1996Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fieldsRequires access

Stability of the event horizon in (2+1)-dimensional black holes

Bin Wang, Ru-Keng Su, K.N. Yu, Enoch C. M. Young

Open publisher page 9 citations

Abstract

Three gedanken experiments constructed to test the cosmic censorship and the generalized second law of thermodynamics by attempting to exceed the extremality conditions of (2+1)-dimensional charged or rotating black holes are presented. These experiments correspond to the addition of matter with a negative gravitational energy, or an infalling classical charge, or a rotating shell to charged and rotating black holes, respectively. Even though the reasons for obstructing their falling into the black hole are different, we arrive at the same conclusions that the event horizon of a (2+1)-dimensional black hole is stable, and that the cosmic censorship and the generalized second law of thermodynamics are well protected.

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What this paper is about

Three gedanken experiments constructed to test the cosmic censorship and the generalized second law of thermodynamics by attempting to exceed the extremality conditions of (2+1)-dimensional charged or rotating black holes are presented. These experiments correspond to the addition of matter with a negative gravitational energy, or an infalling classical charge, or a rotating shell to charged and rotating black holes, respectively. Even though the reasons for obstructing their falling into the black hole are different, we arrive at the same conclusions that the event horizon of a (2+1)-dimensional black hole is stable, and that the cosmic censorship and the generalized second law of thermodynamics are well protected.

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OpenAlex reports 9 citations for this work. Citation counts describe recorded attention and do not establish research quality.

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Available abstract

Three gedanken experiments constructed to test the cosmic censorship and the generalized second law of thermodynamics by attempting to exceed the extremality conditions of (2+1)-dimensional charged or rotating black holes are presented. These experiments correspond to the addition of matter with a negative gravitational energy, or an infalling classical charge, or a rotating shell to charged and rotating black holes, respectively. Even though the reasons for obstructing their falling into the black hole are different, we arrive at the same conclusions that the event horizon of a (2+1)-dimensional black hole is stable, and that the cosmic censorship and the generalized second law of thermodynamics are well protected.

Key concepts: Cosmic censorship hypothesis, Event horizon, Physics, Black hole (networking), Charged black hole, Horizon, Apparent horizon, Gravitation

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