XV. 2]
THE ZEEMAN EFFECT
209
2. The Quantum Theory of the Zeeman Effect
Difficulty is met with in applying the quantum theory even
in the case of the simple Zeeman effect. The problem has been
discussed by a number of workers, including Herzfeld,* * * § Bohr, f
and later Debye | and Sommerfeld.§ Considerable progress has
been made in the solution of the problem by the last two on
this list. The difficulty of accounting for any effect at all had
been emphasized by Mosharrafa,i| and more recently by Hicks,
the former having shown how the extended form of the quantum
restrictions put forward by W. Wilson leads to the simple Zeeman
effect. Wilson himself has also discussed this problem.
We shall, however, consider only the simple deduction of the
Zeeman separation due to Sommerfeld. According to Bohr’s
second postulate radiation is emitted only in the transition be
tween two stationary states, the frequency v of the emitted
spectral line being determined by the relation hv = H a — H e ,
where H a and H e are the initial and final energies of the system.
The effect of the magnetic field is to produce a change in the
energy in the initial state of amount AH a , and in the final state
of amount AH e .
Consequently there is a change in the frequency of the radia
tion emitted determined by the equation
hAv =AH a — AH e ... .15:4
It is necessary then to determine the change in the energy
of a stationary state due to some applied magnetic field of
strength H. Sommerfeld supposes that orientation in space
occurs as described in a previous chapter, but finds that there
is no change in the form of the orbit, the change in energy being
equal simply to the change in the kinetic energy, and the amount
h
of this change AH is equal to m—o where o is the angular velo-
QTC
city corresponding to the Larmor precession. When we sub
stitute the value for o we obtain
AH = nth— —
m 0 47TC
15:5
In this expression m is the equatorial or magnetic quantum num
ber which determines the resolved angular momentum about the
* Herzfeld, Phys. Zeits., vol. 15, p. 193, 1914.
t Bohr, Phil. Mag., vol. 27, p. 506, 1914.
I Debye, Phys. Zeits., vol. 17, p. 507, 1916.
§ Sommerfeld, Phys. Zeits., vol. 17, p. 491, 1916.
II Mosharrafa, Proc. Roy. Soc. A, vol. 102, p. 529, 1923.
TJ Hicks, Nature, vol. 115, p. 978, 1925.