|
|||
ON THE SPECTRUM OF HYDROGEN
|
11
|
||
|
|||
these systems. No one has ever seen a Planck's resonator, nor
indeed even measured its frequency of oscillation; we can observe only the period of oscillation of the radiation which is emitted. It is therefore very convenient that it is possible to show that to obtain the laws of temperature radiation it is not necessary to make any assumptions about the systems which emit the radiation except that the amount of energy emitted each time shall be equal to Kv, where h is Planck's constant and v is the frequency of the radiation. Indeed, it is possible to derive Planck's law of radiation from this assumption alone, as shown by Debye, who employed a method which is a combination of that of Planck and of Jeans. Before considering any further the nature of the oscillating systems let us see whether it is possible to bring this assumption about the emission of radiation into agreement with the spectral laws.
If the spectrum of some element contains a spectral line corre-
sponding to the frequency v it will be assumed that one of the atoms of the element (or some other elementary system) can emit an amount of energy hv. Denoting the energy of the atom before and after the emission of the radiation by El and E% we have |
|||
|
|||
t-* or » = -
fi |
.(5)
|
||
|
|||
During the emission of the radiation the system may be regarded
as passing from one state to another; in order to introduce a name for these states, we shall call them "stationary" states, simply indicating thereby that they form some kind of waiting places between which occurs the emission of the energy corresponding to the various spectral lines. As previously mentioned the spectrum of an element consists of a series of lines whose wave lengths may be expressed by the formula (2). By comparing this expression
Si
with the relation given above it is seen that—since v = -, where o
A,
is the velocity of light—each of the spectral lines may be regarded
as being emitted by the transition of a system between two stationary states in which the energy apart from an additive arbitrary constant is given by —chFr(n^) and —chFs(n2) respectively. Using this interpretation the combination principle asserts that a series of stationary states exists for the given system, and that it can |
|||
|
|||