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The Statistical Mechanics of the (2+1)-Dimensional Black Hole

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arxiv gr-qc/9409052 v1 pith:LZ3ITPRP submitted 1994-09-26 gr-qc hep-th

classification gr-qchep-th
keywords dimensionalblackholehorizonstatesappearancebreaksentropy
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The presence of a horizon breaks the gauge invariance of (2+1)-dimensional general relativity, leading to the appearance of new physical states at the horizon. I show that the entropy of the (2+1)-dimensional black hole can be obtained as the logarithm of the number of these microscopic states.

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Cited by 1 Pith paper

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  1. 3-dimensional charged black holes in $f({Q})$ gravity

    gr-qc 2025-06 conditional novelty 7.0 of 10

    New exact charged black hole solutions in (2+1)D f(Q) gravity with cubic form yield a novel AdS solution without GR counterpart, with multiple horizons, stable thermodynamics, and stable photon orbits.

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