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Microstates of non-supersymmetric black holes

1997/02/28 by Atish Dabholkar · 48 citations
Physics and Astronomy · #Black Holes and Theoretical Physics #Black brane #Black hole (networking) #Black hole thermodynamics #Cosmology and Gravitation Theories #Entropy (arrow of time) #Extremal black hole #Heterotic string theory #Mathematical physics #Noncommutative and Quantum Gravity Theories #Physics #Quantum mechanics #String theory #Supersymmetry #Theoretical physics #hep-th

paper · pdf · doi:10.1016/s0370-2693(97)00439-5

published in Physics Letters B 402(1-2), 53-58 (Elsevier BV) · 11 pages, harvmac, a paragraph about classical non-renormalization in asymptotically flat co-ordinates and references added

arxiv created 1997/03/19 · openalex publication_date 1997/06/01 · arxiv updated 2009/11/30 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05

Abstract

A five-dimensional dyonic black hole in Type-I theory is considered that is extremal but non-supersymmetric. It is shown that the Bekenstein-Hawking entropy of this black hole counts precisely the microstates of a D-brane configuration with the same charges and mass, even though there is no apparent supersymmetric nonrenormalization theorem for the mass. A similar result is known for the entropy at the stretched horizon of electrically charged, extremal, but non-supersymmetric black holes in heterotic string theory. It is argued that classical nonrenormalization of the mass may partially explain this result.

Citations