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The aim of this chapter is to develop a quantum mechanical theory of electron
dynamics that is consistent with special relativity. Such a theory is needed
to explain the origin of electron spin (which is essentially a relativistic effect),
and to account for the fact that the spin contribution to the electron's magnetic
moment is twice what we would naively expect by analogy with (non-relativistic)
classical physics (see Section 5.5). Relativistic electron theory is
also required to fully understand the fine structure of the hydrogen
atom energy levels (recall, from Section 7.7, and Exercises 3 and 4, that the modification to the energy
levels due to spin-orbit coupling is of the same order of magnitude as the
first-order correction due to the electron's relativistic mass increase.)
In the following, we shall use
,
,
to represent the Cartesian coordinates
,
,
, respectively, and
to represent
.
The time dependent wavefunction then takes the form
. Adopting
standard relativistic notation, we write the four
's as
, for
. A space-time
vector with four components that transforms under Lorentz transformation in an analogous manner to the four space-time coordinates
is termed a 4-vector, and its components are written like
(i.e., with an upper
Greek suffix). We can lower the suffix according to the rules
 |
 |
(1098) |
 |
 |
(1099) |
 |
 |
(1100) |
 |
 |
(1101) |
Here, the
are called the contravariant components of the vector
, whereas the
are termed the covariant components. Two 4-vectors
and
have the Lorentz invariant scalar product
 |
(1102) |
a summation being implied over a repeated letter suffix. The metric tenor
is defined
 |
 |
(1103) |
 |
 |
(1104) |
 |
 |
(1105) |
 |
 |
(1106) |
with all other components zero.
Thus,
 |
(1107) |
Likewise,
 |
(1108) |
where
,
, with all other components zero.
Finally,
if
, and
otherwise.
In the Schrödinger representation, the momentum of a particle, whose components are written
,
,
, or
,
,
,
is represented by the operators
 |
(1109) |
for
. Now, the four operators
form the covariant components of a
4-vector whose contravariant components are written
. So, to make
expression (1109) consistent with relativistic theory, we must first write it with its
suffixes balanced,
 |
(1110) |
and then extend it to the complete 4-vector equation
 |
(1111) |
According to standard relativistic theory, the new operator
, which forms a 4-vector when
combined with the momenta
, is interpreted as the energy of the particle divided by
, where
is the velocity of
light in vacuum.
Next: Dirac Equation
Up: Relativistic Electron Theory
Previous: Relativistic Electron Theory
Richard Fitzpatrick
2013-04-08