8) (4' + 5;«) 

+ 22f(«»-co8'd)8m^dd(i,iB. + i;j^/)} (53). 

It will be seen that, while V in (39) is expressible by the 
squares only of the co-ordinates, a like assertion cannot in general 
be made of T. Hence A^y B, &c. are Tiot in general the normal 
co-ordinates. Nor could this have been expected. If, for example, 
we take the case where the spherical surface is bounded by two 
circles of latitude equidistant from the equator, symmetry shews 
that the normal co-ordinates are, not A and £, but {A -h B) and 
{A - B). In this case /(- s) =f(s). 

A verification of (53) may readily be obtained in the particular 
case of « = 1, the surface under, consideration being the entire 
sphere. Dropping the dashed letters, we get 

T = iTTcra^ {^ (i,» -h A') + f ii A} 

= i7rcra*{ 4(i, -h A)* + f (ii - A)"} (54). 

In this case the displacements are of the purely translatory and 
rotatory tjrpes already discussed, and the coiTCCtness of (54) may 
be confirmed. 

Whatever may be the position of the circles of latitude by 
which the surfisuje is bounded, the true types and periods of 
vibration are determined by the application of Lagrange's method 
to (39), (53). 

When one pole, e.g. d = 0, is included within the surface, the 
co-ordinates B vanish, and il,, A/ become the normal co-ordinates. 
If we omit the dashed letters, the expression for T becomes 

r=iircra*2/(«)i,» (55). 

From (43), (55) the frequencies of free vibrations for a hemi- 
sphere are immediately obtainable. The equation for A, ia 

<ra'f{8)As'{-H(8'-8)i2^^1)A,^0 (56); 

so that, if Ag vary as coapat, 

^,_fl^(^-^)(25»-l) 2nh' (^■^^)(2^-l) , .. 

p' — ^v(.) ^s^^' m ^ ^' 

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if we introduce the value of H from (40), and express a by means 
of the volume density p. 

In like manner for the saucer of 120°, from (44), 

^,_ g(^-^)(8^ + 4g-3) 

P' craV(.).3*+^ ^^^^- 

The values of /(«) can be calculated without difficulty in the 
various cases. Thus, for the hemisphere, 

/(2)= I ar-«(4 - ^x •\' a?){\ +Qx -- a?)dx 

= 20 log 2 - 12^ = 1-52961, 

/(3) = 57^ - 80 log 2 = 1-88156, 

/(4) = 200 log 2 - 136i = 2-29609, &c. ; 
so that 

i>,=-^-^x 5-2400, ^,= ^x 14-726, p^ = -xT" x 28462. 

In experiment, it is the intervals between the various tones 
with which we are most concerned. We find 

jt)8/pa = 2-8102, jt)4/p2 = 5-4316 (59). 

In the case of glass bells, such as are used with air-pumps, 
the interval between the two gravest tones is usually somewhat 
smaller ; the representative fraction being nearer to 2-5 than 2*8. 

For the saucer of 120°, the lower limit of the integral in (52) 
is |, and we get on calculation 

/(2) = -12864, /(3) = -054884, 

S^^^^S P^-St^^^''''^^ ^' = 0^:^^20-911, 

;)8:jt),= 2-6157. 

The pitch of the two gravest tones is thus decidedly higher than 
for the hemisphere, and the interval between them is less. 

With reference to the theory of tuning bells, it may be worth 
while to consider the effect of a small change in the angle, for the 
case of a nearly hemispherical bell. In general 

^Hif-syi sin-»dtan*'iddd 

i>.^ n -.(60). 

aV tan" \e [{a + cos 0^ + 2 sin* 0] sin 0d0 

Digitized by 




If 0^^ + B0, and P, denote the value of p^ for the exact hemi- 
sphere, we get from previous results 

K=P.' [i + s^ Iff -r^el] = ^«* (^ -2««^)' 

shewing that an increase in the angle depresses the pitch. As to 
the interval between the two gravest tones, we get 

shewing that it increases with 0. This agrees with the results 
given above for = 60°. 

The fact that the form of the normal functions is independent 
of the distribution of density and thickness, provided that they 
vary only with latitude, allows us to calculate a great variety of 
cases, the difficulties being merely those of simple integration. If 
we suppose that only a narrow belt in co-latitude has sufficient 
thickness to contribute sensibly to the potential and kinetic 
energies, we have simply, instead of (60), 

P' a^a{(8 + coa0y + 28m^0] ^^^^' 

whence ^' = 4 /r 6 + 4cosg-cos«g ) 

Whence p."" V tll + 6cosd«cos«d{ ^^^^• 

The ratio varies very slowly from 3, when = 0, to 2*954, when 
^ = j7r. 

If 2h denote the thickness at any co-latitude 0, Hcch\ aoc h. 
I have calculated the ratio of frequencies of the two gravest tones 
of a hemisphere on the suppositions (1) that hoc cob 0, and (2) that 
A oc (1 + cos 0). The formula used is that marked (60) with H and a- 
under the integral signs. In the first case, p^ipt^ 17942, differing 
greatly from the value for a uniform thickness. On the second 
more moderate supposition as to the law of thickness, 

Pz'.pt^ 2-4591, P4:pi = 4-4837. 

Digitized by VjOOQ IC 


It would appear that the smallness of the interval between the 
gravest tones of common glass bells is due in great measure to the 
thickness diminishing with increasing 0, 

It is worthy of notice that the curvature of deformation S(p~0» 
which by (38) varies as sin"* d tan* Jd, vanishes at the pole for 
« s 3 and higher values, but is finite for 8 — 2, 

The present chapter has been derived very largely from 
various published memoirs by the author^ The methods have 
not escaped criticism, some of which, however, is obviated by 
the remark that the theory does not profess to be strictly 
applicable to shells of finite thickness, but only to the limiting 
case when the thickness is infinitely small. When the thickness 
increases, it may become necessary to take into account certain 
" local perturbations " which occur in the immediate neighbourhood 
of a boundary, and which are of. such a nature as to involve 
extensions of the middle surface. The reader who wishes to 
pursue this rather difficult question may refer to memoirs by 
Love", Lamb', and Basset*. From the point of view of the present 
chapter the matter is perhaps not of great importance. For it 
seems clear that any extension that may occur must be limited to 
a region of infinitely small area, and affects neither the types nor 
the frequencies of vibration. The question of what preciselj 
happens close to a free edge may require further elucidation, but 
this can hardly be expected fix>m a theory of thin shells. At 
points whose distance from the edge is of the same order as the 
thickness, the characteristic properties of thin shells are likely to 

1 Proc, Land. Math. Soc, xiii. p. 4, 1881 ; xx. p. 372, 1889 ; Proe. Ray. Soe., toL 
45, p. 106, 1888; Tol. 45, p. 448, 1888. 

» Phil Trans., 179(a), p. 491, 1888; Proc. Ray, Soc., vol. 49, p. 100, 1891; 
Theory of Elasticity, ch. xxi. 

> Proe. Land. Math. Soc, voL xxi. p. 119, 1890. 

« Phil. Trans. 181 (a), p. 488, 1890 ; Am. Math. Jaum., vol. xvi. p. 254, 1894. 

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235 i. The introduction of the telephone into practical use, 
and the numerous applications to scientific experiment of which 
it admits, bring the subject of alternating electric currents 
within the scope of Acoustics, and impose upon us the obligation 
of shewing how the general principles expounded in this work may 
best be brought to bear upon the problems presenting themselves. 
Indeed Electricity affords such excellent illustrations that the 
temptation to use some of them has ah^ady (§§ 78, 92 a, 111 6) 
proved irresistible. It will be necessary, however, to take for 
granted a knowledge of elementary electrical theory, and to abstain 
for the most part from pursuing the subject in its application to 
vibrations of enormously high frequency, such as have in recent 
years acquired so much importance from the researches initiated 
by Lodge and by Hertz. In the writings of those physicists and in 
the works of Prof. J. J. Thomson^ and of Mr O. Heaviside* the 
reader will find the necessary information on that branch of the 

The general idea of including electrical phenomena under those 
of ordinary mechanics is exemplified in the early writings of Lord 
Kelvin ; and in his " Dynamical Theory of the Electro-magnetic 
Field' " Maxwell gave a systematic exposition of the subject from 
this point of view. 

^ Recent Researches in Electricity and Magnetism^ 1898. 

s Electrical Papers, 1892. 

' Phil, Trans. Yol. 155, p. 459, 1865 ; CoUeeted Works, vol. 1, p. 526. 

R, ' 28 

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236/ We commence with the consideration of a simple 
electrical circuit, consisting of an electro-magnet whose terminab 
are connected with the poles of a condenser, or Uyden}, of capacity 
(7. The electro*magnet may be a simple coil of insulated wire, of 
resistance i2, and of self-induction or inductance L. If there be an 
iron core, it is necessary to suppose that the metal is divided so as 
to avoid the interference of internal induced currents, and further 
that the whole change of magnetism is small*. Otherwise the 
behaviour of the iron is complicated with hysteresis, and its effect 
cannot be represented as a simple augmentation of L. Also for 
the present we will ignore the h3rstere8is exhibited by many kinds 
of leydens. 

If X denote the charge of the leyden at time t, a: is the 
current, and if i^icosj^^ be the imposed electro-motive force, the 
equation is 

Lx'hRx'\-x/C^EiCOBpt (1). 

The solution of (1) gives the theory ot forced electrical vibrations; 
but we may commence with the consideration of the free vibra- 
tions corresponding to Ei^O. This problem has already been 
treated in § 45, from which it appears that the currents are 

oscillatory, if 

R<2^(L/C) (2). 

The fact that the discharges of leydens are often oscillatory was 
suspected by Henry and by v. Helmholtz, but the mathematical 
theory is due to Kelvin*. 

When R is much smaller than the critical value in (2). a lai^ 
number of vibrations occur without much loss of amplitude, and 
the period r is given by 

T = 27rV((7Z) (3). 

In (2), (3) the data may be supposed to be expressed in CG.s. 
electro-magnetic measure. If we introduce practical units, so 
that L\ R\ C represent the inductance, resistance and capacity 
reckoned respectively in earth-quadrants or henrys, ohms, and 
microfarads*, we have in place of (2) 

iJ'<2000V(Z7C") (2-), 

1 This term has been approved by Lord Kelvin (" On a New Form of Aii Lejdefl 
<fec.*' Proc. Roy, Soe., vol. 62, p. 6, 1892). 
« Phil Mag., vol. 23, p. 226, 1887. 

s ** On Transient Electric Currents," Phil. Mag., Jane, 185S. 
< Ohm=:10», henry =10*, microfarad =10"". 

Digitized by 



and in place of (3) 

T = 27r.lO-V(C7'2;0 (30. 

With ordinary appliances the value of t is very small ; but by 
including a considerable coil of insulated wire in the discharging 
circuit of a leyden composed of numerous glass plates Lodge ^ has 
succeeded in exhibiting oscillatory sparks of periods as long as 

If the leyden be of infinite capacity or, what comes to the 
same thing, if it be short-circuited, the equation of free motion 
reduces to 

Z« + jRi«0 (4); 

whence x^di^er<^l^^* (5)», 

io representing the value of x when ^ = 0. The quantity LjR is 
sometimes called the time-constant of the circuit, being the time 
during which free currents fall off in the ratio of 6 : 1. 

Returning to equation (1), we see that the problem falls under 
the general head of vibrations of one degree of freedom, discussed 
in § 46. In the notation there adopted, w' = (CZ)-^ k^R/L, 
EssEJL; and the solution is expressed by equations (4) and (5). 
It is unnecessary to repeat at length the discussion already given, 
but it may be well to call attention to the case of resonance, 
where the natural pitch of the electrical vibrator coincides with 
that of the imposed force (p^LC^l). The first and third terms 
then (§ 46) compensate one another, and the equation reduces to 

Rx^E^coapt (6). 

