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Gravity and Strings

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514 Extended objects<br />

p-brane solutions of the p-brane a-model we are about to study can be built by “dressing”<br />

it with appropriate factors.<br />

18.2.2 The p-brane a-model<br />

As we have already said, this is the simplest model that embodies the main characteristics<br />

of the string effective action (<strong>and</strong> supergravity actions): gravity coupled to one scalar <strong>and</strong><br />

a (p + 1)-form to which the scalar couples non-minimally. It generalizes the a-model for<br />

BHs that we used before, which appears here as the p = 0case, but here we canonically<br />

normalize the (p + 1)-form field strengths. The action is 10<br />

S =<br />

1<br />

16πG (d)<br />

N<br />

<br />

d d x <br />

|g| R + 2(∂ϕ) 2 + (−1)p+1<br />

2 · (p + 2)! e−2aϕ F 2<br />

<br />

(p+2) , (18.61)<br />

where F(p+2) = dA(p+1) is the field strength of the (p + 1)-form potential A(p+1).<br />

The equations of motion are<br />

Gµν + 2T ϕ µν<br />

1<br />

− 2e−2aϕT A(p+1)<br />

µν = 0,<br />

∇2ϕ + (−1)p+1<br />

4 · (p + 2)! ae−2aϕ F 2<br />

(p+2)<br />

<br />

−2aϕ<br />

∇µ e F(p+2) µν1···νp+1<br />

= 0,<br />

= 0,<br />

(18.62)<br />

where T A(p+1) is the (p + 1)-form energy–momentum tensor, given in Eq. (1.122). As<br />

usual, not all of them are independent in general (they can be derived from the Bianchi<br />

identities). On the other h<strong>and</strong>, the solutions we will find will be defined up to gauge transformations,<br />

including large gauge transformations that change the asymptotic behavior of<br />

the fields so the physics could be inequivalent. The classical equations of motion are insensitive<br />

to these subtleties.<br />

We want to find single-charged-black-p-brane solutions of an analogous nature to the<br />

black Schwarzschild p-brane of the previous section. The method we used to construct<br />

them in Section 11.3.3 cannot be used in the presence of p-forms: we cannot simply add<br />

extra dimensions to a lower-dimensional charged BH metric. For instance, if we took a<br />

four-dimensional RN BH <strong>and</strong> added several extra dimensions, we would obtain a higherdimensional<br />

metric with vanishing scalar curvature (as in four dimensions) but now the<br />

trace of the Maxwell energy-momentum tensor would not be zero in more than four dimensions.<br />

Another way of expressing the same fact is that, if we dimensionally reduce<br />

the above action to d − p dimensions, one does not simply obtain the above action written<br />

directly in d − p dimensions, but one finds extra fields. In particular, one finds extra<br />

10 This action is equivalent to the original one written in [557] (whose main results we reobtain in a different<br />

fashion here) which was given in the string frame. Here we do not want to assume that the scalar is the<br />

dilaton <strong>and</strong> thus we prefer to use an Einstein-frame action. The constant a is, then, not the same as in [557]<br />

butweobtain simpler, more-symmetric expressions.

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