- Pauli equation
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 theelectromagnetic field . It is the non-relativistic border case of theDirac equation and can be used where particles are slow enough that relativistic effects can be neglected.The Pauli equation was formulated by
Wolfgang Pauli .Details
The Pauli equation is stated as:
::
Where:
* is the mass of the particle.
* is the charge of the particle.
* is a three-component vector of the two-by-twoPauli matrices . This means that each component of the vector is a Pauli matrix.
* is the three-component vector of the momentumoperators . The components of this vector are
* is the three-component magnetic vector potential.
* is the electric scalar potential.
* is the two componentspinor wavefunction, which can be represented as .Somewhat more explicitly, the Pauli equation is:
::
Notice that the Hamiltonian (the expression between square brackets) is a two-by-two matrix operator, because of the Pauli matrices.
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:
* The familiar Schrödinger Equation (on a complex scalarwavefunction ), which is non-relativistic and does not predict spin.
* The Dirac Equation (on a complex four-component spinor), which is fully relativistic (with respect tospecial relativity ) and predicts spin.Note that because of the properties of the Pauli matrices, if the magnetic vector potential is equal to zero, then the equation reduces to the familiar Schrödinger equation for a particle in a purely electric potential , 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.
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:
.where :: is the scalar electric
potential :: the electromagneticvector potential ::, in Dirac notation , are the Paulispinor components:: are thePauli matrices :: is the externalmagnetic field :: two dimensionalIdentity matrix With the
Stern Gerlach term it is possible to comprehend the obtaining of spin orientation of atoms with onevalence 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 .Derivation of the Pauli equation by Schrodinger
Starting from the Dirac equation for weak electromagnetic interactions :
withusing the following approximatations :
* Simplification of the equation through following ansatz ::
* Eliminating the rest energy through an Ansatz with slow time dependence::
* weak coupling of the electric potential::Examples
References
*cite book | author=Schwabl, Franz| title=Quantenmechanik I | publisher=Springer |year=2004 |id=ISBN 978-3540431060
*cite book | author=Schwabl, Franz| title=Quantenmechanik für Fortgeschrittene | publisher=Springer |year=2005 |id=ISBN 978-3540259046
*cite book | author=Claude Cohen-Tannoudji, Bernard Diu, Frank Laloe| title= Quantum Mechanics 2| publisher=Wiley, J |year=2006 |id=ISBN 978-0471569527External links
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