In general, if the leyden be short-circuited ((7= oo ), 


^ "" Dj^Xb^ ^^ cos j>^ -I- J)/; sin pt] ..(7); 

so that, if p much exceed JR/X, the current is greatly reduced by 
self-induction. In such a case the introduction of a leyden of 
suitable capacity, by which the self-induction is compensated, 
results in a large augmentation of current*. The imposed electro- 
motive force may be obtained from a coil forming part of the 
circuit and revolving in a magnetic field. 

1 Ptoc. Roy. ImU, March, 1SS9. 
' Helinholtz, Pogg. Arm., lzxzzii., p. 505, 1851. 

» Maxwell, «* Experiment in Magneto-Electric Induction," Phil. Mag., May, 


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In any circuit, where vibrations, whether forced or free, pro- 
portional to cos pt are in progress, we have x s —p^x, and thus the 
terms due to self-induction and to the leyden enter into the 
equation in the same manner. The law is more readily expressed 
if we use the stifftiess /a, equal to 1/(7, rather than the capacity 
itself. We may say that a stiffness fi compensates an inductance 
£, if fi^p^L, and that an additional indtlctance AX is compensated 
by an additional stiffness A/t, provided the above proportionality 
hold good This remark allows us to simplify our equations by 
omitting in the first instance the stiffness of leydens. When the 
solution has been obtained, we may at any time generalise it 
by the introduction, in place of Z, of L — /fP"^, or Z — (p^CyK In 
following this course we must be prepared to admit negative 
values of L, 

235 k. We will next suppose that there are two independent 
circuits with coefficients of self-induction L, N, and of mutual 
induction M, and examine what will be the effect in the second 
circuit of the instantaneous establishment and subsequent main- 
tenance of a current x in the first circuit. At the first moment 
the question is one of the function T only, where 

T^^Ldi' + Mxy + ^N^ (1); 

and by Kelvin's rule (§ 79) the solution is to be obtained by 
making (1) a minimum under the condition that x has the given 
value. Thus initially 

y.--f* (2); 

and accordingly (§ 235 j) after time t 

y = -^ie-(«W (3), 

if S be the resistance of the circuit. The whole induced current, 
as measured by a ballistic galvanometer, is given by 

'.,. Mx ... 

y* = --^- (4), 

in which N does not appear. The current in the secondary circuit 
due to the cessation of a previously established steady current x in 
the primary circuit is the opposite of the above. 

A curious property of the initial induced current is at once 
evident from Kelvin's theorem, or from equation (2). It appears 


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that, if if be given, the initial current is greatest when N is least. 
Further, if the secondary circuit consist mainly of a coil of n turns, 
the initial current increases with diminishing n. For, although 
ifxw, Nocn*; and thus yoal/n. In fact the small current 
flowing through the more numerous convolutions has the same 
effect as regards the energy of the field as the larger current in the 
fewer convolutions. This peculiar dependence upon n cannot be 
investigated by the galvanometer, at least without commutators 
capable of separating one part of the induced current from the 
rest ; for, as we see from (4), the galvanometer reading is affected 
in the reverse direction. It ia possible however to render evident 
the increased initial current due to a diminished n by observing 
the magnetizing effect upon steel needles. The magnetization 
depends mainly upon the initial maximum value of the current, 
and in a less degree, or scarcely at all, upon its subsequent 
duration. ^ 

The general equations for two detached circuits, influencing 
one another only by induction, may be obtained in the usual 
manner from (1) and 

F^^Rx'^^Sy' (5). 

Thus Lx + My-^Rx^X) . 

ifir + i\ry + Sy=F| ^^^• 

These equations, in a more general form, are considered in 
§ 116. If a harmonic force X ^e^^* act in the first circuit, and 
the second circuit be free from imposed force (F=0), we have on 
elimination of y 

shewing that the reaction of the secondary circuit upon the first is 
to reduce the inductance by 

P* ^*^ (8)« 

P p'N^ + S' ^°'' 

and to increase the resistance by 

^ p^N'^8- ^^^• 

1 PhU, Mag,, vol. 8S, p. 1, 1869 ; vol. 89, p. 428, 1870. 

< MazweU, Phil, Tram,, vol 155, p. 459, 1865, where, however, Af* is mis- 
printed M. 

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The formula (8) and (9) may be applied to deal with a more 
general problem of considerable interest, which arises when (as in 
some of Henry's experiments) the secondary circait acts upon a 
third, this upon a fourth, and so on, the only condition being that 
there must be no mutual induction except between immediate 
neighbours in the series. For the sake of distinctness we will 
limit ourselves to four circuits. 

In the fourth circuit the current is due ex hypothetn only to 
induction from the third. Its reaction upon the third, for the rate 
of vibration under contemplation, is given at once by (8) and (9) ; 
and if we use the complete values applicable to the third circuit 
under tliese conditions, we may thenceforth ignore the fourth 
circuit In like manner we can now deduce the reaction upon 
the secondary, giving the effective resistance and inductance of 
that circuit under the influence xrf the third and fourth circuits ; 
and then, by another step of the same kind, we may arrive at the 
values applicable to the primary circuit, under the influence of Wl 
the others. The process is evidently general; and we know by 
the theorem of § 111 6 that, however extended the train of circuits, 
the influence of the others upon the first must be to increase its 
effective resistance and diminish its effective inertia, in greater 
and greater degree as the frequency of vibration increasea 

In the limit, when the frequency increases indefinitely, the 
distribution of currents is determined by the induction-coefficients, 
irrespective of resistance, and, as we shall see presently, it is of 
such a character that the currents are alternately opposite in sign 
as we pass along the series. 

236 1. Whatever may be the number of independent currents, 
or degrees of freedom, the general equations are always of the 
kind already discussed g 82, 103, 104, viz. 

ddTdFdV^y . 

didx'^di^d^^^ ^ ^' 

where T,F, Fare (§ 82) homogeneous quadratic functions. In(l) 
the co-ordinates a^, ajj, ... denote the whole quantity of electricity 
which has passed at time t, the currents being £i, ^, &c. When 
F«0, it is simpler to express the phenomena by means of the 
currents. Thus, in the problem of steady electric flow where all 

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the quantities X, representing electro-motive forces, are constant, 
the currents are determined directly by the linear equations 

dFjdik^Xu dF/dx^^X^,Sic (2). 

On the other hand when the question under consideration is 
one of initial impulsive effects, or of forced vibrations of ex- 
ceedingly high frequency, everything depends upon T, and the 
equations reduce to 

d dT ^ d dT «. p .^v 

didAT^'' didi,'^*'^ ^^>- 

As an example we may consider the problem, touched upon at 
the close of § 235 &, of a train of circuits where the mutual induc- 
tion is confined to immediate neighbours, so that 

+aiaa?iJJi+aa,ajja:a-|-a,4^sa?4-|- (4)^ 

coefficients such as au, 014, o^ not appearing. If ^ be given, 
either as a current suddenly developed and afterwards maintained 
constant, or as a harmonic time function of high frequency, while 
no external forces operate in the other circuits, the problem 
is to determine x^, x^, Sic so as to make T as small as possible, 
§ 79. The equations are easily written down, but the conclusion 
aimed at is perhaps arrived at more instructively by consideration 
of the function T itself. For, T being homogeneous in Xi^x^, &c., 
we have identically 

''■-'•'£*'•'£,* <»)• 

And, since when T is a minimum, dT/dx^, dT/dx^, &c., all vanish, 


But if a?2, a:,, &c., had all been zero, 2T would have been equal to 
OriiXiK It is clear therefore that chiXiX^ is negative ; or, as a^ is 
taken positive, the sign of x^ is the opposite to that of a^i. 

Again supposing Xi, x^ both given, we must, when T is a 
minimum, have dT/dx^, dT/dx^y &c., equal to zero, and thus 

^T^iTL = Oiia?!* + iOiiX^x^ + aj,a?8« -h 2a„ir,a?,. 
As before, 27 might have been 

' The dots sure omitted as unneoeBBaiy. 

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simply. The minimum value is necessarily less than this, and 
accordingly the signs of x^ and x^ are opposite. This argfument 
may be continued, and it shews that, however long the series may 
be, the induced currents are alternately opposite in sign^ a result 
in harmony with the magnetizations observed by Henry. 

In certain cases the minimum value of T may be very nearly 
zero. This happens when the coils which exercise a mutual 
inductive influence are so close throughout their entire lengths 
that they can produce approximately opposite magnetic forces at 
all points of space. Suppose, for example, that there are two 
similar coils A and B, each wound with a double wire (ili, -4,), 
{Bu -Ba), and combined so that the primary circuit consists of -4,, 
the secondary of A^ and Bi joined by inductionless leads, and the 
tertiary of B^ simply closed upon itself. It is evident that T is 
made approximately zero by taking x^^-^x^ and 5?, = — a:, = a-,. 
The argument may be extended to a train of such coils, however 
long, and also to cases where the number of convolutions in 
mutually reacting coils is not the same. 

In a large class of problems, where leyden effects do not occur 
sensibly, the course of events is determined by T and F simply. 
These functions may then be reduced to sums of squares ; and the 
typical equation takes the form 

ax + hx=^X (6). 

If X = 0, that is if there be no imposed electro-motive forces, the 
solution is 

x^d^e-^f^ (7). 

Thus any system of initial currents flowing whether in detached 
or connected linear conductors, or in ^olid conducting masses, may 
be resolved into " normal " components, each of which dies down 
exponentially at its own proper rate. 

A general property of the "persistences," equal to a/6, is 
proved in § 92 a. For example, any increase in permeability, due 
to the introduction of iron (regarded as non-conducting), or any 
diminution of resistance, however local, will in general bring about 
a rise in the values of all the persistences*. 

In view of the discussions of Chapter v. it is not necessary to 
dwell upon the solution of equations (1) when X is retained. The 

* PMl Mag., vol. 38, p. 18, 1869. 
' Bnt. Assoc. Report, 1886, p. 911. 

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reciprocal theorem of § 109 has many interesting electrical appli- 
cations ; but» after what has there been said, their deduction will 
present no difficulty. 

235 m. In § 111 6 one application of the general formulae to 
an electrical system has already been given. As another example, 
also relating to the case of two degrees of freedom, we may take 
the problem of two conductors in parallel It is not necessary to 
include the influence of the leads outside the points of bifurcation; 
for provided that there be no mutual induction between these parts 
and the remainder, their inductance and resistance enter into the 
result by simple addition. 

Under the sole operation of resistance, the total current a^ 
would divide itself between the two conductors (of resistances jR 
and S)in the parts 

8_ . R 

R + S""' ^"""^ RVS""''* 

and we may conveniently so choose the second co-ordinate that 
the currents in the two conductors are in general 

70:1 + a^a and t>T"c»^"'^2' 

Xi still representing the total current in the leads. The dissi- 
pation-function, found by multiplying the squares of the above 
currents by ^R, ^8 respectively, is 

^ = i^a'i' + K-B + 'S)^,' ^^)- 

Also, L, M, N being the induction coefficients of the two 

■'"* (R+sy '^^ 

Thus, in the notation of § 111 b, 

_ LS*+2MR8 + NR* (L-M)8 + (M-Jfr)R 

">'" {R + Sy ' "^'^ R + S 

ar,=^L-2M + N; 

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Accordingly by (5), (8) § 111 6, 

^,_L S' + 2MRS+NR^ {(£^itf)g + (if-iy^ii}« 

{{L^M)8-^(M-N)RY ... 

These are respectively the efiective resistance and the efifaetive 
inductance of the combination ^ It is to be remarked that 
(L — 2M + N) is necessarily positive, representing twice the kinetic 
energy of the system when the currents in the two conductors 
are + 1 and — 1. 

The expressions for R and L' may be put into a form' which 
for many purposes is more convenient, by combining the com- 
ponent fractional terms. Thus 

J., ^ RS(R + S)-^p^{R(M^Ny + S{L^My} . ,. 

(R'\'Sy+p^(L^2M^Ny ^ ^' 

in which {LN-^M^) is positive by virtue of the nature of T. 

As p increases from zero, we know by the general theorem 
§ 111 6, or from the particular expressions (3), (4), that B! con- 
tinually increases and that L' continually decreases. 

