Microscopic formulation of black holes in string theory |
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| Affiliation: | 1. Department of Physics, University of California, Santa Barbara, CA 93106, USA;2. Research Department of Theoretical Physics, Tata Institute of Fundamental Research, Homi Bhabha Road, Mumbai 400 005, India;1. DISTAL, University of Bologna, Via G. Fanin 50, 40127 Bologna, Italy;2. DiGeSA, University of Catania, Via S. Sofia 100, 95123 Catania, Italy;3. DAFNAE, University of Padova, Viale dell''Università 16, 35020 Legnaro, PD, Italy;4. DiSTAfA, University of Reggio Calabria, Via Feo di Vito, 89122 Reggio Calabria, Italy;1. Dipartimento di Matematica, Politecnico di Milano, Piazza Leonardo da Vinci 32, 20133 Milano, Italy;2. DICATAM, Sezione di Matematica, Università degli studi di Brescia, Via Branze, 38, 25123 Brescia, Italy;1. Mathematics and Statistics, Lancaster University, UK;2. Shell Research Ltd., Manchester, M22 0RR, UK;1. Key Laboratory of Thermo-Fluid Science and Engineering, Ministry of Education, International Joint Research Laboratory of Thermal Science and Engineering, Xi’an Jiaotong University, Shaanxi 710049, China;2. Research Institute of State Grid Jiangsu Electric Power Company Ltd, China |
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| Abstract: | ![]()
In this report we review the microscopic formulation of the five-dimensional black hole of type IIB string theory in terms of the D1–D5 brane system. The emphasis here is more on the brane dynamics than on supergravity solutions. We show how the low energy brane dynamics, combined with crucial inputs from AdS/CFT correspondence, leads to a derivation of black hole thermodynamics and the rate of Hawking radiation. Our approach requires a detailed exposition of the gauge theory and conformal field theory of the D1–D5 system. We also discuss some applications of the AdS/CFT correspondence in the context of black hole formation in three dimensions by thermal transition and by collision of point particles. |
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