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String Theory and M-Theory

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4.3 Constraint equations <strong>and</strong> conformal invariance 119<br />

momentum tensor of the RNS string is<br />

Tαβ = ∂αX µ ∂βXµ + 1<br />

4 ¯ ψ µ ρα∂βψµ + 1<br />

4 ¯ ψ µ ρβ∂αψµ − (trace). (4.36)<br />

The conserved current associated with the global world-sheet supersymmetry<br />

of the RNS string is the world-sheet supercurrent. It can be constructed<br />

using the Noether method. Specifically, taking the supersymmetry parameter<br />

ε to be nonconstant, one finds that up to a total derivative the variation<br />

of the action (4.2) takes the form<br />

<br />

δS ∼ d 2 σ(∂α¯ε)J α , (4.37)<br />

where<br />

This current satisfies<br />

J α A = − 1<br />

2 (ρβ ρ α ψµ)A∂βX µ . (4.38)<br />

(ρα)ABJ α B = 0 (4.39)<br />

as a consequence of the identity ραρ β ρ α = 0. This is the analog of the<br />

tracelessness of the Tαβ. In fact, it can be traced back to local super-Weyl<br />

invariance in the formalism with local world-sheet supersymmetry. As a<br />

result, J α A has only two independent components, which can be denoted J+<br />

<strong>and</strong> J−.<br />

Written in terms of world-sheet light-cone coordinates, the nonzero components<br />

of the energy–momentum tensor in Eq. (4.36) are<br />

T++ = ∂+Xµ∂+X µ + i<br />

2 ψµ + ∂+ψ+µ , (4.40)<br />

T−− = ∂−Xµ∂−X µ + i<br />

2 ψµ −∂−ψ−µ . (4.41)<br />

Similarly, the nonzero components of the supercurrent in Eq. (4.38) are<br />

J+ = ψ µ<br />

+ ∂+Xµ <strong>and</strong> J− = ψ µ<br />

− ∂−Xµ. (4.42)<br />

The supercurrent (4.38) is conserved, ∂αJ α A<br />

equations of motion, which leads to<br />

= 0, as a consequence of the<br />

∂−J+ = ∂+J− = 0. (4.43)<br />

The energy–momentum tensor satisfies analogous relations<br />

∂−T++ = ∂+T−− = 0. (4.44)<br />

These relations follow immediately from the equations of motion ∂+∂−X µ =

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