Dual brane pairs and the Bekenstein-Hawking entropy of non-Susy spacetimes

Details Dual brane pairs and the Bekenstein-Hawking entropy of non-Susy spacetimes Dual brane pairs and the Bekenstein-Hawking entropy of non-Susy spacetimes

Jun 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003cqgra..20s.533k&link_type=abstract

Classical and Quantum Gravity, Volume 20, Issue 12, pp. S533-S540 (2003).

Computer Science

2

Scientific paper

A novel approach is described towards a microscopic understanding of the Bekenstein-Hawking entropy of non-supersymmetric spacetimes - including the Schwarzschild black hole. It is based at an intermediate step on the description of the event horizon in terms of dual Euclidean brane pairs of type-II string theory or M theory. By counting specific chain structures on the brane complex, it is shown that one can reproduce the exact Schwarzschild black hole entropy plus its logarithmic correction.

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