Properties of black holes in toroidally compactified string theory

DOI10.1016/s0920-5632(97)00303-4zbMath0925.83069arXivhep-th/9701152OpenAlexW2108237188WikidataQ126866042 ScholiaQ126866042MaRDI QIDQ6205112

Mirjam Cvetič

Publication date: 10 June 1997

Published in: Nuclear Physics. B. Proceedings Supplements (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/hep-th/9701152

zbMATH Keywords

duality symmetriesM theoryBekenstein Hawking entropyADM massintersecting M branesR R sector

Mathematics Subject Classification ID

Black holes (83C57) String and superstring theories in gravitational theory (83E30) String and superstring theories; other extended objects (e.g., branes) in quantum field theory (81T30)

Related Items (1)

Microscopic formulation of black holes in string theory

Cites Work

• Black holes in higher dimensional space-times
• Black hole solutions in heterotic string theory on a torus
• Microscopic origin of the Bekenstein-Hawking entropy
• Black holes and \(U\)-duality
• Internal structure of black holes
• Massless black holes and conifolds in string theory
• Enhanced gauge symmetries in superstring theories
• Harmonic superpositions of \(M\)-branes
• Intersecting \(M\)-branes as four-dimensional black holes
• Extremal black hole entropy from conformal string sigma model
• Overlapping branes in M-theory
• Non-extreme black holes from non-extreme intersecting M-branes
• Dirichlet Branes and Ramond-Ramond Charges

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