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Microscopic origin of the entropy of astrophysical black holes

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arxiv 2212.08623 v3 pith:MUXQLR2G submitted 2022-12-16 hep-th gr-qc

Vijay Balasubramanian , Albion Lawrence , Javier M. Magan , Martin Sasieta This is my paper
classification hep-thgr-qc
keywords blackentropyholesmicrostatesoriginoverlapsareaastrophysical
verification ladder T0 review T1 audit T2 compute T3 formal
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We construct an infinite family of microstates for black holes in Minkowski spacetime which have effective semiclassical descriptions in terms of collapsing dust shells in the black hole interior. Quantum mechanical wormholes cause these states to have exponentially small, but universal, overlaps. We show that these overlaps imply that the microstates span a Hilbert space of log dimension equal to the event horizon area divided by four times the Newton constant, explaining the statistical origin of the Bekenstein-Hawking entropy.

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Cited by 7 Pith papers

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

  1. A Holographic Map from AdS$_3$ to CFT$_2$

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  7. The Baby Universe is Fine and the CFT Knows It: On Holography for Closed Universes

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