1999Unpublished venueRequires access

Pair Creation of Black Holes in Anti-de Sitter Space Background

Zhong Chao Wu

Open publisher page 21 citations

Abstract

For a spherically symmetric vacuum model with a negative cosmological constant, a complex constrained instanton is considered as the seed for quantum pair creation of Schwarzschild-anti-de Sitter black holes. The relative creation probability is found to be the exponential of the negative of one quarter of the black hole horizon area or the black hole entropy. In the absence of a general no-boundary proposal for open creation, the constrained instanton approach is used in treating both the open and closed paircreation of black holes.

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What this paper is about

For a spherically symmetric vacuum model with a negative cosmological constant, a complex constrained instanton is considered as the seed for quantum pair creation of Schwarzschild-anti-de Sitter black holes. The relative creation probability is found to be the exponential of the negative of one quarter of the black hole horizon area or the black hole entropy. In the absence of a general no-boundary proposal for open creation, the constrained instanton approach is used in treating both the open and closed paircreation of black holes.

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Available abstract

For a spherically symmetric vacuum model with a negative cosmological constant, a complex constrained instanton is considered as the seed for quantum pair creation of Schwarzschild-anti-de Sitter black holes. The relative creation probability is found to be the exponential of the negative of one quarter of the black hole horizon area or the black hole entropy. In the absence of a general no-boundary proposal for open creation, the constrained instanton approach is used in treating both the open and closed paircreation of black holes.

Key concepts: de Sitter–Schwarzschild metric, Physics, Black hole (networking), Nonsingular black hole models, Instanton, Extremal black hole, Exponential function, Charged black hole

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