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6.5 Spectra 191
does not give results that correspond to actual observations. For this reason, we
refer to this treatment as the pseudo-Zeeman effect.
When a magnetic ®eld B is applied to a hydrogen-like atom with magnetic
moment M, the resulting potential energy V is given by the classical expression
: ì B :
V ÿM B L B (6:86)
"
where equation (5.81) has been introduced. If the z-axis is selected to be
parallel to the vector B, then we have
V ì B BL z =" (6:87)
If we replace the z-component of the classical angular momentum in equation
^
(6.87) by its quantum-mechanical operator, then the Hamiltonian operator H B
for the hydrogen-like atom in a magnetic ®eld B becomes
ì B B
^ ^ ^
H B H L z (6:88)
"
^
where H is the Hamiltonian operator (6.14) for the atom in the absence of the
magnetic ®eld. Since the atomic orbitals ø nlm in equation (6.56) are simultan-
^
^
^ 2
eous eigenfunctions of H, L , and L z , they are also eigenfunctions of the
^
operator H B . Accordingly, we have
^ ^ ì B B ^
H B ø nlm H L z ø nlm (E n mì B B)ø nlm (6:89)
"
where E n is given by (6.48) and equation (6.15c) has been used. Thus, the
energy levels of a hydrogen-like atom in an external magnetic ®eld depend on
the quantum numbers n and m and are given by
2
Z e9 2
E nm ÿ mì B B, n 1, 2, ... ; m 0, 1, ... , (n ÿ 1)
2a ì n 2
(6:90)
This dependence on m is the reason why m is called the magnetic quantum
number.
The degenerate energy levels for the hydrogen atom in the absence of an
external magnetic ®eld are split by the magnetic ®eld into a series of closely
spaced levels, some of which are non-degenerate while others are still
degenerate. For example, the energy level E 3 for n 3 is nine-fold degenerate
in the absence of a magnetic ®eld. In the magnetic ®eld, this energy level is
split into ®ve levels: E 3 (triply degenerate), E 3 ì B B (doubly degenerate),
E 3 ÿ ì B B (doubly degenerate), E 3 2ì B B (non-degenerate), and E 3 ÿ 2ì B B
(non-degenerate). Energy levels for s orbitals (l 0) are not affected by the
application of the magnetic ®eld. Energies for p orbitals (l 1) are split by the