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arxiv: hep-th/0203048 · v2 · submitted 2002-03-06 · ✦ hep-th · gr-qc

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Microscopic Formulation of Black Holes in String Theory

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classification ✦ hep-th gr-qc
keywords blacktheorybraneholecorrespondenced1-d5dynamicsformulation
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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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Cited by 4 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. The Resolved Elliptic Genus and the D1-D5 CFT

    hep-th 2026-03 unverdicted novelty 8.0

    The resolved elliptic genus refines the supersymmetry index for the D1-D5 CFT by summing only over symmetry sectors that mix under a deformed supercharge, yielding agreement with supergravity below the black-hole thre...

  2. Chaos of Berry curvature for BPS microstates

    hep-th 2026-04 unverdicted novelty 7.0

    Berry curvature of BPS states is random-matrix-like for supersymmetric black hole microstates but non-random and often zero for horizonless geometries, offering a chaos diagnostic in degenerate sectors.

  3. Towering Gravitons in AdS$_3$/CFT$_2$

    hep-th 2026-04 unverdicted novelty 5.0

    A procedure dresses supergravitons with singletons to extend the BPS gravity-sector spectrum in AdS3/CFT2, yielding affine multiplets that match the D1-D5 CFT better after deformation up to higher levels.

  4. Testing the nature of dark compact objects: a status report

    gr-qc 2019-04 accept novelty 2.0

    Current and future observations can test whether dark compact objects are Kerr black holes or exotic alternatives, with null results strengthening the black hole paradigm.