Pauli equation

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The Pauli Equation, also known as the Schrödinger-Pauli equation, is the formulation of the Schrödinger equation for spin one-half particles which takes into account the interaction of the particle's spin with the electromagnetic field. 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

[edit] Details

The Pauli equation is stated as:

\left[ \frac{1}{2m}(\vec{\sigma}\cdot(\vec{p} - q \vec{A}))^2 + q \phi \right] |\psi\rangle = i \hbar \frac{\partial}{\partial t} |\psi\rangle

Where:

  • m \ \ is the mass of the particle.
  • q \ \ is the charge of the particle.
  • \vec{\sigma} \ \ is a three-component vector of the two-by-two Pauli matrices. This means that each component of the vector is a Pauli matrix.
  • \vec{p} \ \ is the three-component vector of the momentum operators. The components of this vector are - i \hbar \frac{\partial}{\partial x_n}
  • \vec{A} \ \ is the three-component magnetic vector potential.
  • \phi \ \ is the electric scalar potential.
  • |\psi\rangle \ \ is the two component spinor wavefunction, which can be represented as \begin{pmatrix} \psi_0 \\ \psi_1 \end{pmatrix} .

Somewhat more explicitly, the Pauli equation is:

\left[ \frac{1}{2m} \left( \sum_{n=1}^3 (\sigma_n ( - i \hbar \frac{\partial}{\partial x_n} - q A_n)) \right) ^2 + q \phi \right] \begin{pmatrix} \psi_0 \\ \psi_1 \end{pmatrix} = i \hbar \begin{pmatrix} \frac{ \partial \psi_0 }{\partial t} \\ \frac{ \partial \psi_1 }{\partial t} \end{pmatrix}

Notice that the Hamiltonian (the expression between square brackets) is a two-by-two matrix operator, because of the Pauli σ matrices.

[edit] Relationship to the Schrödinger Equation and the Dirac Equation

The Pauli equation is non-relativistic, but it does predict spin. As such, it can be thought of an occupying the middle ground between:

Note that because of the properties of the Pauli matrices, if the magnetic vector potential \bold{A} is equal to zero, then the equation reduces to the familiar Schrodinger equation for a particle in a purely electric potential φ, except that it operates on a two component spinor. Therefore, we can see that the spin of the particle only affects its motion in the presence of a magnetic field.

[edit] Special Cases

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

With an external electromagnetic field the full Pauli equation reads:

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

where

φ is the scalar electric potential
A the electromagnetic vector potential
\vec \varphi_\pm, in Dirac notation |\psi\rangle :=\begin{pmatrix} |\varphi_+\rangle \\ |\varphi_-\rangle \end{pmatrix}, are the Pauli spinor components
\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 obtaining of spin orientation of atoms with one valence electron e.g. silver atoms which flow through an inhomogeneous magnetic field.

Analogously, the term is responsible for the splitting of spectral lines (corresponding to energy levels) in a magnetic field as can be viewed in the anomalous Zeeman effect.

[edit] Derivation of the Pauli equation by Schrodinger

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

[edit] Examples

[edit] References

[edit] External links