When p is very small, 

^, R8 J, ZS« + 2Jlfi2iSf + -yiJ« ,., 

^^R^^ ^ (RVsy ^^^- 

In this case the distribution of the main current between the 
conductors is determined by the resistances, and (§1116) the values 
of R: and L coincide respectively with 2F\x^, 2Tlx^\ The resist- 
ance is manifestly the same as if the currents were steady. 
On the other hand, when p is very great, 

p, R{M^Ny^^8{L-My LN^M- 

^ {L^2M-^Ny ' ^'L^2M+N-^''^' 

In this case the distribution of currents is independent of the 
resistances, being determined in accordance with Kelvin's theorem 

1 PhiL Mag,, vol. 21, p. 877, 18S6. 
3 J. J. Thomson, loc, eit. § 421. 

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.235 m.] CONTIGUOUS wires. 443 

in such a manner that the ratio of the currents in the two con- 
ductors is (N—M) : (L — M). As when p is small, the values in 
(6) coincide with 2F/xi\ 2,Tlx^. 

When the two wires composing the conductors in parallel are 
wound closely together, the energy of the field under high fre- 
quency may be very small. There is an interesting distinction to 
be noted here dependent upon the manner in which the con- 
nections are made. Consider, for example, the case of a bundle 
of five contiguous wires wound into a coil, of which three wires, 
connected in series so as to have maximum inductance, constitute 
one of the branches in parallel, and the other two, connected 
similarly in series, constitute the other branch. There is still an 
alternative as to the manner of connection of the two branches. 
If steady currents would circulate opposite ways {M negative), the 
total current is divided into two parts in the ratio 3 : 2, in such a 
manner that the more powerful current in the double wire nearly 
neutralises at external points the magnetic effects of the less 
poweifiil current in the triple wire, and the total energy of the 
system is very small. But now suppose that the connections are 
such that steady currents would circulate the same way in both 
branches {M positive). It is evident that the condition of mini- 
mum energy cannot be satisfied when the currents are in the same 
direction, but requires that the smaller current in the triple wire 
should be in the opposite direction to that of the larger current in 
the double wire. In feet the currents must be as 3 to — 2 ; so 
that (since on the same scale the total current is unity) the 
component currents in the branches are both numerically greater 
than the total current which is algebraically divided between 
them. And this peculiar feature becomes more and more strongly 
marked the nearer L and N approach to equality^ 

The unusual development of currents in the branches is, of 
course, attended by an augmented effective resistance. In the 
limiting case when the m convolutions of one branch are supposed 
to coincide geometrically with one another and with the n convo- 
lutions of the second branch, we have 

L\M\ N^m^ : mn : n\ 

andfrom(6) ^''"S^- 01 

1 Phil. Mag,, vol. 21, p. S76, 18S6. 

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an expression which increases without limit, as m and n approach 
to equality. 

The fact that under certain conditions the currents in both 
branches of a divided circuit may exceed the current in the mains 
has beeu verified by direct experiments Each of the three 
currents to be compared traversed short lengths of similar German- 
silver wire, and the test consisted in finding what lengths of this 
wire it was necessary in the various cases to include between the 
terminals of a high resistance telephone in order to obtain sounds 
of equal intensity. The variable currents were derived from a 
battery and scraping contact apparatus (§ 235 r), directly included 
in the main circuit. 

The general formulae (3'), (4') undergo simplification when the 
conductoi*s in parallel exercise no mutual induction. Thus, when 

Jlf = 0, 

_ RS( R + S) +i^ (RN^ + SD) 


If further K^O, (8) and (9) reduce to 

8[R(R + S)-^1^ D} LS^ 

^~ (R-^-Sy-^p^L' ' ^^{R + Sy + p^L^'-'^^^^- 

The peculiar features of the combination are brought out most 
strongly when 8, the resistance of the inductionless component, is 
great in comparison with 12. In that case if the current be steady 
or slowly vibrating, it flows mainly through fi, while the resistance 
and inductance of the combination approximate to 12 andZ respec- 
tively ; but if on the other hand the current be a rapidly vibrating 
one, it flows mainly through 8, so that the resistance of the combi- 
nation approximates to 8, and the inductance to zero. These 
conclusions are in agreement with (10). 

If the branches in parallel be simple electro-magnets, L and N 
are necessarily positive, and the numerator in (9) is incapable of 
vanishing. But, as we have seen, when leydens are admitted, this 
restriction may be removed. An interesting case arises when the 
second branch is inductionless, and is interrupted by a leyden of 

1 PhU. Mag,, vol. 22, p. 495, 1SS6. 

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capacity (7, so that i\r= — ((7p')"*^ while at the same time -B = fif. 
The latter condition reduces the numerator in (9) to 

Thus L vanishes, (i) when LCp^ = 1, and (ii) when CB^ = L. The 
first alternative is the condition that the loop circuit, considered 
by itself, should be isochronous with the imposed vibrations. 
The second expresses the equality of the time-constants of the two 
branches. If they be equal, the combination behaves like a simple 
resistance, whatever be the character of the imposed electro- 
motive forced 

235 n. When there are more than two conductors in parallel, 
the general expressions for the equivalent resistance and induc- 
tance of the combination would be very complicated ; but a few 
particular cases are worthy of notice. 

The first of these occurs when there is no mutual induction 
between the members. If the quantities relating to the various 
branches be distinguished by the suffixes 1, 2, 3, ..., and it Ehe 
the difference of potentials at the common terminals, we have 

E^{ipL, + It,)xj^{ipL^ + IL)x^^ .'...(1); 

by which R and L' are determined. Thus, if we write 

we have from (2) 

^F+7F~^' ^W+p^L^'^ ^^^' 

^'A'+fB" ^ ~ A*+p*JEP ^*^' 

Equations (3) and (4) contain the solution of the problem'. 
When p = 0, 

""~2(ij-')' {2(ie-)i ^''''■ 

When on the other hand p is very great, 

^""{2(1-0}"' ~2(X-^) ^^^' 

* Chxystal, "On the Differential Telephone," Edin. Trans., vol. 29, p. 615, 

« Phil. Mag., vol 21, p. 879, 1886. 

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Google _ 


Even when the mutual induction between varioos membeis 
cannot be neglected, tolerably simple expressions can be found for 
the equivalent resistance and inductance in the extreme cases otp 
infiuitely small or infinitely large. As has already been proved, 
(§111 b), the above-mentioned quantities then coincide in value 
with 2i7(a?, + ic, + ...)', and 2r/(iCi-|-a^ + ...)", and the calculation 
of these values is easy, inasmuch as the distribution of currents 
among the branches is determined in the first case entirely by F 
and in the second case entirely by T. Thus, when p is infinitely 
small, i^ is a minimum, and the currents are in proportion to the 
conductances of the several branches. Accordingly, if the induction 
coefficients of the branches be denoted, as in § 111 6, by Ou, o^, ... 
Oia, ttui •••> and the resistances by IZx, iZ,, &c., we have 

^■~'(i7ij,+i/ie,+..:)» ~i/ij,+i/ij,+ ... ^'^' 

^ " (l/iJ, + 1/B, 4- l/fi, + ...)» •••^^^• 

A similar method applies when p — oo, but the result is leas 
simple on account of the complication in the ratios of currents due 
to mutual induction \ 

235 0. The induction-balance, originally contrived by Dove 
for use with the galvanometer, has in recent years been adapted 
to the telephone by Hughes^ who has described experiments 
illustrating the marvellous sensibility of the arrangement. The 
essential features are a primary, or battery, circuit, in which 
circulates a current rendered intermittent by a make and break 
intennipter, or by a simple scraping contact, and a secondary 
circuit containing a telephone. By suitable adjustments the two 
circuits are rendered conjugate, that is to say the coefficient of 
mutual induction is caused to vanish, so as to reduce the telephone 
to silence. The introduction into the neighbourhood of a third 
circuit, whether composed of a coil of wire, or of a simple con- 
ducting mass, such as a coin, will then in general cause a revival 
of sound. 

The destruction of the mutual induction in the case of two flat 
coils can be aiTived at by placing them at a short distance apart, 

^ J. J. Thomson, loc. ciU § 422. 
« PhxL Mag, vol. vra., p. 60, 1879. 

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235 0.] hughes' induction balance, 447 

in parallel planes, and with accurately adjusted overlapping. But 
in Hughes' apparatus the balance is obtained more symmetrically 
by the method of duplication. Four similar coils are employed. 
Of these two Ai, A^, mounted at some distance apart with their 
planes horizontal, and connected in series, constitute the primary 
induction coiL The secondary induction coil consists in like 
manner of JBi, -Bj, placed symmetrically at short distances from 
^1, il„ and also connected in series, but in such a manner that 
the induction between Ai and Bi tends to balance the induction 
between A^ and B^. If the four coils were perfectly similar, 
balance would be obtained when the distances were equal. This 
of course is not to be depended upon, but by a screw motion the 
distance between one pair, e.g. Ai and Bi, is rendered adjustable] 
and in this way a balance between the two inductions is obtained. 
Wooden cups, fitting into the coils, are provided in such situations 
that a coin resting in one of them is situated symmetrically 
between the corresponding primary and secondar}' coils. The 
balance, previously adjusted, is of course upset by the introduction 
of a coin upon one side, but if a perfectly similar coin be intro- 
duced upon the other side also, balance may be restored. Hughes 
found that very minute differences between coins could be ren- 
dered evident by outstanding sound in the telephone. 

The theory of this apparatus, when the primary currents are 
harmonic, is simple ^ especially if we suppose that the primary 
current a?i is given. If a?i, a?,,... be the currents; 61,62,... the 
resistances; an, (hi, Oij, ... the inductances, the equations for 
the case of three circuits are 

We now assume that cci, a?s, &c. are proportional to 6*^*, where 
p/2'7r is the frequency of vibration. Thus, 

ip (OajflJa + as,a7,) -h 6ja?a = - iporu^i* 

ip ((hsCCi + a^a?,) + 6,a?, = — ipa^ooi ; 

whence by elimination of ic, 

a:Aipa^ + b. + J^\^^ipa..x,-P>^^ (2). 

1 Brit, Assoc. Rep. 1880, p. 472. 

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From this it appears that a want of balance depending on a^ 
cannot compensate for the action of the third circuit, so as to 
produce silence in the secondary circuit, unless bt be negligible 
in comparison with pa», that is unless the time-constant of the 
third circuit be very great in comparison with the period of the 
vibration. Otherwise the effects are in different phases, and 
therefore incapable of balancing. 

We will now introduce a fourth circuit, and suppose that the 
primary and secondary circuits are accurately conjugate, so that 
ais ~ 0, and also that the mutual induction o^ between the third 
and fourth circuits may be neglected. Then 

ip (a42^s + ^^44^4) + &4^4 = — tpcti4^ 5 

= — 0"^i i- ,- + ^ -xf W 

^ bpd^ + o^ tpa44 + 04) 

It appears that two conditions must be satisfied in order to 
secure a balance, since both the phases and the intensities of the 
separate effects must be the same. The first condition requires 
that the time-constants of the third and fourth circuits be equal, 
unless indeed both be very great, or both be very small, in com- 
parison with the period. If this condition be satisfied, balance 
ensues when 

?^ + 2^^ = (4): 

and it is especially to be noted that the adjustment is independent 
of pitch, so that (by Fourier's theorem) it sufiices whatever be the 
nature of the variable currents operative in the primary. 

As regards the position of the third and fourth circuits, usually 
represented by coins in illustrative experiments, it will be seen 
from the symmetry of the right-hand member of (3) that the 
middle position between the primary and secondary coils is suit- 
able, inasmuch as the product OuOn is stationary in value when 
the coin is moved slightly so as to be nearer say to the primaiy 

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and further from the secondary ^ Approximate independence of 
other displacements is secured by the geometrical symmetry of the 
coils round the axis. 

236 p. For the accurate comparison of electrical quantities 
the "bridge" arrangement of Wheatstone is usually the most 
convenient, and is equally available with the galvanometer in the 
case of steady or transitory currents, or with the telephone in the 
case of periodic currents. Similar effects may be obtained in most 
cases without a bridge by the employment of the differential 
galvanometer or the differential telephone*. 

