04.06.2013 Views

Gravity and Strings

Gravity and Strings

Gravity and Strings

SHOW MORE
SHOW LESS

Create successful ePaper yourself

Turn your PDF publications into a flip-book with our unique Google optimized e-Paper software.

328 The Kaluza–Klein black hole<br />

Lower-dimensional S dualities <strong>and</strong> generation of KK branes. In this example, we are<br />

also going to study a three-step mechanism for generating new solutions that exploits the<br />

existence of an S-duality symmetry in the four-dimensional KK theory, as discussed in<br />

Section 11.2.4.<br />

1. Reduction of a purely gravitational five-dimensional solution to a four-dimensional<br />

KK-theory solution.<br />

2. S dualization of the four-dimensional KK-theory solution.<br />

3. Oxidation of the S-dualized KK-theory solution to a new purely gravitational fivedimensional<br />

solution.<br />

In particular, we are going to apply this recipe to the “black pp-wave” solutions given<br />

in Eqs. (11.153). Using the transformation Eq. (11.93) on the four-dimensional solution<br />

Eq. (11.154), we immediately obtain<br />

ds2 KK = Wdt2 <br />

− H W −1dr2 + r 2d2 <br />

(2) ,<br />

d ˜s 2 E = H − 1 2 Wdt2 − H 1 <br />

2 W −1dr2 + r 2d2 <br />

(2) ,<br />

˜F = αhd 2 ,<br />

˜k = H − 1 2 ,<br />

H = 1 + h r , W = 1 + ω r , ω= h(1 − α2 ).<br />

(11.155)<br />

The solution is naturally given in terms of the field strength ˜F. Finding the potential<br />

is equivalent to solving the Dirac-monopole problem, which we already solved in Section<br />

8.7.2. Here we simply quote the result: in spherical coordinates the non-vanishing<br />

components of ˜F are<br />

˜Fθϕ = αh sin θ = ∂θ Ãϕ, ⇒ Ãϕ =−αh cos θ, (11.156)<br />

up to gauge transformations. This potential is singular at θ = 0 <strong>and</strong> θ = π <strong>and</strong> the solution<br />

to this problem is to define the potential in two different patches à (±)<br />

ϕ related by a gauge<br />

transformation:<br />

à (±)<br />

ϕ =±αh(1 ∓ cos θ). (11.157)<br />

It is useful to rewrite the equation that the untilded A has to satisfy (the Dirac-monopole<br />

equation) in a coordinate-independent way that will allow us to generalize the solutions,<br />

∂[i A j] = αk −1 1<br />

0 2ɛijk∂k H. (11.158)<br />

All the properties that depend only on the modified Einstein-frame metric (singularities,<br />

horizons, causality, extremality, thermodynamics etc.) are the same as in the electric case.<br />

The characteristic features of the magnetic BH appear in the KK frame <strong>and</strong> in ˆd dimensions.

Hooray! Your file is uploaded and ready to be published.

Saved successfully!

Ooh no, something went wrong!