Certain special constant Hermitian -matrices with complex entries. They were introduced by W. Pauli (1927) to describe spin ()
and magnetic moment
of an electron. His equation describes correctly in the non-relativistic case particles of spin 1/2 (in units )
and can be obtained from the Dirac equation for .
In explicit form the Pauli matrices are:
Their eigen values are .
The Pauli matrices satisfy the following algebraic relations:
Together with the unit matrix
the Pauli matrices form a complete system of second-order matrices by which an arbitrary linear operator (matrix) of dimension 2 can be expanded. They act on two-component spin functions ,
,
and are transformed under a rotation of the coordinate system by a linear two-valued representation of the rotation group. Under a rotation by an infinitesimal angle
around an axis with a directed unit vector ,
a spinor
is transformed according to the formula
From the Pauli matrices one can form the Dirac matrices ,
:
The real linear combinations of ,
,
,
form a four-dimensional subalgebra of the algebra of complex -matrices (under matrix multiplication) that is isomorphic to the simplest system of hypercomplex numbers, the quaternions, cf. Quaternion. They are used whenever an elementary particle has a discrete parameter taking only two values, for example, to describe an isospin nucleon (a proton-neutron). Quite generally, the Pauli matrices are used not only to describe isotopic space, but also in the formalism of the group of inner symmetries .
In this case they are generators of a -dimensional representation of
and are denoted by ,
and .
Sometimes it is convenient to use the linear combinations
In certain cases one introduces for a relativistically covariant description of two-component spinor functions instead of the Pauli matrices, matrices
related by means of the following identities:
where the symbol
denotes complex conjugation. The matrices
satisfy the commutator relations
where
are the components of the metric tensor of the Minkowski space of signature .
The formulas (1) and (2) make it possible to generalize the Pauli matrices covariantly to an arbitrary curved space:
where
are the components of the metric tensor of the curved space.
References[edit]
[1] | W. Pauli, , Works on quantum theory , 1–2 , Moscow (1975–1977) (In Russian; translated from German) |
[2] | N.F. Nelina, "Physics of elementary particles" , Moscow (1977) (In Russian) |
[3] | D. Bril, J.A. Wheeler, , The latest problems on gravitation , Moscow (1961) pp. 381–427 (In Russian) |
References[edit]
[a1] | W. Pauli, "Zur Quantenmechanik des magnetischen Elektrons" Z. Phys. , 43 : 601 |
[a2] | W. Pauli (ed.) , Handbuch der Physik , 24 , Springer (1933) |
[a3] | R.M. Wald, "General relativity" , Univ. Chicago Press (1984) pp. Chapt. 4 |
[a4] | Y. Choquet-Bruhat, C. DeWitt-Morette, M. Dillard-Bleick, "Analysis, manifolds and physics" , North-Holland (1982) (Translated from French) |