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String Theory Demystified

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CHAPTER 14 Black Holes 247<br />

hole squared. In terms of area, the entropy is 1/4 of the area of the horizon in units<br />

of Planck length:<br />

A<br />

S = (14.25)<br />

2<br />

4 Let us compute the temperature in the case of a Schwarzschild black hole. In the<br />

Chapter Quiz you will get a chance to try your luck fi nding the temperature of a<br />

charged black hole. We follow a procedure outlined in a note published by P.R.<br />

Silva. 2<br />

We proceed as follows. We perform a Wick rotation t→iτand write the<br />

Schwarzschild metric as<br />

Now set<br />

ds<br />

p<br />

Computing the Temperature of a Black Hole<br />

GM<br />

GM 2 2<br />

1 d<br />

dr r<br />

r<br />

r<br />

2<br />

1 2<br />

⎛ ⎞ ⎛ ⎞<br />

=− −<br />

⎝<br />

⎜<br />

⎠<br />

⎟ τ + −<br />

⎝<br />

⎜<br />

⎠<br />

⎟ + dΩ 2 (14.26)<br />

2 4 2 4<br />

12 /<br />

⎛ GM⎞<br />

Rdα<br />

= − dτ<br />

⎝<br />

⎜1<br />

r ⎠<br />

⎟<br />

−<br />

⎛ GM⎞<br />

dR = − d<br />

⎝<br />

⎜<br />

r ⎠<br />

⎟<br />

2<br />

1 2<br />

4<br />

12 /<br />

4 r<br />

and integrate. We take the limits of integration to be<br />

This gives us two relations:<br />

α : 0≤α ≤2π<br />

τ : 0 ≤τ ≤β<br />

r: G m≤ r′ ≤ r<br />

2 4<br />

−1<br />

−12<br />

/ 12 /<br />

2πR= ( 2G m) ( r−2G m)<br />

β<br />

4<br />

12<br />

R= 22 ( G m) ( r−2G m)<br />

4<br />

/ 12 /<br />

4<br />

2 Available on the arXiv at http://arxiv.org/ftp/gr-qc/papers/0605/0605051.pdf.<br />

4<br />

(14.27)<br />

(14.28)

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