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2.3 Fine structure 39

as shown in Fig. 2.5(b). For both configurations, it is easy to see that
the spin–orbit interaction does not shift the mean energy


E=(2j+1)Ej(n, l)+(2j′+1)Ej′(n, l), (2.58)

wherej′=l− 1 /2andj=l+1/2 for the two levels. This calculation of
the ‘centre of gravity’ for all the states takes into account the degeneracy
of each level.
(b)


No spin−orbit
interaction

(a)

No spin−orbit
interaction

Fig. 2.5The fine structure of hydro-
gen. The fine structure of (a) the 2p
and (b) the 3d configurations are drawn
on different scales: β2p is consider-
ably greater thanβ3d.Allp-andd-
configurations look similar apart from
an overall scaling factor.

The spin–orbit interaction does not affect the 2 S 1 / 2 or 3 S 1 / 2 so we
might expect these levels to lie close to the centre of gravity of the
configurations withl>0. This is not the case. Fig. 2.6 shows the
energies of the levels for then= 3 shell given by a fully relativistic
calculation. We can see that there are other effects of similar magnitude
to the spin–orbit interaction that affect these levels in hydrogen. Quite
remarkably, these additional relativistic effects shift the levels by just the
rightamounttomakenP 1 / 2 levels degenerate with thenS 1 / 2 levels, and
nP 3 / 2 degenerate withnD 3 / 2. This structure does not occur by chance,
but points to a deeper underlying cause. The full explanation of these
observations requires relativistic quantum mechanics and the technical
details of such calculations lie beyond the scope of this book.^52 We shall


(^52) See graduate-level quantum mechan-
ics texts, e.g. Sakurai (1967) and Series
(1988).
simply quote the solution of the Dirac equation for an electron in a
Coulomb potential; this gives a formula for the energyEDirac(n, j)that
depends only onnandj, i.e. it gives the same energy for levels of the
samenandjbut differentl, as in the cases above. In a comparison of the
Relativistic
mass
Non-relativistic limit
Darwin term
for s-electrons
Relativistic
mass
Spin−orbit
Relativistic Spin−orbit
mass
S P D
Fig. 2.6The theoretical positions of the energy levels of hydrogen calculated by the fully relativistic theory of Dirac depend
onnandjonly (notl), as shown in this figure for then= 3 shell. In addition to the spin–orbit interaction, the effects that
determine the energies of these levels are: the relativistic mass correction and, for s-electrons only, the Darwin term (that
accounts for relativistic effects that occur at smallr, where the electron’s momentum becomes comparable tomec).

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