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Pauli matrices

From Encyclopedia of Mathematics - Reading time: 3 min


Certain special constant Hermitian (2×2)-matrices with complex entries. They were introduced by W. Pauli (1927) to describe spin (s=(/2)σ) and magnetic moment (μ=(e/2mc)σ) 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 v/c1. In explicit form the Pauli matrices are:

σ1=(0110);  σ2=(0ii0);  σ3=(1001).

Their eigen values are ±1. The Pauli matrices satisfy the following algebraic relations:

σiσk+σkσi=2δik,

σiσkσkσi=2iϵiklσl.

Together with the unit matrix

σ0=(1001)

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 ψA, A=1,2, 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 θ around an axis with a directed unit vector n, a spinor ψA is transformed according to the formula

ψA=[σ0,AB+12iθ(σn)AB]ψB,

σn=σ1nx+σ2ny+σ3nz.

From the Pauli matrices one can form the Dirac matrices γα, α=0,1,2,3:

γ0=(σ000σ0);  γk=(0σkσk0);  k=1,2,3.

The real linear combinations of σ0, iσ1, iσ2, iσ3 form a four-dimensional subalgebra of the algebra of complex (2×2)-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 SU(2). In this case they are generators of a 2-dimensional representation of SU(2) and are denoted by τ1, τ2 and τ3. Sometimes it is convenient to use the linear combinations

τ+=12(τ1+iτ2)= (0100);  τ=12(τ1iτ2)= (0010).

In certain cases one introduces for a relativistically covariant description of two-component spinor functions instead of the Pauli matrices, matrices Sα related by means of the following identities:

(1)S0S0+σ0=0;  SiS0=σi,  i=1,2,3,

where the symbol denotes complex conjugation. The matrices Sα satisfy the commutator relations

(2)SαSβ+SβSα=2ηα,β,

where ηα,β are the components of the metric tensor of the Minkowski space of signature +2. The formulas (1) and (2) make it possible to generalize the Pauli matrices covariantly to an arbitrary curved space:

SαSβ+SβSα=2gαβ,

where gαβ 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)

Comments[edit]

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)

How to Cite This Entry: Pauli matrices (Encyclopedia of Mathematics) | Licensed under CC BY-SA 3.0. Source: https://encyclopediaofmath.org/wiki/Pauli_matrices
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