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In
atomic physics, the
fine structure describes the splitting of the
spectral lines of
atoms due to
electron spin and
relativistic corrections to the non-relativistic
Schrödinger equation. It was first measured precisely for the
hydrogen atom by
Albert A. Michelson and
Edward W. Morley in 1887
[1] laying the basis for the theoretical treatment by
Arnold Sommerfeld, introducing the
fine-structure constant.
[2]
Background
Gross structure
The
gross structure of line spectra is the line spectra predicted by the quantum mechanics of non-relativistic electrons with no spin. For a
hydrogenic atom, the gross structure energy levels only depend on the
principal quantum number n. However, a more accurate model takes into account relativistic and spin effects, which break the
degeneracy
of the energy levels and split the spectral lines. The scale of the
fine structure splitting relative to the gross structure energies is on
the order of (
Zα)
2, where
Z is the
atomic number and
α is the
fine-structure constant, a
dimensionless number equal to approximately 1/137.
Relativistic corrections
The fine structure energy corrections can be obtained by using
perturbation theory. To perform this calculation one must add the three corrective terms to the
Hamiltonian:
the leading order relativistic correction to the kinetic energy, the
correction due to the spin-orbit coupling, and the Darwin term coming
from the quantum fluctuating motion or
zitterbewegung of the electron.
These corrections can also be obtained from the non-relativistic limit of the
Dirac equation, since Dirac's theory naturally incorporates relativity and
spin interactions.
The hydrogen atom
This sections discusses the analytical solutions for the
hydrogen atom as the problem is completely solvable and its the base model for energy level calculations in more complex atoms.
Kinetic energy relativistic correction
Classically, the kinetic energy term of the
Hamiltonian is
where
is the momentum and
is the mass of the electron.
However, when considering a more accurate theory of nature via
special relativity, we must use a relativistic form of the kinetic energy,
where the first term is the total relativistic energy, and the second term is the
rest energy of the electron (
is the
speed of light). Expanding this in a
Taylor series ( specifically a
binomial series ), we find
Then, the first order correction to the Hamiltonian is
Using this as a
perturbation, we can calculate the first order energy corrections due to relativistic effects.
where
is the unperturbed wave function. Recalling the unperturbed Hamiltonian, we see
We can use this result to further calculate the relativistic correction:
For the hydrogen atom,
,
, and
,
where
is the
Bohr Radius,
is the
principal quantum number and
is the
azimuthal quantum number. Therefore, the first order relativistic correction for the hydrogen atom is
where we have used:
On final calculation, the order of magnitude for the relativistic correction to the ground state is
.
Spin-orbit coupling
For a
hydrogen-like atom with
protons, orbital momentum
and electron spin
, the spin-orbit term is given by:
is the electron mass,
is the
vacuum permittivity and
is the spin
g-factor.
is the distance of the electron from the nucleus.
The
spin-orbit correction can be understood by shifting from the standard
frame of reference (where the
electron orbits the
nucleus)
into one where the electron is stationary and the nucleus instead
orbits it. In this case the orbiting nucleus functions as an effective
current loop, which in turn will generate a magnetic field. However, the
electron itself has a magnetic moment due to its
intrinsic angular momentum. The two magnetic vectors,
and
couple together so that there is a certain energy cost depending on
their relative orientation. This gives rise to the energy correction of
the form
Notice that there is a factor of 2, called the
Thomas precession, which comes from the relativistic calculation that changes back to the electron's frame from the nucleus frame.
Since
the expectation value for the Hamiltonian is:
Thus the order of magnitude for the spin-orbital coupling is
.
Darwin term
There is one last term in the non-relativistic expansion of the
Dirac equation. It is referred to as the Darwin term, as it was first derived by
Charles Galton Darwin, and is given by:
The Darwin term affects only the s orbitals. This is because the wave function of an electron with
vanishes at the origin, hence the
delta function has no effect. For example, it gives the 2s orbital the same energy as the 2p orbital by raising the 2s state by
9.057×10−5 eV.
The Darwin term changes the effective potential at the nucleus. It
can be interpreted as a smearing out of the electrostatic interaction
between the electron and nucleus due to
zitterbewegung, or rapid quantum oscillations, of the electron. This can be demonstrated by a short calculation.
[3]
Quantum fluctuations allow for the creation of
virtual electron-positron pairs with a lifetime estimated by the
uncertainty principle . The distance the particles can move during this time is
, the
Compton wavelength. The electrons of the atom interact with those pairs. This yields a fluctuating electron position
. Using a
Taylor expansion, the effect on the potential
can be estimated:
Averaging over the fluctuations
gives the average potential
Approximating
, this yields the perturbation of the potential due to fluctuations:
To compare with the expression above, plug in the
Coulomb potential:
This is only slightly different.
Another mechanism that affects only the s-state is the
Lamb shift, a further, smaller correction that arises in
quantum electrodynamics
that should not be confused with the Darwin term. The Darwin term gives
the s-state and p-state the same energy, but the Lamb shift makes the
s-state higher in energy than the p-state.
Total effect
The full Hamiltonian is given by
where
is the Hamiltonian from the
Coulomb interaction.
The total effect, obtained by summing the three components up, is given by the following expression:
[4]
where
is the
total angular momentum (
if
and
otherwise). It is worth noting that this expression was first obtained by Sommerfeld based on the
old Bohr theory; i.e., before the modern
quantum mechanics was formulated.
Exact relativistic energies
The
total effect can also be obtained by using the Dirac equation. In this
case, the electron is treated as non-relativistic. The exact energies
are given by
[5]
This expression, which contains all higher order terms that were left
out in the other calculations, expands to first order to give the
energy corrections derived from perturbation theory. However, this
equation does not contain the
hyperfine structure corrections, which are due to interactions with the nuclear spin. Other corrections from
quantum field theory such as the Lamb shift and the
anomalous magnetic dipole moment of the electron are not included.