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Gravity and Strings

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5<br />

N = 1, 2, d = 4 supergravities<br />

In the previous chapter, we introduced increasingly complex theories of gravity, starting<br />

from GR, to accommodate fermions <strong>and</strong> we saw that the generalizations of GR that we had<br />

to use could be thought of as gauge theories of the symmetries of flat spacetime.<br />

Avery important development of the last few decades has been the discovery of supersymmetry<br />

<strong>and</strong> its application to the theory of fundamental particles <strong>and</strong> interactions.<br />

This symmetry relating bosons <strong>and</strong> fermions can be understood as the generalization of<br />

the Poincaré orAdS groups which are the symmetries of our background spacetime to the<br />

super-Poincaré or super-AdS (super-)groups which are the symmetries of our background<br />

superspacetime, ageneralization of st<strong>and</strong>ard spacetime that has fermionic coordinates.<br />

It is natural to construct generalizations of the st<strong>and</strong>ard gravity theories that can be understood<br />

as gauge theories of the (super-)symmetries of the background (vacuum) superspacetime.<br />

These generalizations are the supergravity (SUGRA) theories. Given that the kind<br />

of fermions that one can have depends critically on the spacetime dimension, the SUGRA<br />

theories that one can construct also depend critically on the spacetime dimension. Furthermore,<br />

one can extend the st<strong>and</strong>ard bosonic spacetime in different ways by including more<br />

than one (N) set of fermionic coordinates. This gives rise to additional supersymmetries<br />

relating them <strong>and</strong>, therefore, to supersymmetric field theories <strong>and</strong> SUGRA theories with N<br />

supersymmetries. The latter are also known as extended SUGRAs (SUEGRAs).<br />

There is, thus, a large variety of supergravities, but not infinitely large, because the gauging<br />

of supersymmetries with N > 8ind = 4 dimensions or N = 1ind = 11 needs the<br />

inclusion of more than one graviton <strong>and</strong>/or fields of spin higher than 2, which we do not<br />

know how to couple consistently.<br />

We are going to study SUGRA theories because they provide an interesting extension of<br />

the ideas we have reviewed so far <strong>and</strong> because the effective-field theories that describe the<br />

behavior of superstrings at low energies are SUGRA theories.<br />

Supersymmetry <strong>and</strong> SUGRA have been developed over the last several years <strong>and</strong> are<br />

currently the object of extensive work, so we cannot give here a complete review of any of<br />

these subjects. There are excellent books <strong>and</strong> reviews that cover most of the basic aspects,<br />

though, for instance [150, 404, 912, 915, 916, 946, 948]. Reference [828] contains reprints<br />

of many of the original articles on SUGRA.<br />

150

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