In the ordinary use of the bridge the four members a, b, c, d 
combined in a quadrilateral Fig. (53 a) are 
simple resistances. The battery branch/ ^\^ ^' 

joins one pair of opposite comers, and the 
indicating instrument is in the "bridge" 
e joining the other pair. "Balance" is 
obtained, when ad — be. But for our 
purpose we have to suppose that any 
member, e.g. a, is not merely a resistance, 
or even a combination of resistances. It may include an electro- 
magnet, and it may be interrupted by a leyden. But in any case, 
so long as the current x is strictly harmonic, proportional. to e^^S 
the general relation between it and the difference of potentials V 
at the extremities is given by 

F=(ai + iaa)a; (1), 

where Oi and io, are the real and imaginary parts of a complex 
coefficient a, and are functions of the frequency p/2ir. In the 
particular case of a simple conductor, endowed with inductance L, 
ai represents the resistance, and a, is equal to pL. In general, Oi 
is positive; but a^ may be either positive, as in the above ex- 
ample, or negative. The latter case arises when a resistance R is 
interrupted by a leyden of capacity (7. Here ai = ii, a, = — l/pG, 
If there be also inductance i, 

a, = R, at^pL-l/pC (2). 

As we have already seen, § 235 j, Os may vanish for a particular 
frequency, and the combination is then equivalent to a simple 

> See Lodge, Phil. Mag., rol. 9, p. 123, 1S80. 
' Chrystal, Edin. Trans., loc. eit. 

R. 29 

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resistance. But a variation of frequency gives rise to a positive 
or negative a,. 

In all electrical problems, where there is no mutual induction, 
the generalize quantities, a, 6, &c., combine, just as they do when 
they represent simple resistances^ Thus, if a, a be two complex 
quantities representing two conductors in series, the corresponding 
quantity for the combination is (a + a). Again, if a, a represent 
two conductors in parallel, the reciprocal of the resultant i« given 
by addition of the reciprocals of a, a. For, if the currents be x, x , 
corresponding to a difference of potentials V at the common 

so that a: + a?' = F(l/a + 1/a'). 

In the application to Wheatstone*s combination of the general 
theory of forced vibrations, we will limit the impressed forces to 
the battery and the telephone branches. If x, y be the currents 
in these branches, X, Y the corresponding electro-motive forces, 
we have, § 107, linear relations between x, y, and X, F, which may 
be written 

7^Bx + Cy 

} (3), 

the coeflBcient of y in the first equation being identical with that 
of a? in the second equation, by the reciprocal property. The three 
constants A, J5, C are in general complex quantities, functions o(p. 

The reciprocal relation may be interpreted as follows. If 
F = 0, 5a:+(7y = 0, and 

y^B^^Ac <^> 

In like manner, if we had supposed X « 0, we should have 

BY ,., 

^'^n^ic ^""^^ 

shewing that the ratio of the current in one member to the electro- 
motive force operative in the other is independent of the way in 
which the parts are assigned to the two members. 

^ For a more complete disonBsion of this rabject see Heaviside '* On Besistanee 
and CJonductance Operators,*' PHt Mag., vol. 24, p. 479, 1887; EUctrietd Papm, 
Tol. n., p. 856. 

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235 j9.] wheatstone's bridge. 451 

We have now to determine the constants A, B^ C in terms of 
the electrical properties of the system. If y be maintained zero 
by a suitable force T, the relation between x and X is X^Ax. 
A therefore denotes the (generalized) resistance to any electro- 
motive force in the battery member, when the telephone member is 
open. This resistance is made up of /, the resistance in the 
battery member, and of that of the conductors a'\-c, b + d, 
combined in parallel. Thus 

^./+(?_+^klh-4) (6). 

In like manner 

^^ (a + m£±d) 

a + 6 + c + a ^ ^ 

To determine B let us consider the force F which must act 
in e in order that the current through it may be zero, in spite 
of the operation of X. We have T=Bx. The total current x 
flows partly along the branch (a + c), and partly along (6-l-d). 
The current through (a-^-c) is 

^Ka-^c) ^ (b-^djx 
l/(a + c) + l/(6 + d) a-^b + cVd ^ ^' 

and that through (b + d) is 

(a + c) a? 


a-l-6-i-c + d ' 

The difference of potentials at the terminals of e, supposed to 
be interrupted, is thus 

c (6 + d) X — d (a + c) J? ^ 
oTft+c+d ' 

and accordingly 5=._J|r^ (10). 

By (6), (7), (10) the relationship of Z, Yto x,y is completely 

The problem of the bridge requires the determination of the 
current y as proportional to X, when F»0, that is when no 
electro-motive force acts in the bridge itself; and the solution is 
given at once by the introduction into (4) of the values of A, JB, C 
from (6), (7), (10). 

If there be an approximate " balance," the expression simplifies. 
For (be — ad) is then small, and JS" may be neglected relatively to 


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AC in the denomiuator of (4). Thus, as a sufficient approximation 
in this case, we may write 

y,^^A (L^) (11) 

X AC (6)x(7) ^ ^' 

The following interpretation of the process leads very simply 
to the approximate form (11), and is independent of the general 
theory. Let us first inquire what electro-motive force is necessary 
in the telephone member to stop any current through it. If such 
a force act, the conditions are, externally, the same as if the 
member were open ; and the current x in the battery member due 
to a force equal to X in that member is X/A, where A is written 
for brevity as representing the right-hand member of (6). The 
difference of potentials at the terminsds of e, still supposed to be 
open, is found at once when ic is known. It is given by 

cx(8)-dx(9) = fiar, 

where B is defined by (10), In terms of X the difference of 
potentials is thus BXjA. If e be now closed, the same fraction 
expresses the force necessary in « in order to prevent the genera- 
tion of a current in that member. 

The case with which we have to deal is when X acts in /and 
there ia no force in e. We are at liberty, however, to suppose that 
two opposite forces, each of magnitude BX/A, act in e. One of 
these, as we have seen, acting in conjunction with X in/, gives no 
current in c ; so that, since electro-motive forces act independently 
of one another, the actual current in 6, closed without internal 
electro-motive force, is simply that due to the other component. 
The question is thus reduced to the determination of the current 
in e due to a given force in that member. 

So far the argument is rigorous ; but we will now suppose that 
we have to deal with an approximate balance. In this case a force 
in e gives rise to very little current in / and in calculating the 
current in e, we may suppose /to be broken. The total resistance 
to the force in e is then given simply by C of equation (7), and the 
approximate value for y is derived by dividing — BX/A by C, as 
we found in (11). 

A continued application of the foregoing process gives y/X in 
the form of an infinite geometric series : — 

., . 5» , B' ) _ B 

[ "^ AC^ A'C''^ '"I " B'-AC' 

X Acy 

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This is the rigorous solution already found in (4) ; but the first 
term of the series suffices for practical purposes. 

The form of (11) enables us at once to compare the effects of 
increments of resistance and of inductance in disturbing a balance. 
For let ad = be, and then change d to d + d', where d' = d/ + idj'. 
The value of y/X is proportional to d\ and the amplitude of the 
vibratory current in the bridge is proportional to mod. d\ that is, 
bo V(di'* + dj'*). Thus di', d,' are equally efficacious when nu- 
merically equaP. In most cases where a telephone is employed, 
the balance is more sensitive to changes of inductance than to 
changes of resistance. 

In the use of the Wheatstone balance for purposes of measure- 
ment, it is best to make a equal to c. The equality of b and d can 
then be tested by interchange of a and c, independently of the 
exactitude of the equality of these quantities. Another advantage 
lies in the fact that balance is independent of mutual induction 
between a and c or between b and d. 

236 q. In the formulae of § 235 p it has been assumed that 
there is no mutual induction between the various members of the 
combination. The more general theory has been considered very 
fully by Heaviside*, but to enter upon it would lead us too far. 
It may be well, however, to sketch the theory of the arrangement 
adopted by Hughes, which possesses certain advantages in dealing 
with the electrical properties of wires in short lengths'. 

The apparatus consists of a Wheatstone's quadrilateral, Fig. 53 b, 
with a telephone in the bridge, one of the 
sides of the quadrilateral being the wire 
or coil under examination (P), and the 
other three being the parts into which a 
single German-silver wire is divided by 
two sliding contacts. If the battery- 
branch (B) be closed, and a suitable in- 
terrupter be introduced into the telephone- 
branch (T), balance may be obtained by 
shifting the contacts. Provided that the 
interrupter introduces no electro-motive 

^ "On the Bridge Method in its Application to Periodic Electric Currents.'* 
Proc. Roy, Soc, vol. 49, p. 203, 1891. 

2 '^On the Self-induction of Wires," Part VI.; Phil. Mag,, Feb. 1887; Electrical 
Papers, 1892, vol. n., p. 281. 

» Jotirn, Tel. Eng., vol. xv. (1886) p. 1 ; Proc. Roy. Soc., vol. xl. (1886) p. 451. 

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force of its own\ the balance indicates the proportionality of 
the four resistances. If P be the unknown resistance of the 
conductor under test, Q, R the resistances of the adjacent parts of 
the divided wire, 8 that of the opposite part (between the sliding 
contacts), then, by the ordinary rule, PS^QR; while Q, iZ, S are 
subject to the relation 

Q + i2 + S=Tr, 

W being a constant. If now the interrupter be transferred from 
the telephone to the battery-branch, the balance is usually dis- 
turbed on account of induction, and cannot be restored by any 
mere shifting of the contacts. In order to compensate the 
induction, another influence of the same kind must be intro- 
duced. It is here that the peculiarity of the apparatus lies. A 
coil (not shewn in the figure) is inserted in the batter}^ and another 
in the telephone-branch which act inductively ujx)n one another, 
and are so mounted that the effect may be readily varied. The 
two coils may be concentric and relatively movable about the 
common diameter. In this case the action vanishes when the 
planes are perpendicular. If one coil be very much smaller than 
the other, the coefficient of mutual induction M is proportional to 
the cosine of the angle between the planes. By means of the 
two adjustments, the sliding of the contacts and the rotation of the 
coil, it is usually possible to obtain a fair silence. 

Hughes interpreted his observations on the basis of an as- 
sumption that the inductance of P was represented by M, irre- 
spective of resistance, and that the resistance to variable currents 
could (as in the case of steady currents) be equated to QRjS. 
But the matter is not quite so simple. The true formulae are, 
however, readily obtained for the case where the only sensible 
induction among the sides of the quadrilateral is the inductance L 
of the conductor P. 

Since there is no current through the bridge, there must be 
the same current (x) in P and in one of the adjacent sides (say) iZ, 
and for a like reason the same current y in Q and 8, The differ- 
ence of potentials at time t between the junction of P and R and 
the junction of Q and 8 may be expressed by each of the three 
following equated quantities : — 

' A condition not always satisfied in practice. 

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2355.] hughes' arrangement. 455 

Introducing the assumption that all the quantities vary har- 
monically with frequency j?/27r, and eliminating the ratio y : a?, we 
find Bs the conditions required for silence in the telephone 

QR^SP^p^ML (1), 

3f(P + Q + ii + S) = Si (2). 

It will be seen that the ordinary resistance balance (SP = QR) 
is departed from. The change here considered is peculiar to the 
apparatus and, so far as its influence is concerned, it does not 
indicate a real alteration of resistance in the wire. Moreover, 
since p is involved, the disturbance depends upon the rapidity of 
vibration, so that in the case of ordinary mixed sounds silence can 
be attained only approximately. Again, from the second equation 
we see that M is not in general a correct measure of the value 

If, however, P be known, the application of (2) presents no 
diflBculty. In many cases we may be sure beforehand that P, 
viz, the effective resistance of the conductor, or combination of 
conductors, to the variable currents, is the same as if the currents 
were steady, and then P may be regarded as known. But there 
are other cases, — some of them will be alluded to below — ^in 
which this assumption cannot be made; and it is impossible to 
determine the unknown quantities L and P from (2) alone. We 
may then fall back upon (1). By means of the two equations 
P and L can always be found in terms of the other quantities. 
But among these is included the frequency of vibration ; so that 
the method is practically applicable only when the interrupter is 
such as to give an absolute periodicity. A scraping contact, 
otherwise very convenient, is thus excluded; and this is un- 
doubtedly an objection to the method. 

