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arXiv · 2107.01556

How Anti-de Sitter Black Holes Reach Thermal Equilibrium

Ru Ling·Hao Xu·Yen Chin Ong
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Abstract

It is commonly known in the literature that large black holes in anti-de Sitter spacetimes (with reflective boundary condition) are in thermal equilibrium with their Hawking radiation. Focusing on black holes with event horizon of toroidal topology, we study a simple model to understand explicitly how this thermal equilibrium is reached under Hawking evaporation. It is shown that it is possible for a large toroidal black hole to evolve into a small (but stable) one.

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Ru Ling, Hao Xu, Yen Chin Ong. 2021-07-04. How Anti-de Sitter Black Holes Reach Thermal Equilibrium. https://doi.org/10.1016/j.physletb.2022.136896

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