Pauli equation

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The Pauli equation is a Schrödinger equation which describes the time evolution of spin 1/2 particles (eg. electrons). It is the non-relativistic border case of the Dirac equation and can be used where particles are slow enough that relativistic effects can be neglected.

The Pauli equation was formulated by Wolfgang Pauli.

Contents

The time dependent linear Pauli equation :

(\vec{\sigma}\cdot \vec{p} - c)|\psi\rangle=0
where
\vec{p}is the momentum
c is the speed of light
\vec{\sigma} are the Pauli matrices
|\psi\rangle := \begin{pmatrix} |\psi_+\rangle \\                                        |\psi_-\rangle \end{pmatrix} is the Pauli-Spinor

Both spinor components satisfy the Schrödinger-Equation. This means that the system is as to the additional degree of freedom, degenerated.

With an external electromagnetic field the full Pauli equation reads:


\underbrace{i \hbar \partial_t \vec \varphi_\pm = \left( \frac{(\underline{\vec p}-q \cdot \vec A)^2}{2 m} + q \phi \right) \hat 1 \vec \varphi_\pm}_{\rm{Schr}\ddot o\rm{dingerequation}} - \underbrace{\frac{q \hbar}{2m}\vec{\hat \sigma} \cdot \vec B \vec \varphi_\pm}_{\rm Stern Gerlach  term}.

where

φ is the skalar electric potenial
A das Vector potential
\vec \varphi_\pm bzw. in Dirac-Notation |\psi\rangle :=\begin{pmatrix} |\varphi_+\rangle \\ |\varphi_-\rangle  \end{pmatrix} are the Pauli-Spinors
\vec{\hat \sigma} are the Pauli matrices
\vec B is the external magnetic field
\hat 1 two dimensional Identity matrix

With the Stern Gerlach term it is possible to comprehend the obtaing of spin orientation of atoms with one valence electron e.g. silver atoms which flow through an inhomogenous magntic field.

Analogous the term is resonsible for the energetic disperment in a magnetic field as can be viewed in the anomal Zeeman effect.

Starting from the Dirac equation for weak electromagnetic interactions :

i \hbar \partial_t \left( \begin{array}{c} \vec \varphi_1\\\vec \varphi_2\end{array} \right) = c \left( \begin{array}{c} \vec{\hat \sigma} \vec \pi \vec \varphi_2\\\vec{\hat \sigma} \vec \pi \vec \varphi_1\end{array} \right)+q \phi \left( \begin{array}{c} \vec \varphi_1\\\vec \varphi_2\end{array} \right) + mc^2 \left( \begin{array}{c} \vec \varphi_1 \\-\vec \varphi_2\end{array} \right)

with \vec \pi = \vec p - q \vec A

using the following approximatations :

  • Simplification of the equation through following ansatz
\left( \begin{array}{c} \vec \varphi_1 \\ \vec \varphi_2 \end{array}  \right) = e^{-i \frac{mc^2t}{\hbar}} \left( \begin{array}{c} \vec{\tilde \varphi_1} \\ \vec{\tilde \varphi_2} \end{array} \right)
  • Eliminating the rest energy through an Ansatz with slow time dependence
\partial_t \vec \varphi_i \ll \frac{mc^2}{\hbar} \vec \varphi_i
  • weak coupling of the electric potential
q \phi \ll mc^2

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