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Microscopic origin of the entropy of black holes in general relativity

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arxiv 2212.02447 v4 pith:2AGLTBV2 submitted 2022-12-05 hep-th gr-qc

Vijay Balasubramanian , Albion Lawrence , Javier M. Magan , Martin Sasieta This is my paper
classification hep-thgr-qc
keywords entropymicrostatesblackbridgesconstructdimensiongeneralholes
verification ladder T0 review T1 audit T2 compute T3 formal
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We construct an infinite family of microstates with geometric interiors for eternal black holes in general relativity with negative cosmological constant in any dimension. Wormholes in the Euclidean path integral for gravity cause these states to have small, but non-zero, quantum mechanical overlaps that have a universal form. The overlaps have a dramatic consequence: the microstates span a Hilbert space of log dimension equal to the Bekenstein-Hawking entropy. The semiclassical microstates we construct contain Einstein-Rosen bridges of arbitrary size behind their horizons. Our results imply that all these bridges can be interpreted as quantum superpositions of wormholes of size at most exponential in the entropy.

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Cited by 12 Pith papers

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

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