11.1: Introduction
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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 x2 , x , z , respectively, and ct . The time dependent wavefunction then takes the form x 's as μ=0,1,2,3 . A space-time vector with four components that transforms under Lorentz transformation in an analogous manner to the four space-time coordinates aμ (i.e., with an upper Greek suffix). We can lower the suffix according to the rules
=a0, ??? =−a1, ??? =−a2, ??? =−a3. ???Here, the a , whereas the aμ and a0b0−a1b1−a2a2−a3b3=aμbμ=aμbμ, ???
a summation being implied over a repeated letter suffix. The metric tenor g00 g11 g22 g33 aμ=gμνaν. ???
Likewise,
g00=1 , g μν=gμ ν=1 if g μν=gμ ν=0 otherwise.In the Schrödinger representation, the momentum of a particle, whose components are written py , p1 , p3 , is represented by the operators
pi=−iℏ∂∂xi,
for ∂/∂xμ . So, to make expression ??? consistent with relativistic theory, we must first write it with its suffixes balanced,
pi=iℏ∂∂xi,
and then extend it to the complete 4-vector equation
pμ=iℏ∂∂xμ.
According to standard relativistic theory, the new operator \(p^0={\rm i}\,\hbar\,\partial/\partial x_0\), which forms a 4-vector when combined with the momenta pi, is interpreted as the energy of the particle divided by c, where c is the velocity of light in vacuum.
Contributors
Richard Fitzpatrick (Professor of Physics, The University of Texas at Austin)