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Gravity and Strings

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6.3 The positive-energy theorem 183<br />

These two terms are manifestly positive. The second one vanishes if we use spinors<br />

satisfying the Witten condition<br />

γ i ei µ ∇µɛ = 0. (6.61)<br />

Thus, we have proven that, if the dominant energy condition is satisfied <strong>and</strong> we use<br />

spinors satisfying the Witten condition, I (ɛ) is non-negative.<br />

2. We rewrite I (ɛ) as follows:<br />

I (ɛ) = 1<br />

<br />

d 2<br />

2 µνɛ µνρσ ¯ɛγ5γσ ∇ρɛ, (6.62)<br />

∂<br />

<strong>and</strong> exp<strong>and</strong> the integr<strong>and</strong> around the vacuum ¯gµν (Minkowski spacetime) to which the<br />

solution asymptotically tends. We also impose on the chosen spinors that they admit the<br />

expansion<br />

where r →∞at spatial infinity <strong>and</strong><br />

<br />

1<br />

ɛ = ɛ0 + O ,<br />

r<br />

(6.63)<br />

¯∇µɛ0 = 0. (6.64)<br />

A spinor satisfying this condition in N = 1 SUGRA is a Killing spinor of the solution ¯gµν.<br />

Since ∇µ = ¯∇µ − 1<br />

4 ωµ ab γab <strong>and</strong> the integral is taken at spatial infinity,<br />

I (ɛ) =− 1<br />

8<br />

<br />

d 2 µνɛ µνρσ ¯ɛ0γ5γσ ∇ρɛ0 = 1<br />

4<br />

<br />

d 2 ρµν,γ<br />

µν −3g αβωρ αβ <br />

k0 γ<br />

= 1<br />

4 E(k0), (6.65)<br />

where we have used Eq. (6.34) <strong>and</strong> the fact that<br />

k a 0 = i ¯ɛ0γ a ɛ0<br />

(6.66)<br />

is, trivially, a Killing vector of the vacuum ¯gµν. When it is timelike, k0 is the generator of<br />

translations in time <strong>and</strong> E(k0) is just the mass.<br />

This proves that M ≥ 0 <strong>and</strong> M = 0for Minkowski spacetime.<br />

The above relation between Killing spinors <strong>and</strong> Killing vectors is quite generic <strong>and</strong>, with<br />

minor adaptations, is true in most SUGRAs. Just as the Killing vectors of a metric constitute<br />

a Lie algebra that generates its isometry group, the Killing spinors <strong>and</strong> Killing vectors<br />

of a solution of a SUGRA theory, which may involve other fields apart from the metric,<br />

constitute a superalgebra that generates a supergroup that leaves the solution invariant. The<br />

simplest case is Minkowski spacetime, whose invariance supergroup is the super-Poincaré<br />

one.

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