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

2 Pith papers cite this work. Polarity classification is still indexing.

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abstract

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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fields

gr-qc 1 hep-th 1

years

2025 1 1997 1

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representative citing papers

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

gr-qc · 2025-06-11 · conditional · novelty 7.0

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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