If the member P be without inductance, but be interrupted by 
a leyden of capacity (7, the same formulae may be employed, with 
substitution of — 1/p^C for i. Equation (1) then gives a measure 
of C which is independent of the frequency. 

236 r. The success of experiments with this kind of apparatus 
depends very largely upon the action of the interrupter by which 
the currents are rendered variable. When periodicity is not 

1 " Diflousdion on Prof. Hughes' Address." Joum. Tel. Eng., vol. xv., p. 64, 

Feb., lase. 

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necessary, a scraping contact, actuated by a clock or by a small 
motor, answers very well; but it is advisable, following Lodge 
and Hughes, so to arrange matters that the current is suspended 
altogether at short intervals. The faint scraping sound, heard in 
the neighbourhood of a balance, is more certainly identified when 
thus rendered intermittent. 

But for many of the most interesting experiments a scraping 
contact is unsuitable. When the inductance and resistance under 
observation are rapidly varying functions of the frequency, it is 
evident that no sharp results are possible without an interrupter 
giving a perfectly regular electrical vibration. With proper appli- 
ances an absolute silence, or at least one disturbed only by a slight 
sensation of the octave of the principal tone, can be arrived at 
under circumstances where a scraping contact would admit of no 
approach to a balance at all. 

Tuning-forks, driven electromagnetically with liquid or solid 
contacts (§ 64), answer well so long as the frequency required 
does not exceed (say) 300 per second ; but for experiments with the 
telephone we desire frequencies of from 500 to 2000 per second. 
Qood results may be obtained with harmonium reed interrupters, 
the vibrating tongue making contact once during each period 
with a stop, which can be adjusted exactly to the required position 
by means of a screw'. 

But perhaps the best interrupter for use with the telephone is 
obtained by taking advantage of the instability of a jet of fluid. 
If the diameter and the speed be chosen suitably, the jet may be 
caused to resolve itself into drops under the action of a tuning- 
fork in a perfectly regular manner, one drop corresponding to 
each complete vibration of the fork. Each drop, as it passes, 
may be made to complete an electric circuit by squeezing itself 
between the extremities of two fine platinum wires. If the 
electro-motive force of the battery be pretty high, and if the 
jet be salted to improve its conductivity, sufficient current passes, 
especially if the aid of a small step-down transformer be invoked. 
Finally the apparatus is made self-acting by bringing the fork 
under the influence of an electro-magnet, itself traversed by the 
same intermittent current. Such an apparatus may be made to 
work with frequencies up to 2000 per second, and it possesses 
many advantages, among which may be mentioned almost absolute 

i PhiL Mag., vol. 22, p. 472, 18S6. 

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235 r.] INTERRUPTEBS. 457 

constancy of pitch, and the avoidance of loud aerial disturbance. 
The principles upon which the action of this interrupter depends 
will be further considered in a subsequent chapter. 

2S6 8, Scarcely less important than the interrupter are the 
arrangements for measuring induction, whether mutual induc- 
tion, as required in § 235 q, or self-induction. Inductometers, as 
Heaviside calls them, may be conveniently constructed upon 
the pattern of Hughes. A small coil is mounted so that one 
diameter coincides with a diameter of a larger coil, and is 
movable about that diameter. The mutual induction M between 
the two circuits depends upon the position given to the smaller 
coil, which is read by a pointer attached to it, and moving over a 
graduated circle. If the smaller coil were supposed to be infinitely 
small, the value of M, as has already been stated, would be pro- 
portional to the sine of the displacement from the zero position 
(Jf = 0). But an approximation to this state of things is not 
desirable. If the mean radius of the small coil be increased until 
it amounts to '55 of that of the larger, not only is the efficiency 
much enhanced, but the scale of M is brought to approximate 
coincidence, over almost the whole practical range, with the scale 
of degrees*. The absolute value of each degree may be arrived at 
in various ways, perhaps most simply by adjusting the mutual 
induction of the instrument to balance a standard of mutu^^l 

For experiments upon the plan of § 235 q the one coil is 
included in the telephone and the other in the battery branch, 
but when the object is to secure a variable and meiwurable 
inductance, the two coils are connected in series. The inductance 
of the combination is then L + iM-^N, of which the first and 
third terms are independent of the relative position of the coils. 

236 t Good results by the method of § 235 q have been 
obtained by Weber", and by the author* using a reed interrupter 
of frequency 1050 per second ; but the fact that inductance and 
resistance are mixed up in the measurements is a decided draw- 
back, if it be only because the readings require for their interpre- 
tation calculations not readily made upon the spot. 

1 Phil Mag,, vol. 22, p. 498, 1886. 

a EUctHeal Review, April 9, July 9, 1886. 

' Phil. Mag., loc, cit. 

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G oogl e 


The more obvious arrangement is one in which both the 
induction and the resistance of the branch cont^ning the subject 
under examination are in every case brought up to the given 
totals necessary for a balance. To carry this out conveniently we 
require to be able to add inductance without altering resistance, 
and resistance without altering inductance, and both in a measur- 
able degree. The first demand is easily met. If we include in 
the circuit the two coils of an inductometer, connected in series, 
the inductance of the whole can be varied in a known manner by 
rotating the smaller coil. On the other hand the introduction, or 
removal, of resistance without alteration of inductance cannot well 
be carried out with rigour. But in most cases the object can be 
sufficiently attained with the aid of a resistance-slide of thin 
German-silver wire which may be in the form of a nearly close 

In the Wheatstone's quadrilateral, as arranged for these ex- 
periments, the adjacent sides R, 8 may be made of similar wires 
of German silver of equal resistance {\ ohm). If doubled they 
give rise to little induction, but the accuracy of the method is 
independent of this circumstance. The side P includes the 
conductor, or combination of conductors, under examination, an 
inductometer, and the resistance-slide. The other side, Q, must 
possess resistance and inductance greater than any of the con- 
ductors to be compared, but need not be susceptible of ready and 
measurable variations. In order to avoid mutual induction be- 
tween the branches, P and Q should be placed at some distance 
away, being connected with the rest of the apparatus by leads of 
doubled wire. 

It will be evident that when the interrupter acts in the 
battery branch, balance can be obtained at the telephone in the 
bridge only under the conditions that both the inductance and 
the resistance in P are equal in the aggi'egate to the correspond- 
ing quantities in Q. Hence when one conductor is substituted for 
another in P, the alterations demanded at the inductometer and 
in the slide give respectively the changes of inductance and of 
resistance. In this arrangement inductance and resistance are 
well separated, so that the results can be interpreted without 
calculation; but the movable contacts of the slide appear to 
introduce uncertainty into the determination of resistaoice. 

In order to get rid of the objectionable movable contacts 
some sacrifice of theoretical simplicity seems unavoidable. We 

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can no longer keep the total resistances P and Q constant ; but by 
reverting to the arrangement adopted in a well-known form of 
Wheatstone's bridge, we cause the resistances taken from P to be 
added to Q, and vice versd. The transferable resistance is that of 
a straight wire of German-silver, with which one telephone ter- 
minal makes contact at a point whose position is read off on a 
divided scale. Any uncertainty in the resistance of this contact 
does not influence the measurements. 

Fig. 53 c. 


= @ ^ ,.^ :^^=^o>= 

The diagram Fig. (53 c) shows the connection of the parts. One 
of the telephone terminals T goes to the junction of the (^ ohm) 
resistances R and S, the other to a point upon the divided wire. 
The branch P includes one inductometer (with coils connected in 
series), the subject of examination, and part of the divided wire. 
The branch Q includes a second inductometer (replaceable by a 
simple coil possessing suitable inductance), a rheostat, or any 
resistance roughly adjustable from time to time, and the re- 
mainder of the divided wire. The battery branch B, in which may 
also be included the interrupter, has its terminals connected, one 
to the junction of P and B, the other to the junction of Q and 8. 
When it is desired to use steady currents, the telephone can of 
course be replaced by a galvanometer. 

In this arrangement, as in the other, balance requires that the 
branches P and Q be similar in respect both of inductance and of 
resistance. The changes in inductance due to a shift in the 
movable contact may usually be disregarded, and thus any alte- 
ration in the subject (included in P) is measured by the rotation 
necessitated at the inductometer. As for the resistance, it is 
evident that (R and 8 being equal) the value for any additional 
conductor interposed in P is measured by twice the displacement 
of the sliding contact necessary to regain the balance. 

Experimental details of the application of this method to the 

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measurement of variouB combinations will be found in the paper* 
from which the above sketch is derived. Among these may be 
mentioned the verification of Maxwell's formulae, (8), (9) § 235 k, 
as to the influence of a neighbouring circuit, especially in the 
extreme case where the equivalent inductance is almost destroyed, 
and of the formula (10) § 235 vi relating to the behaviour of an 
electro-magnet shunted by a relatively high simple resistance. 
But the most interesting in many respects is the application to 
the phenomena presently to be considered, where the conductors 
in question are no longer approximately linear but must be 
regarded as solid masses in which the currents are distributed in 
a manner that needs to be determined by general electrical 

As has already been remarked more than once, a leyden may 
always be supposed to be included in the circuit, the stiffness 
thereof having the effect of a negative inductance. If there be no 
hysteresis in the action of the leyden, the whole effect is thus 
represented ; but when the dielectric employed is solid, it appears 
that dissipative loss cannot be avoided. The latter effect manifests 
itself as an augmentation of apparent resistance, indistinguishable, 
unless the frequency be varied, from the ordinary resistance of the 
leads. A similar treatment may be applied to an electrolytic cell, 
the stiffness and resistance being presumably both functions of the 

236 u. It was proved by Maxwell* that a perfectly con- 
ducting sheet, forming a closed or an infinite surface, acts as a 
magnetic screen, no magnetic actions which may take place on 
one side of the sheet producing any magnetic effect on the other 
side. " In practice we cannot use a sheet of perfect conductivity ; 
but the above described state of things may be approximated to 
in the case of periodic magnetic changes, if the time-constants of 
the sheet circuits be large in comparison with the periods of the 

"The experiment is made by connecting up into a primary 
circuit a battery, a microphone-clock, and a coil of insulated wire. 
The secondary circuit includes a parallel coil and a telephone. 
Under these circumstances the hissing sound is heard almost as 
well as if the telephone were inserted in the primary circuit 

1 Phil Mag., loc. cit, 

^ Electricity and Magneti$m, 1873, § 656. 

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itself. But if a large and stout plate of copper be interposed 
between the two coils, the sound is greatly enfeebled. By a proper 
choice of battery and of the distance between the coils, it is not 
difficult so to adjust the strength that the sound is conspicuous in 
the one case and inaudible in the other "\ 

One of the simplest applications of Maxwell's principle is to 
the case of a long cylindrical shell placed within a coaxal magnet- 
izing helix. The condition of minimum energy requires that such 
currents be developed in the shell as shall neutralize at interna) 
points the action of the coil. Thus, if the conductivity of the 
shell be sufficiently high, the interior space is screened from the 
magnetizing force of periodic currents flowing in the outer helix, 
and conducting circuits situated within the shell must be devoid 
of induced currents. An obvious deduction is that the currents 
induced in a solid conducting core will be more and more confined 
to the neighbourhood of the surface as the frequency of electrical 
vibration is increased. 

The point at which the concentration of current towards the 
surface becomes important depends upon the relative values of the 
imposed vibration-period and the principal time-constant of the 
core circuit. If p be the specific resistance of the material, ^i its 
magnetic permeability, a the radius of the cylinder, the expression 
for the induction (c) parallel to the axis, during the progress of the 
subsidence of free currents in a normal mode, is 

c^^U.ikr) (1). 

where k^^^^^'^J'- (2). 


and ka is determined by the condition that 

/o(Ara) = (3). 

