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References - Bogoliubov Laboratory of Theoretical Physics - JINR

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or<br />

Equation (1) may then be written, using the usual formula for covariant differentiation<br />

Sμ;ν = Sμ,ν − Γ λ μνSλ<br />

Si;0 = Si,0 − Γ λ i0 Sλ = Si,0 − Γ k i0 Sk , (3)<br />

where the connection coefficients Γλ μν<br />

relevant non-zero coefficients are Γ2 10 = ω, Γ1 20 = −ω, giving<br />

or (with ω = ωn)<br />

(2)<br />

are calculated from the above metric tensor. The<br />

S1;0 = S1,0 − Γ 2 10S2 = S1,0 − ωS2,<br />

S2;0 = S2,0 + ωS1, S3;0 = S3,0, (4)<br />

DS<br />

Dt<br />

= dS<br />

dt<br />

+ Ω ∧ S.<br />

as in (1) above.<br />

From a fundamental perspective, however, spin is not described by a 4-vector, but by<br />

a rank 2 antisymmetric tensor. Indeed, the total angular momentum Jμν contains orbital<br />

and spin parts<br />

Jμν = Lμν + Sμν<br />

andasiswellknownJμν are the generators <strong>of</strong> the Lorentz group. The most pr<strong>of</strong>ound<br />

analysis <strong>of</strong> spin, however, was made by Wigner [2] in 1939, who pointed out that to<br />

describe spin it is insufficient to consider the (homogeneous) Lorentz group. Instead the<br />

group <strong>of</strong> translations in space-time must be added, yielding the inhomogeneous Lorentz<br />

group, or Poincaré group. This has generators Pμ and Jμν , and spin is generated by little<br />

group <strong>of</strong> the Poincaré group. The structure <strong>of</strong> this group depends on the sign <strong>of</strong> P μ Pμ.<br />

With metric (+, −, −, −) massive particles have P μ Pμ = m 2 . In the nonrelativistic limit<br />

spin is described by the rotation group SO(3) or SU(2), and indeed this turns out to be<br />

true for all states with P μ Pμ > 0:<br />

P μ Pμ > 0 (timelike states) : little group is SU(2) .<br />

Wigner showed, however, that for other values P μ Pμ the little group has a different<br />

structure:<br />

P μ Pμ < 0 (spacelike states) : little group is SO(2, 1) .<br />

P μ Pμ = 0 (null states) : little group is E(2).<br />

Thus, for example, the spin <strong>of</strong> spacelike (virtual) particles in Feynman diagrams is not<br />

properly described by the rotation group, but by the noncompact group SO(2,1).<br />

Wigner’s analysis identified the group structure <strong>of</strong> the little groups but did not reveal<br />

the actual forms <strong>of</strong> the generators <strong>of</strong> these groups, leaving the question, what are<br />

these generators? The Casimir operators <strong>of</strong> the Poincaré groupareP μ Pμ and W μ Wμ ,<br />

describing, in effect, the mass and spin <strong>of</strong> quantum states. Here Wμ is the Pauli-Lubanski<br />

vector<br />

Wμ = 1<br />

2 ɛμνκλJ νκ P λ .<br />

452

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