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Gravity and Strings

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390 Unbroken supersymmetry<br />

The superalgebra will now include a bosonic generator associated with the constantgauge<br />

transformations that rotate the spinor doublets <strong>and</strong> leave the vector field invariant.<br />

This generator must appear in the anticommutator of two supercharges <strong>and</strong> the corresponding<br />

structure constants are given by the bilinears −i ¯κ(αi)σ 2 κ(β j) = Cαβɛij.<br />

13.4 The vacua of d = 5, 6 supergravities with eight supercharges<br />

To complete our overview of supergravity vacua in lower dimensions, we are going to<br />

study the vacua of the minimal supergravities in d = 5 <strong>and</strong> 6 dimensions that are related by<br />

dimensional reduction with N = 2, d = 4 Poincaré supergravity <strong>and</strong> have the same number<br />

of supercharges. Almost all the maximally supersymmetric vacua of these theories also<br />

happen to be related by dimensional reduction [664].<br />

13.4.1 N = (1, 0), d = 6 supergravity<br />

The fields of this theory are the metric êâ ˆµ , 2-form field ˆB −<br />

with anti-self-dual field<br />

ˆµˆν<br />

strength ˆH − = 3∂ ˆB − <strong>and</strong> positive-chirality symplectic Majorana–Weyl gravitino ˆψ +<br />

ˆµ [727]<br />

(we use the gamma matrices of Appendix B).<br />

To write an action for an anti-self-dual 3-form, one has to introduce auxiliary fields.<br />

Alternatively, one can write an action for a generic 3-form,<br />

<br />

ˆS =<br />

d6 <br />

ˆx | ˆg| ˆR + 1<br />

12<br />

ˆH 2<br />

<br />

, (13.98)<br />

<strong>and</strong> impose the anti-self-duality constraint ⋆ ˆH − =− ˆH − on the equations of motion. The<br />

Killing-spinor equation is <br />

ˆ∇<br />

1<br />

− â 48 ˆH − <br />

ˆγ ˆκ â<br />

+ = 0, (13.99)<br />

where ˆκ + is a spinor of positive chirality.<br />

Three maximally supersymmetric vacua of this theory are known: 13 Minkowski spacetime,<br />

the near-horizon limit of the extreme anti-self-dual string solution [441] that has an<br />

AdS3 × S 3 geometry, <strong>and</strong> the KG6 Hpp-wave solution [690]. The latter can be obtained by<br />

taking the Penrose limit of the former [158, 495, 764].<br />

The AdS3 × S 3 solution can be written as follows:<br />

d ˆs 2 = R 2 3 d2 (3) − R2 3 d2 (3) ,<br />

ˆH − = 4R3(ωAdS3 + ω S 3),<br />

(13.100)<br />

13 Actually, it has been shown in [229] that the maximally supersymmetric vacua of this theory <strong>and</strong> of N =<br />

(2, 0), d = 6 supergravity are in one-to-one correspondence, <strong>and</strong> their metrics are locally isometric to biinvariant<br />

Lorentzian metrics of six-dimensional Lie groups with anti-self-dual parallelizing torsion. The<br />

three solutions that we present have this property <strong>and</strong> exhaust all the possibilities.

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