The roots of (3) are, § 206, 

2-404, 5-520, 8-654, 11-792, &c., 

so that for the principal mode of greatest persistence 

c = e^* Jo (2-404 r/a) (4), 

, _ (2-404)V .^^ 

where ^ = - :i \ W- 

Aooastical Observations, PhiL Mag., toI. 13, p. 344, 16S2. 

Digitized by y^:iOOQ\^^ 


For copper in c.G.S. measure p = 1642, fi^l, and thus 

T = (-X)->.g^nearly\ 

In the case of iron we may take as approximate values, /i = 100, 
p = 10*. Thus for an iron wire of diameter (2a) equal to '33 cnt, 
the value of r is about -^^ of a second, and is therefore comparable 
with the periods concerned in telephonic experiments. 

Regarded from an analytical point of view the theory of forced 
vibrations in a conducting core is equally simple, and was worked 
out almost simultaneously by Lamb', Oberbeck' and Heaviside^ 
In this case we are to regard \ as given, equal (say) to ip, where 
pjiir is the frequency. If le^^ be the imposed magnetizing force, 
the solution is 

"■fM)"'-^ » 

the value of k being given by (2). 

" When the period in the field is long in comparison with the 
time of decay of free currents, we have JaQcr)^!, nearly, so that 
c is approximately constant and ^ p,I throughout the section of 
the cylinder. But, in the opposite extreme, when the oscillations 
in the intensity of the field are rapid in comparison with the decay 
of free currents, the induced currents extend only to a small depth 
beneath the surface of the cylinder, the inner strata (so to speak) 
being almost completely sheltered from electromotive force by the 
outer ones. Writing A* = (1 - iyq\ where 

we have, when qr is large, 

Jo (At) = const. X , 

approximately, and thence 

This indicates that the electrical disturbance in the cylinder 

1 "On the Daration of Free Electric Currents in an Infinite Gondnetifig 
Cylinder," BriU Assoc, Report for 1SS2, p. 446. 
9 Proc, Math, Soc, vol. xv., p. 189, Jan. 18S4. 
3 Wied, Anti.t vol. zxi., p. 672, Ap. 1884. 
* Electrician, May, 1884. Electrical Papers, vol. n., p. 853. 

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consists in a series of waves propagated inwards with rapidly 
diminishing amplitude\" 

For experimental purposes what we most require to know is 
the reaction of the core currents upon the helix, in which alone 
we can directly measure electrical eflTects. This problem is fully 
treated by Heaviside*, but we must confine ourselves here to a 
mere statement of results. These are most conveniently expressed 
by the changes of effective inductance L and resistance R due to 
the core. If m be the number of turns per unit length in the 
magnetizing helix, and if SL, BR be the apparent alterations of L 
and R due to the introduction of the core, also reckoned per unit 
length, we have 

Si = 4»i»7r«a«(/iP-l)) ,.. 

Si2:=47;i»7r2aV.pQ j ^ ^' 

where P and Q are defined by 

P-iQ^<l>'l<l> (8), 

the function <f> being of the form 

<^(a:) = J'o(2tV^) = l+a?+-^i-...+ ^^^f^ ^, + (9), 

and the argument x being 

ipfx.ira^lp (10). 

If the material composing the core be non-conducting, a; » 0, and 

P = l, (2 = 0. 

Accordingly SZ:=4mVa»(/i- 1), Si2 = (11). 

These values apply also, whatever be the conductivity of the 
core, if the firequency be suflBciently low. 

At the other extreme, when ^ s= oo , we require the ultimate 
form of <^7<^. From the value of J© given in (10) § 200, or other- 
wise, it may be shewn that in the limit 

f/*«^-* (12), 

80 that P«Q« ^ (13). 

The introduction of these values into (7) shews that in the 
limit, when the frequency is exceedingly high^ 

Si»-4mVa«, hR^O (14), 

^ Lamb, loc, ciu, where is also discussed the problem of the currents induced by 
the sudden cessation of a previously constant field. 
' loc. cit. 

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as might also have been inferred from the consideration that the 
induced currents are then confined to the sur£9kce of the core. 

An example of the application of these formulae to an Inter- 
mediate case and a comparison with experiment will be found in 
the paper already referred to^ 

236 V. The application of Maxwell's principle to the case of 
a wire, in which a longitudinal electric current is induced, is less 
obvious; and Heaviside' appears to have been the first to state 
distinctly that the current is to be regarded as propagated inwards 
from the exterior. The relation between the electromotive force 
E and the total current C had, however, been given many years 
earlier by Maxwell* in the form of a series. His result is equi- 
valent to 

/c-W^-'-lltS <•>• 

in which R denotes the whole resistance of the length I to 
steady currents, /i the permeability, and pjiir the frequency. The 
function ^ is that defined by (9) § 235 1^, and ^ is a constant 
dependent upon the situation of the return current*. 

The most convenient form of the results is that which we have 
already several times employed. If we writ« 

E^RC-^ipLV (2), 

in which R' and Z' are real, these quantities will represent the 
effective resistance and inductance of the wire. When the argu- 
ment in (1) is small, that is when the frequency is relatively low, 
we thus obtain 

iJ' = ii{l + ^^^'-^£^+...} (3). 

i7^=4-.^|i-A^'];?+BM.^v...} (♦)'• 

1 Phil Mag., vol. 22, p. 493, 1886. 

^ Electrician, Jan., 1885 ; Electrical Papers, vol. i., p. 440. 

» Phil, Trant., 1865 ; Electricity and Magnetism, vol. ii., § 690. 

* The simplest case arises when the dielectric, which bounds the cylindrical 
wire of radius a, is enclosed within a second conducting mass extending outwards 
to infinity and bounded internally at a cylindrical surface r=b. We then have 
il = 2 log (6/a). See J. J. Thomson, loc. cit,, § 272. 

< Phil. Mag., vol. 21, p. 387, 1886. It is singular that Maxwell {loc. eit.) seems 
to have regarded his solution as conveying a correction to the self-induction only of 
the wire. 

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235 v.] LIMITING FORMS. 465 

When p is very small, these equations give, as was to be 

R^R^ i' = Z(^+i/i) (5). 

If we include the next terms, we recognise that, in accordance 
with the general rule, L begins to diminish and -R' to increase. 

When p is very great, we have to make use of the limiting 
form of ^7^* As in § 235 u, 

4./f=(i+i)V(ii)WJJ) (6); 

and thus ultimately 

R^^dplfiR) (7), 

L'll^A^s/{,jLRmi) (8), 

the first of which increases without limit with p, while the second 
tends to the finite limit A, corresponding to the total exclusion of 
current from the interior of the wire. 

Experiments^ upon an iron wire about 18 metres long and 3*3 
millimetres in diameter led to the conclusion that the resistance 
to variable currents of frequency 1050 was such that RjR = 1*9. 
A calculation based upon (1) shewed that this result is in harmony 
with theory, if ft = 99 '5. Such is about the value indicated by 
other telephonic experiments. 

2216 w. The theory of electric currents in such wires as are 
commonly employed in laboratory experiments is simple, mainly in 
consequence of the subordination of electrostatic capacity. When 
this element can be neglected, the current is necessarily the same 
at all points along the length of the wire, so that whatever enters 
a wire at the sending end leaves it unimpaired at the receiving 
end. In this case the whole electrical character of the wire can 
be expressed by two quantities, its resistance -R and inductance Z, 
and these may usually be treated as constants, independent of the 
frequency. The relation of the current to the electromotive force 
under such circumstances has already been discussed (7) § 235 j. 
When we have occasion to consider only the amplitude of the 
current, irrespective of phase, we may regard it as determined 
by ^/\R'\'P^L% a quantity which is called by Heaviside the 
impedance. Thus in circuits devoid of capacity the impedance is 
always increased by the existence of L, 

1 PhiL Mag,, vol. 22, p. 488, 1886. 

R. 30 

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Circuits employed for practical telephony may often be re- 
garded as coming under the above description, especially when 
the wires are suspended and are of but moderate length. But 
there are other cases in which electrostatic capacity is the domi- 
nating feature. The theory of electric cables was established 
many years ago by Lord Kelvin^ for telegraphic purposes. If S 
be the capacity and R the resistance of the cable, reckoned per 
unit length, V and C the potential and the current at the point z, 
we have 

SdV/dt^-dC/dz, RC^-dVjdz (1). 

whence RSdCjdt^d^Gldz^ (2), 

the well known equation for the conduction of heat discussed by 
Fourier. On the assumption that C is proportional to c***, it 
reduces to 

d»(7/ck«={V(ii>iiS).(l-fi)}»a (3); 

so that the solution for waves propagated in the positive direc- 
tion is 

(7=Ooe-^<*^^J-'cos{pe-V(ii>i2fif).-^} (4). 

The distance in traversing which the current is attenuated in the 
ratio of to 1 is thus 

z = ^(2lpRS) (5). 

A very slight consideration of the magnitudes involved is 
sufficient to give an idea of the difficulty of telephoning through a 
long cable. If, for example, the frequency (p/Zir) be that of a 
note rather more than an octave above middle c, and the cable be 
such as are used to cross the Atlantic, we have in c.G.S. measure 

Vi> = 60, (RSy^ ^2 xlO'\ 

and .accordingly from (5) 

^ = 3 X 10* cm. = 20 miles approximately. 

A distance of 20 miles would thus reduce the intensity of 
sound, measured by the square of the amplitude, to about a 
tenth, an operation which could not be repeated often without 
rendering it inaudible. With such a cable the practical limit 
would not be likely to exceed fifty miles, more especially as 
the easy intelligibility of speech requires the presence of tones 
still higher than is supposed in the above numerical example'. 

^ Proc, Roy, Soc.y 1855 ; Mathematical and Physical Papers^ vol. n. p. 61. 
3 •( On Telephoning through a Cable." Brit, Ass. Report for 1884, p. 682. 

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235 X.] heaviside's theory. 467 

236 X, In the above theory the insulation is supposed to be 
perfect and the inductance to be negligible. It is probable that 
these conditions are sufficiently satisfied in the case of a cable, 
but in other telephonic lines the inductance is a feature of great 
importance. The problem has been treated with full generality 
by Heaviside, but a slight sketch of his investigation is all that 
our limits permit. 

If jB, S, Z, J2* be the resistance, capacity or permittance, in- 
ductance, and leakage- conductance respectively per unit of length, 
V and C the potential-difference and current at distance z, the 
equations, analogous to (I) § 235 w, are 

^r..i-=-f, .c.zf.-|E (,, 

Thus, if the currents are harmonic, proportional to e^^*, 

^^^{R + ipL){K+ipS)C. (2). 

with a similar equation for F. 

It might perhaps have been expected that a finite leakage K 
would always act as a complication; but Heaviside^ has shewn 
that it may be so adjusted as to simplify the matter. This case, 
which is remarkable in itself and also serves to throw light upon 
the general question, arises when RjL = KjS. We will write 

XSt;«=l, RIL^KjS^q (2), 

where t; is a velocity of the order of the velocity of light. The 
equation for V is then by (1) 

i;»d«F/d^ = (d/dt-f?yF (3); 

or if we take U so that 

V^&-^U (4), 

v^d^Uldz^^d^UldV' (5), 

the well-known equation of undisturbed wave propagation § 144. 
"Thus, if the wave be positive, or travel in the direction of 
increasing z, we shall have, if /i {z) be the state of F initially, 

Fx = e-Vx(^-vO. ^^1= y^lLv (6). 

If Fa, Oj be a negative wave, travelling the other way, 

y^-^e'^Mz^vt\ C^^VJLv (7). 

^ Electrician, June 17, 1887. Electrical Papers, vol ii. pp. 125, 809. 

30—2 — 

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Thus, any initial state being the sum of V^ and F, to make F, 
and of Ci and (7, to make C, the decomposition of an arbitrarily 
given initial state of V and C into the waves is effected by 

F, = i(F+t;iO), V,^\{V^vLC) (8). 

We have now merely to move V^ bodily to the right at speed 
V, and F, bodily to the left at speed v, and attenuate them to the 
extent e~^, to obtain the state at time t later, provided no changes 
of condition have occurred. The solution is therefore true for all 
future time in an infinitely long circuit. But when the end of a 
cii*cuit is reached, a reflected wave usually results, which must be 
added on to obtain the real result." 

