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String Theory and M-Theory

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11.5 The attractor mechanism 587<br />

clear: it can be interpreted as brane-antibrane annihilation. Specifically, for<br />

the set-up in the preceding subsection, where there are both left-moving <strong>and</strong><br />

right-moving Kaluza–Klein excitations, they can collide to give a massless<br />

closed-string state, which is then emitted from the black hole. The calculation<br />

has been carried out for ¯n ≪ n with the conclusion that the decay rate<br />

as a function of frequency is<br />

where the temperature is<br />

A<br />

dΓ(ω) =<br />

eω/T d<br />

− 1<br />

4k , (11.108)<br />

(2π) 4<br />

T = 2√¯n . (11.109)<br />

πR<br />

If one considers D1-brane anti-D1-brane or D5-brane/anti-D5-brane annihilations<br />

instead, then a different viewpoint is convenient. When a brane<br />

<strong>and</strong> an antibrane coincide, their common world volume contains a tachyonic<br />

mode that arises as the lowest mode of the open string that connects the<br />

brane to the antibrane. This tachyon signals an instability of the worldvolume<br />

theory, which results in the emission of closed-string radiation as<br />

in the previous discussion. In fact, one can test this reasoning by using<br />

Witten’s string field theory to describe the open string. Sen has argued persuasively<br />

that this theory gives a potential for the tachyon field, <strong>and</strong> that the<br />

decay corresponds to sliding down this potential from a local maximum to a<br />

local minimum, that is, tachyon condensation. Furthermore, the value of the<br />

potential at the minimum should be lower than its value at the maximum<br />

by exactly twice the brane tension. Thus the world-volume tachyon rolling<br />

to the minimum of its potential precisely corresponds to brane–antibrane<br />

annihilation. This results in the emission of closed-string quanta. In the<br />

black-hole setting considered here, these quanta comprise the Hawking radiation.<br />

This prediction for the gap between the maximum <strong>and</strong> minimum<br />

of the potential has been tested numerically in Witten’s bosonic string field<br />

theory, <strong>and</strong> it has been verified to high precision. Moreover, it has recently<br />

been derived analytically.<br />

11.5 The attractor mechanism<br />

Moduli fields<br />

As has been discussed in previous sections, black holes can appear when<br />

a superstring theory or M-theory is compactified to lower dimensions <strong>and</strong><br />

when branes are wrapped on nontrivial cycles of the compact manifold. The

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