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String Theory and M-Theory

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572 Black holes in string theory<br />

M-theory interpretation<br />

Starting from the Type IIA configuration described above, one can carry out<br />

two more T-duality transformations along the y 2 <strong>and</strong> y 3 directions to obtain<br />

a type IIA configuration consisting of Q1 D2-branes wrapped on y 2 <strong>and</strong> y 3 ,<br />

Q5 D2-branes wrapped on y 4 <strong>and</strong> y 5 <strong>and</strong> n fundamental strings wrapped on<br />

y 1 . This configuration can be interpreted at strong coupling as M-theory<br />

compactified on a 6-torus. Calling the M-theory circle coordinate y 6 , the n<br />

fundamental type IIA strings are then identified as n M2-branes wrapped<br />

on the y 1 <strong>and</strong> y 6 circles. The two sets of D2-branes are then identified as<br />

sets of M2-branes. Altogether, there are three sets of M2-branes wrapped<br />

on three orthogonal tori. This is a satisfying picture in that it puts the<br />

three sources of charges on a symmetrical footing, which nicely accounts for<br />

their symmetrical appearance in the entropy formula. The verification that<br />

this brane configuration gives the same entropy as before is a homework<br />

problem.<br />

Nonextremal three-charge black holes for D = 5<br />

The extremal three-charge black-hole solutions in five dimensions given<br />

above have nonextremal generalizations, which describe nonsupersymmetric<br />

black holes with finite temperature. These black holes are described by the<br />

metric<br />

where<br />

<strong>and</strong><br />

λ =<br />

3<br />

i=1<br />

<br />

1 +<br />

ds 2 = −h λ −2/3 dt 2 + λ 1/3<br />

<br />

dr2 h + r2dΩ 2 <br />

3 , (11.60)<br />

<br />

ri<br />

2<br />

r<br />

h = 1 − r2 0<br />

r 2<br />

(11.61)<br />

with r 2 i = r 2 0 sinh 2 αi, i = 1, 2, 3. (11.62)<br />

This reduces to the extremal metric in Eq. (11.46) in the limit r0 → 0<br />

with ri held fixed. Moreover, the limit αi → 0 with r0 held fixed gives the<br />

Schwarzschild metric in five dimensions given in Eq. (11.9).<br />

The mass of this black hole can be read off using the same rules as before<br />

resulting in<br />

M = πr2 0<br />

(cosh 2α1 + cosh 2α2 + cosh 2α3) . (11.63)<br />

8G5

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