As in § 144, the precise character of the reflection depends 
upon the terminal conditions. ''One case is uniquely simple. 
Let there be a resistance inserted of amount vL, It introduces 
the condition F = vLG if at say B, the positive end of the circuit, 
and F:=— vZC if at the negative end, or beginning. These are 
the characteristics of a positive and of a negative wave respect- 
ively ; it follows that any disturbance arriving at the resistance is 
at once absorbed. Thus, if the circuit be given in any state 
whatever, without impressed force, it is wholly cleared of electrifi- 
cation and current in the time Ijv at the most, if I be the length 
of the circuit, by the complete absorption of the two waves into 
which the initial state may be decomposed." 

" But let the resistance be of amount -Bi at say B ; and let Fj 
and Fj be corresponding elements in the incident and reflected 
waves. Since we have 

V.^vLC,, V, — vLC^, F,-f F, = iJ,(C', + C,)...(9), 

we have the reflected wave given by 

V, R,^vL 

V, R,^vL' 


If Ri be greater than the critical resistance of complete ab- 
sorption, the current is negatived by reflection, whilst the electri- 
fication does not change sign. If it be less, the electrification is 
negatived, whilst the current does not reverse." 

"Two cases are specially notable. They are those in which 
there is no absorption of energy. If iJi = 0, meaning a short 
circuit, the reflected wave of F is a perverted and inverted copy of 

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235 a:.] heaviside's theory. 469 

the incident. But if ii = oo , representing insulation, it is G that 
is inverted and perverted \" 

The cases last mentioned are evidently analogous to the reflec- 
tion of a sonorous aerial wave travelling in a pipe. If the end of 
the pipe be closed, the reflection is of one character, and if it be 
open of another character. In both cases the whole energy is 
reflected, § 257. The waves reflected at the two ends of an electric 
circuit complicate the general solution, especially when the sim- 
plifying condition (2) does not hold. But in many cases of 
practical interest they may be omitted without much loss of 
accuracy. One passage over a long line usually introduces con- 
siderable attenuation, and then the effect of the reflected wave, 
which must traverse the line three times in all, becomes insigni- 

In proceeding to the general solution of (2) for a positive 
wave, we will introduce, after Heaviside, the following abbrevia- 

»'iS=l, RILp=f, KjSp^g (11). 

In terms of these quantities (2) may be written 

d^C/dz'^(P + iQyC (12), 


^ or (? = i {p/vY {(1 +/»)* (1 + 5^0* i (f9 - 1)1 . . . (13). 

Thus, if P and Q be taken positively, the solution for a wave 
travelling in the positive direction is 

(7= Coe'^'cos{pt - Qz) (14), 

the current at the origin being Cq cos pt 

The cable formula, § 235 w, is the particular case arrived at by 
supposing in (13)/= go , ^r = 0, which then reduces to 

i>a = (2» = jpiJ£f (15). 

Again, the special case of equation (3) is derivable by putting 
f=g — qjP' The result is 

P = ?/v, Q^pIv (16). 

If the insulation be perfect, ^ = 0, and (13) becomes 

P« or (?-i(;,/t;)»{(l +/«)»?!} (17). 

^ Heaviside, Collected Worki^ vol. n. p. 312. 

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In certain examples of long copper lines of high conductivity, 
/ may be regarded as small so far as telephonic frequencies are 
concerned. Equation (17) then gives 

P=pfl2v^R/2vL, Q=pIv (18). 

For a further discussion of the various cases that may arise 
the reader must be referred to the writings of Heaviside already 
cited. The object is to secure, as far as may be, the propagation 
of waves without alteration of type. And here it is desirable to 
distinguish between simple attenuation and distortion. If, as in 
(16) and (18), P is independent of p, the amplitudes of all com- 
ponents are reduced in the same ratio, and thus a complex wave 
travels without distortion. The cable formula (15) is an example 
of the opposite state of things, where waves of high frequency are 
attenuated out of proportion to waves of low frequency. It appears 
from Heaviside's calculations that the distortion is lessened by 
even a moderate inductance. 

The eflFectiveness of the line requires that neither the attenua- 
tion nor the distortion exceed certain limits, which however it is 
hard to lay down precisely. A considerable amount of distortion 
is consistent with the intelligibility of speech, much that is 
imperfectly rendered being supplied by the imagination of the 

236 y. It remains to consider the transmitting and receiving 
appliances. In the early days of telephony, as rendered practical 
by Graham Bell, similar instruments were employed for both 
purposes. Bell's telephone consists of a bar magnet, or battery 
of bar magnets, provided at one end with a short pole-piece 
which serves as the core of a coil of fine insulated wire. In close 
proximity to the outer end of the pole-piece is placed a circular 
disc of thin iron, held at the circumference. Under the influence 
of the permanent magnet the disc is magnetized radially, the 
polarity at the centre being of course opposite to that of the 
neighbouring end of the steel magnet. 

The operation of the instrument as a transmitter is readily 
traced. When sonorous waves impinge upon the disc, it responds 
with a symmetrical transverse vibration by which its distance 
from the pole-piece is alternately increased and diminished. 
When the interval is diminished, more induction passes through 
the pole-piece, and a corresponding electro-motive force acts in 

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235 yO bell's telephone. 471 

the enveloping coil. The periodic movement of the disc thus 
gives rise to a periodic current in any circuit connected with the 
telephone coil. 

The electro-motive force is in the first instance proportional 
to the permanent magnetism to which it is due; and this law 
would continue to hold, were the behaviour of the pole-piece and 
of the disc conformable to that of the " soft iron " of approximate 
theory. But as the magnetism rises, and the state of saturation 
is more nearly approached, the response to periodic changes of 
force becomes feebler, and thus the eflSciency falls below that 
indicated by the law of proportionality. If we could imagine the 
state of saturation in the pole-piece to be actually attained, the 
induction through the coil would become almost incapable of 
variation, being reduced to such as might occur were the iron 
removed. There is thus a point, dependent upon the properties 
of magnetic matter, beyond which it is pernicious to raise the 
amount of the permanent magnetism ; and this point marks the 
maximum efficiency of the transmitter. It is probable that the 
most favourable condition is not fully reached in instruments 
provided with steel magnets; but the considerations above 
advanced may serve to explain why an electro-magnet is not 

The action of the receiving instrument may be explained on 
the same principles. The periodic current in the coil alternately 
opposes and cooperates with the permanent magnet, and thus the 
iron disc is subjected to a periodic force acting at its centre. 
The vibrations are thence communicated to the air, and so reach 
the ear of the observer. As in the case of the transmitter, the 
efficiency attains a maximum when the magnetism of the pole- 
piece is still far short of saturation. 

The explanation of the receiver in terms of magnetic forces 
pulling at the disc is sometimes regarded as inadequate or even as 
altogether wide of the mark, the sound being attributed to " mole- 
cular disturbances " in the pole-piece and disc. There is indeed 
every reason to suppose that molecular movements accompany 
the change of magnetic state, but the question is how do these 
movements influence the ear. It would appear that they can do 
so only by causing a transverse motion of the surface of the disc, 
a motion from which nodal subdivisions are not excluded. 

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In support of the '' push and pull theory " it may be useful to 
cite an experiment tried upon a bipolar telephone. In this 
instrument each end of a horse-shoe magnet is provided with a 
pole-piece and coil, and the two pole-pieces are brought into 
proximity with the disc at places symmetrically situated with 
regard to the centre. In the normal use of the instrument the 
two coils are permanently connected as in an ordinary horse-shoe 
electro-magnet, but for the purposes of the experiment provision 
was made whereby one of the coils could be reversed at pleasure 
by means of a reversing key. The sensitiveness of the telephone 
in the two conditions was tested by including it in the circuit of 
a Daniell cell and a scraping contact apparatus, resistance from a 
box being added until the sound was but just easily audible. 
The resistances employed were such as to dominate the self- 
induction of the circuit, and the comparison shewed that the 
reversal of the coil from its normal connection lowered the sensi- 
tiveness to current in the ratio of 11 : 1. That the reduction was 
not still greater is readily explained by outstanding failures of 
symmetry; but on the "molecular disturbance" theory it is not 
evident why there should be any reduction at all. 

Dissatisfaction with the ordinary theory of the action of a 
receiving telephone may have arisen from the difficulty of under- 
standing how such very minute motions of the plate could be 
audible. This is, however, a question of the sensitiveness of the 
eai*, which has been proved capable of appreciating an amplitude 
of less than 8 x lO^^cra.^ The subject of the audible minimum 
will be further considered in the second volume of this work. 

The calculation a priori of the minimum current that should 
be audible in the telephone is a matter of considerable difficulty ; 
and even the determination by direct experiment has led to 
widely discrepant numbers. In some recent experiments by the 
author a unipolar Bell telephone of 70 ohms resistance was 
employed. The circuit included also a resistance box and an 
induction coil of known construction, in which acted an electro- 
motive force capable of calculation. Up to a frequency of 307 
this could be obtained from a revolving magnet of known moment 
and situated at a measured distance from the induction coil. For 
the higher frequencies magnetized tuning-forks, vibrating with 
measured amplitudes, were substituted. In either case the 

1 Proc, Roy, Soc. vol. xxvi. p. 248, 1877. 

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235 y.] 



resistance of the circuit was increased until the residual sound 
was but just easily audible. Care having been taken so to 
arrange matters that the self-induction of the circuit was negli- 
gible, the current could then be deduced from the resistance and 
the calculated electro-motive force operating in the induction 
coil. The following are the results, in which it is to be under- 
stood that the currents recorded might have been halved without 
the sounds being altogether lost : 



Current in 
10-« amperes 


Revolving Magnet 

Revolving Magnet 




The effect of a given current depends, of course, upon the 
manner in which the telephone is wound. If the same space be 
occupied by the copper in the various cases, the current capable of 
producing a particular effect is inversely as the square root of the 

The numbers in the above table giving the results of the 
author's experiments are of the same order of magnitude as 
those found by Ferraris^ whose observations, however, related 
to sounds that were not pure tones. But much lower estimates 
have been put forward. Thus Tait' gives 2 x 10"" amperes, 
and Preece a still lower figure, 6 x 10""". These discrepancies, 
enormous as they stand, would be still further increased were 
the comparison made to refer to the amounts of energy absorbed. 

According to the calculations of the author the above tabulated 
sensitiveness to a periodic current of frequency 256 is about what 
might reasonably be expected on the push and pull theory* At 

1 Atti delta Aeead. d. Scu Di Torino, vol. xiii. p. 1024, 1877. 

2 Edin, Proc. vol. ix. p. 561, 1878. 

' I propose shortly to publish these calculations. 

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this frequency, which is below those proper to the telephone plate 
(§ 221 a), the motion of the plate is governed by elasticity rather 
than by inertia, and an equilibrium theory (§ 100) is applicable as 
a rough approximation. The greater sensitiveness of the telephone 
at frequencies in the neighbourhood of 512 would appear to 
depend upon resonance (§ 46). It is doubtful whether the much 
higher sensitiveness claimed by Tait and Preece could be re- 
conciled with theory. 

It appears to be established that the iron plate of a telephone 
may be replaced by one of copper, or even of non-conducting 
material, without absolute loss of sound; but these effects are 
probably of a different order of magnitude. In the case of copper 
induced currents may confer the necessary magnetic properties. 
For a description of the ingenious receiver invented by Ekiison 
and for other information upon telephonic appliances the reader 
may consult Preece and Stubbs' Manual of Telephony. 

