The description of the hydrogen atom given earlier in chapter 4.3 is very accurate by engineering standards. However, it is not exact. This addendum examines various relativistic effects that were ignored in the analysis.
The approach will be to take the results of chapter 4.3 as the starting point. Then corrections are applied to them using perturbation theory as described in addendum {A.37}.
According to the description of the hydrogen atom given in chapter
4.3, all energy eigenfunctions
with the
same value of
have the same energy
.
energy levels for a given value of
are found to consist of several
closely spaced lines, rather than a single one. That is called the
“hydrogen atom fine structure.” It means that
eigenfunctions that all should have exactly the same energy,
don’t.
To explain why, the solution of chapter 4.3 must be
corrected for a variety of relativistic effects. Before doing so, it
is helpful to express the nonrelativistic energy levels of that
chapter in terms of the “rest mass energy”
of
the electron, as follows:
Nobody knows why it has the value that it has. Still, obviously it is
a measurable value, so, following the stated ideas of quantum
mechanics, maybe the universe “measured” this value
during its early formation by a process that we may never understand,
(since we do not have other measured values for
to deduce any
properties of that process from.) If you have a demonstrably better
explanation, Sweden awaits you.
In any case, for engineering purposes it is a small number, less than
1%. That makes the hydrogen energy levels really small compared to
the rest mass energy of the electron, because they are proportional to
the square of
,
And that in turn means that the relativistic errors in the hydrogen
energy levels are small. Still, even small errors can sometimes be
very important. The required corrections are listed below in order of
decreasing magnitude.
The electron should really be described relativistically using the
Dirac equation instead of classically. In classical terms, that
will introduce three corrections to the energy levels:
Hyperfine splitting couples the spins of proton and electron, and in the ground state, they combine in the singlet state. A slightly higher energy level occurs when they are in a spin-one triplet state; transitions between these states radiate very low energy photons with a wave length of 21 cm. This is the source of the “21 centimeter line” or “hydrogen line” radiation that is of great importance in cosmology. For example, it has been used to analyze the spiral arms of the galaxy, and the hope at the time of this writing is that it can shed light on the so called “dark ages” that the universe went through. Since so little energy is released, the transition is very slow, chapter 7.6.1. It takes on the order of 10 million years, but that is a small time on the scale of the universe.
The message to take away from that is that even errors in the ground state energy of hydrogen that are two million times smaller than the energy itself can be of critical importance under the right conditions.
The following subsections discuss each correction in more detail.
From the Dirac equation, it can be seen that three terms need to be added to the nonrelativistic Hamiltonian of chapter 4.3 to correct the energy levels for relativistic effects. The three terms are worked out in derivation {D.82}. But that mathematics really provides very little insight. It is much more instructive to try to understand the corrections from a more physical point of view.
The first term is relatively easy to understand. Consider
Einstein’s famous relation
,
is
energy,
mass, and
the speed of light. According to this
relation, the kinetic energy of the electron is not
,
the velocity, as Newtonian physics
says. Instead it is the difference between the energy
based on the mass
of the electron
in motion and the energy
based on the mass
of the
electron at rest. In terms of momentum
,
![]() |
(A.248) |
The second correction that must be added to the nonrelativistic
Hamiltonian is the so-called “spin-orbit interaction.”
In classical terms, it is due to the spin of the electron, which makes
it into a “magnetic dipole.” Think of it as a magnet of
infinitesimally small size, but with infinitely strong north and
south poles to make up for it. The product of the infinitesimal
vector from south to north pole times the infinite strength of the
poles is finite, and defines the magnetic dipole moment
.
So how big is this effect? Well, the energy of an electric dipole
in an electric field
is
The final correction that must be added to the nonrelativistic
Hamiltonian is the so-called “Darwin term:”
If that is not very satisfactory, the following much more detailed
derivation can be found on the web. It does succeed in
explaining the Darwin term fully within the nonrelativistic picture
alone. First assume that the electric potential of the nucleus does
not really become infinite as 1![]()
at
0, but is smoothed
out over some finite nuclear size. Also assume that the electron does
not “see” this potential sharply, but perceives of its
features a bit vaguely, as diffused out symmetrically over a typical
distance equal to the so-called Compton wave length
![]()
![]()
.
The key question is now what are the changes in the hydrogen energy
levels due to the three perturbations discussed above. That can be
answered by perturbation theory as soon as the good eigenfunctions
have been identified. Recall that the usual hydrogen energy
eigenfunctions
are made unique by the square angular
momentum operator
,
,
angular
momentum operator
,
,
giving the spin quantum number
for spin up, respectively down. The decisive term
whether these are good or not is the spin-orbit interaction. If the
inner product in it is written out, it is
Fortunately,
does commute with the net
angular
momentum
,
.
![\begin{eqnarray*}
& & [\L _x{\widehat S}_x,\L _z+{\widehat S}_z] = [\L _x,\L _...
...\L _z]{\widehat S}_z + \L _z[{\widehat S}_z,{\widehat S}_z] = 0
\end{eqnarray*}](img5303.gif)
Such good eigenfunctions can be constructed from the
by forming linear combinations of them that combine different
and
values. The coefficients of these good combinations are called
Clebsch-Gordan coefficients and are shown for
1 and
2 in figure 12.5. Note from this figure that the
quantum number
of net square momentum can only equal
or
.
,
,
,
,
angular momentum
.
As far as the other two contributions to the fine structure are
concerned, according to chapter 4.3.1
in the
Einstein term consists of radial functions and radial derivatives plus
.
