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Modave Lectures on Fuzzballs and Emission from the D1-D5 System

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arxiv 1001.1444 v3 pith:4JD2W7E2 submitted 2010-01-10 hep-th

classification hep-th
keywords emissionfuzzballsblackcertaind1-d5d1-d5-pdifferentdiscussion
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These lecture notes present an introduction to the fuzzball proposal and emission from the D1-D5 system which is geared to an audience of graduate students and others with little background in the subject. The presentation begins with a discussion of the Penrose process and Hawking radiation. The fuzzball proposal is then introduced, and the two- and three-charge systems are reviewed. In the three-charge case details are not discussed. A detailed discussion of emission calculations for D1-D5-P black holes and for certain non-extremal fuzzballs from both the gravity and CFT perspectives is included. We explicitly demonstrate how seemingly different emission processes in gravity, namely, Hawking radiation and superradiance from D1-D5-P black holes, and ergoregion emission from certain non-extremal fuzzballs, are only different manifestations of the same phenomenon in the CFT.

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Cited by 2 Pith papers

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

  1. Quasinormal modes of supersymmetric microstate geometries from the D1-D5 CFT

    hep-th 2019-08 conditional novelty 6.0 of 10

    In the near-decoupling limit, the scalar quasinormal mode spectrum of GMS microstate geometries is reproduced exactly by D1-D5 orbifold CFT emission amplitudes, including the slow-decaying ERS modes.

  2. Space cannot stretch too {\it fast}

    hep-th 2025-05 reject novelty 5.0 of 10

    The essay proposes that fast stretching of space releases energy stored in vacuum entanglements left by virtual black hole microstates, resolving the information paradox and yielding dark energy.

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