In existing practice the transmitting instrument depends 
upon a variable contact. The first carbon transmitter was con- 
structed by Edison in 1877, but the instruments now in use are 
modifications of Hughes' microphone \ A battery current is led 
into the line through pieces of metal or of carbon in loose juxta- 
position, carbon being almost universally employed in practice. 
Under the influence of sonorous vibration the electrical resistance 
of the contacts varies, and thus the current in the line is rendered 
representative of the sound to be reproduced at the receiving 

That the resistance of the contact should vary with the 
pressure is not surprising. If two clean convex pieces of metal 
ai*e forced together, the conductivity between them is represented 
by the diameter of the circle of contact (§306). The* relation 
between the circle of contact and the pressure with which the 
masses are forced together has been investigated in detail by 
Hertz \ His conclusion for the case of two equal spheres is that 
the cube of the radius of the circle of contact is proportional to 
the pressure and to the radii of the spheres. But it has not yet 
been shewn that the action of the microphone can be adequately 
explained upon this principle. 

^ Proc. Roy, Soc., vol. xxvii. p. 862, 1878. 
» Crelle, Jo^im. Math. xcn. p. 166, 1882. 

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From the Proceedings of the London Mathematical Society^ 
Vol. IX., p. 21, 1877. 

It has often been remarked that, when a group of waves advances 
into still water, the velocity of the group is less than that of the indi- 
vidual waves of which it is composed ; the waves appear to advance 
through the group, dying away as they approach its anterior limit. 
This phenomenon was, I believe, first explained by Stokes, who re- 
garded the group as formed by the superposition of two infinite trains 
of waves, of equal amplitudes and of nearly equal wave-lengths, ad- 
vancing in the same direction. My attention was called to the subject 
about two years since by Mr Froude, and the same explanation then 
occurred to me independently*. In my book on the "Theory of 
Sound" (§191), I have considered the question more generally, and 
have shewn that, if V be the velocity of propagation of any kind of 
waves whose wave-length is X, and k = 2ir/X., then U, the velocity of 
a group composed of a great number of waves, an3 moving into an un- 
disturbed part of the medium, is expressed by 

-=T' <». 

* Another phenomenon, ftlso mentioned to me by Mr Froude, admits of a similar 
explanation. A steam-launch moving quickly through the water is accompanied by 
a peculiar system of diverging waves, of which the most striking feature is the 
obliquity of the line containing the greatest elevations of successive waves to the 
wave-fronts. This wave pattern may be explained by the superposUion of two (or 
more) infinite trains of waves, of slightly differing wave-lengths, whose directions 
and velocities of propagation are so related in each case that there is no change of 
position relatively to the boat. The mode of composition will be best understood by 
drawing on paper two sets of parallel and equidistant lines, subject to the above 
condition, to represent the crests of the component trains. In the case of two trains 
of slightly different wave-lengths, it may be proved that the tangent of the angle 
between the line of maxima and the wave-fronts is half the tangent of the angle 
between the wave-fronts and the boat's course. 

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or, as we may also write it, 

"■■^-'^z^. <^^ 

Thus, if FocX«, Cr=(l-w) V (3). 

In fact, if the two infinite trains be represented by cos k(Vt^x) 
and cos k' ( V't — a:), their resultant is represented by 

cos A; ( F« - a;) + cos k' ( V't - x\ 
which is equal to 

(k'V'-kV ^ k'--k 1 (k'V'-^kV k' + k \ 

2cos| ^_^-_-a:| .cosj— 2— «- 2 4- 

If k' -ky V - r be small, we have a train of waves whose amplitade 
varies slowly from one point to another between the limits and 2, 
forming a series of groups separated from one another by regions com- 
paratively free from disturbance. The position at time t of the middle 
of that group, which was initially at the origin, is given by 


which shews that the velocity of the group is {k' V - kV) -r {k* — k). 
In the limit, when the number of waves in each group is indefinitely 
great) this result coincides with (1). 

The following particular cases are worth notice, and are here tabu- 
lated for convenience of comparison : — 



Reynolds' disconnected pendulums. 



Deep-water gravity waves. 



Aerial waves, Ac. 



Capillary water waves. 



Flexural waves. 

The capillary water waves are those whose wave-length is so small 
that the force of restitution due to capillarity largely exceeds that due 
to gravity. Their theory has been given by Thomson (PhiL Mag., 
Nov. 1871). The flexural waves, for which U=2V, are those cor- 
responding to the bending of an elastic rod or plate ("Theory of 
Sound," § 191). 

In a paper read at the Plymouth meeting of the British Association 
(afterwards printed in "Nature," Aug. 23, 1877), Prof. Osborne 
Reynolds gave a dynamical explanation of the fact that a group of 
deep-water waves advances with only half the rapidity of the indi- 
vidual waves. It appears that the energy propagated across any point, 
when a train of waves is passing, is only one-half of the energy neoes- 

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sary to supply the waves which pass in the same time, so that, if the 
train of waves be limited, it is impossible that its front can be propa- 
gated with the full velocity of the waves, because this would imply the 
acquisition of more energy than can in fact be supplied. Prof. Reynolds 
did not contemplate the cases where more energy is propagated than 
corresponds to the waves passing in the same time ; but his argument, 
applied conversely to the results already given, shews that such cases 
must exist. The ratio of the energy propagated to that of the passing 
waves \a U : V', thus the energy pi*opagated in the unit time \a U : V 
of that existing in a length F, or U times that existing in the unit 
length. Accordingly 

Energy propagated in unit time : Energy contained (on an average) 

in unit length =d{kV) : dk^ by (1). 

As an example, I will take the case of small ir rotational waves in 
water of finite depth ^. If z be measured downwards from the surface, 
and the elevation (/*-) of the wave be denoted by 

h = H cos {nt — kx) (4), 

in which n = kVj the corresponding velocity-potential (^) is 

* = - VH'^-^^^Bmint-hx) (5). 

This value of <^ satisfies the general differential equation for irrota- 
tional motion (v*^ = 0), makes the vertical velocity dif>/dz zero when 
« =: Z, and - dh/dt when « = 0. The velocity of propagation is given by 

^-i^ («)• 

We may now calculate the energy contained in a length x, which is 
supposed to include so great a number of waves that fractional parts 
may be left out of account. 

For the potential energy we have 

Vi^gpjj zdzdx=zyp jh^dx^lgpH^x (7). 

For the kinetic energy, 

■l''/(*ff)„*'-l'"^-' («)■ 

by (1) and (6). If, in accordance with the argument advanced at the 

* Prof. Be^rnolds considers the troohoidal wave of Bankine and Froude, which 
inyolves molecular rotation. 

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478 APPElffDIX. 

«nd of this paper, the equality of Vi and T be assumed, the value of 
the velocity of propagation follows from the present expressions. Hie 
whole energy in the waves occupying a length x is therefore (for each 

unit of breadth) V^ -^ T = \gpH^ , x (9), 

H denoting the maximum elevation. 

We have next to calculate the energy propagated in time t across a 
plane for which x is constant, or, in other words, the work ( W) that 
must be done in order to sustain the motion of the plane (considered 
as a flexible lamina) in the face of the fluid pressures acting upon the 
front of it. The variable part of the pressure (Sp\ at depth Zy is 
given by 

«p = - p -^ = - nVH — ^ETT^HM — cos (nt - kx), 
while for the horizontal velocity 

^ = ^^^ ^,g-fa ooB{nt^kx); 

so that W=jj^^(hdt = \gpHKVt.h+^i^^'j (10), 

on integration. From the value of V in (6) it may be proved that 

and it is thus verified that the value of W for a unit time 
= — W— X energy m unit length. 

As an example of the direct calculation of U, we may take the case 
of waves moving under the joint influence of gravity and cohesion. 

It is proved by Thomson that 

P = f-i-rA; (11), 

where T' is the cohesive tension. Hence 

"When k is small, the surface tension is negligible, and then U^^^V; 
but when, on the contrary, k is large, U=^V, as has already he&a. 
stated. When TJ^ — g, U=^V. This corresponds to the miniwyj^m 
velocity of propagation investigated by Thomson. 

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Although the argument from interference groups seems satisfactory, 
an independent investigation is desirable of the relation between 
energy existing and energy propagated. For some time I was at a loss 
for a method applicable to all kinds of waves, not seeing in particular 
why the comparison of energies should introduce the consideration of 
a variation of wave-length. The following investigation, in which the 
increment of wave-length is imaginary^ may perhaps be considered to 
meet the want : — 

Let us suppose that the motion of every part of the medium is 
resisted by a force of very small magnitude proportional to the mass 
and to the velocity of the part, the effect of which will be that waves 
generated at the origin gradually die away as x increases. The motion, 
which in the absence of friction would be represented by cos {nt — kx), 
under the influence of friction is represented by e"*** cos {nt — kx), 
where ^ is a small positive coefficient. In strictness the value of k is 
also altered by the friction; but the alteration is of the second order as 
regards the frictional forces, and may be omitted under the circum- 
stances here supposed. The energy of the waves per unit length at 
any stage of degradation is proportional to the square of the amplitude, 
and thus the whole energy on the positive side of the origin is to the 
energy of so much of the waves at their greatest value, i.e., at the 
origin, as would be contained in the unit of length, as j'^ e-^" dx : 1, 
or as (2/a)"^ : 1. The energy transmitted through the origin in the 
unit time is the same as the energy dissipated ; and, if the frictional 
force acting on the element of mass m be hinVy where v is the velocity 
of the element and h is constant, the energy dissipated in unit time is 
Ji^mr^ or 2hTy T being the kinetic energy. Thus, on the assumption 
that the kinetic energy is half the whole energy, we find that the 
energy transmitted in the unit time is to the greatest energy existing 
in the unit length as h : 2^. It remains to find the connection be- 
tween h and /*. 

For this purpose it will be convenient to regard cos {nt - kx) as the 
real part of e*"* 6***, and to inquire how k is affected, when n is given, 
by the introduction of friction. Now the effect of friction is repre- 
sented in the differential equations of motion by the substitution of 
(Pjd^ + hdjdt in place of d^/d^, or, since the whole motion is proportional 
to e*^, by substituting - w* + ihn for — w*. Hence the introduction of 
friction corresponds to an alteration of n from n to n — ^ih (the square 
of h being neglected) ; and accordingly k is altered from k to 
k-^ihdk/dn. The solution thus becomes e"******/^** e' <"*"**>, or, when 
the imaginary part is rejected, e-4*«<»/<*» cos {nt — kx); so that 
/A = ^ A dkjdn^ and A : 2/t = dn/dk. The ratio of the energy transmitted 

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in the unit time to the energy existing in the unit length is therefore 
expressed by dnjdk or d(kV)jdk, as was to be proved 

It has often been noticed, in particular cases of progressive waves, 
that the potential and kinetic energies are equal ; but I do not call to 
mind any general treatment of the question. The theorem is not 
usually true for the individual parts of the medium*, but must be 
understood to refer either to an integral nmnber of wave-lengths, or to 
a space so considerable that the outstanding fractional parts of waves 
may be left out of account. As an example well adapted to give in- 
sight into the question, I will take the case of a uniform stretched 
circular membrane ("Theory of Sound," § 200) vibrating with a given 
number of nodal circles and diameters. The fundamental modes are 
not quite determinate in consequence of the symmetry, for any dia- 
meter may be made nodal. In order to get rid of this indeterminate- 
ness, we may suppose the membrane to carry a small load attached to 
it anywhere except on a nodal circle. There are then two definite 
fundamental modes, in one of which the load lies on a nodal diameter, 
thus producing no effect, and in the other midway between nodal dia- 
meters, where it produces a maximum effect ("Theory of Sound," 
§ 208). If vibrations of both modes are going on simultaneously, the 
potential and kinetic energies of the whole motion may be calculated 
by simple addition of those of the components. Let us now, supposing 
the load to diminish without limit, imagine that the vibrations are of 
equal amplitude and differ in phase by a quarter of a period. The 
result is a progressive wave, whose potential and kinetic energies are 
the sums of those of the stationary waves of which it is composed. 
For the first component we have Vi = B cos' nt, Ti = E sin* rU ; and 
for the second component, V^^ E sin' n<, T^= E cos' rU ; so that 
]\ + r, = 7\ + 7*2 = ^, or the potential and kinetic energies of the 
progressive wave are equal, being the same as the whole energy of 
either of the components. The method of proof here employed appears 
to be sufficiently general, though it is rather difficult to express it in 
language which is appropriate to all kinds of waves. 

* Atrial waves are an important exoeption. 



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