,
and
,
,
,
.
with given values of
,
,
are good ones for the entire fine structure
Hamiltonian.
To get the energy changes, the Hamiltonian perturbation coefficients

The spin-orbit energy correction is

Finally the Darwin term,
To get the total energy change due to fine structure, the three
contributions must be added together. For
0, add the Einstein and
Darwin terms. For
0, add the Einstein and spin-orbit terms;
you will need to do the two possibilities that
and
separately. All three produce the same final result,
anyway:
In the ground state
can only be one half, (the electron spin), so
the ground state energy does not split into two due to fine structure.
You would of course not expect so, because in empty space, both spin
directions are equivalent. The ground state does show the largest
absolute change in energy.
Woof.
The weak Zeeman effect is the effect of a magnetic field that is
sufficiently weak that it leaves the fine structure energy
eigenfunctions almost unchanged. The Zeeman effect is then a small
perturbation on a problem in which the “unperturbed” (by
the Zeeman effect) eigenfunctions
derived in the
previous subsection are degenerate with respect to
and
.
The Zeeman Hamiltonian
However, the following simplistic derivation is usually given instead,
including in this book. First get rid of
by replacing it by
.
can then be
evaluated as being
,
If the
-
is substituted for
in the
expression for the Hamiltonian perturbation coefficients, the energy
changes are
In the intermediate Zeeman effect, the fine structure and Zeeman
effects are comparable in size. The dominant perturbation Hamiltonian
is now the combination of the fine structure and Zeeman ones. Since
the Zeeman part does not commute with
,
are no longer good. Eigenfunctions with the same
values of
and
,
must be
combined into good combinations. For example, if you look at
2, the eigenfunctions
and
have the same unperturbed energy and good
quantum numbers
and
.
and
eigenfunctions. To obtain the
matrix coefficients, use the Clebsch-Gordan coefficients from figure
12.5 to evaluate the effect of the Zeeman part. The fine
structure contributions to the matrices are given by (A.252)
when the
values are equal, and zero otherwise. This can be seen
from the fact that the energy changes must be the fine structure ones
when there is no magnetic field; note that
is a good quantum
number for the fine structure part, so its perturbation coefficients
involving different
values are zero.
A famous experiment by Lamb & Retherford in 1947 showed that the
hydrogen atom state
2,
0,
,![]()
2,
1,
,![]()
and same
total angular momentum quantum number
should have the same energy.
The difference in orbital angular momentum quantum number
should
not affect the energy.
The cause of the unexpected energy difference is called Lamb shift. To explain why it occurs would require quantum electrodynamics, and that is well beyond the scope of this book. Roughly speaking, the effect is due to a variety of interactions with virtual photons and electron/positron pairs. A good qualitative discussion on a nontechnical level is given by Feynman [18].
Here it must suffice to list the approximate energy corrections
involved. For states with zero orbital angular momentum, the energy
change due to Lamb shift is
It follows that the energy change is really small for states with
nonzero orbital angular momentum, which includes the ![]()
![]()
1, but
since there are no states with nonzero angular momentum in the ground
state, there is no splitting of spectral lines involved there.)
Qualitatively, the reason that the Lamb shift is small for states with
nonzero angular momentum has to do with distance from the nucleus.
The nontrivial effects of the cloud of virtual particles around the
electron are most pronounced in the strong electric field very close
to the nucleus. In states of nonzero angular momentum, the wave
function is zero at the nucleus, (D.9). So in those states
the electron is unlikely to be found very close to the nucleus. In
states of zero angular momentum, the square magnitude of the wave
function is 1![]()
at the nucleus, reflected in both the
much larger Lamb shift as well as its approximate 1![]()
dependence
on the principal quantum number
.
Hyperfine splitting of the hydrogen atom energy levels is due to the
fact that the nucleus acts as a little magnet just like the electron.
The single-proton nucleus and electron have magnetic dipole moments
due to their spin equal to
This discussion will restrict itself to the ground state, which is by
far the most important case. For the ground state, there is no
orbital contribution to the magnetic field of the electron. There is
only a “spin-spin coupling” between the magnetic moments
of the electron and proton, The energy involved can be thought of most
simply as the energy
of the electron in the
magnetic field
of the nucleus. If the nucleus is modelled
as an infinitesimally small electromagnet, its magnetic field is that
of an ideal current dipole as given in table 13.2. The
perturbation Hamiltonian then becomes
The good states are not immediately self-evident, so the four
unperturbed ground states will just be taken to be the ones which the
electron and proton spins combine into the triplet or singlet states
of chapter 5.5.6:
Now the first term in the spin-spin Hamiltonian does not produce a
contribution to the perturbation coefficients. The reason is that the
inner product of the perturbation coefficients written in spherical
coordinates involves an integration over the surfaces of constant
.
is constant on
these surfaces. So there will be terms like
in the integration, and those
are zero because
is just as much negative as positive on these
spherical surfaces, (as is
). There will also be terms like
in the integration. These will be zero too because by symmetry the
averages of
,
,
are equal on the
spherical surfaces, each equal to one third the average of
.
So only the second term in the Hamiltonian survives, and
the Hamiltonian perturbation coefficients become
The spatial integration in this inner product merely picks out the
value
1![]()
at the origin, as delta functions
do. That leaves the sum over the spin states. According to addendum
{A.10},
Plugging it all in and rewriting in terms of the Bohr energy and fine
structure constant, the energy changes are:
| (A.256) |