Black Brane Entropy from Brane-Antibrane Systems

Astronomy and Astrophysics – Astrophysics – General Relativity and Quantum Cosmology

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6 pages, revtex; aimed at non-string-theorists. Invited talk at the IV Mexican Workshop on Gravitation and Mathematical Physic

Scientific paper

In the context of string theory, it is possible to explain the microscopic origin of the entropy of certain black holes in terms of D-brane systems. To date, most of the cases studied in detail refer to extremal (supersymmetric) or near-extremal black holes. In this work we propose a microscopic model for certain black branes (extended versions of black holes) which would apply to cases arbitrarily far from extremality, including the Schwarzschild case. The model is based on a system of D-branes and anti-D-branes, and is able to reproduce several properties of the corresponding supergravity solution. In particular, the microscopic entropy agrees with supergravity, except for a factor of 2^{p/p+1}, where p is the dimension of the brane.

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