Moving mirrors and event horizons in non-flat background geometry

Fuente: arXiv
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Autor principal: Ievlev, Evgenii
Formato: Preprint
Publicado: 2023
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author Ievlev, Evgenii
author_facet Ievlev, Evgenii
contents Moving mirrors have been used for a long time as simple models for studying various properties of black hole radiation, such as the thermal spectrum and entanglement entropy. These models are typically constructed to mimic the collapse of a spherically symmetric distribution of matter in the Minkowski background. We generalize this correspondence to the case of non-trivial background geometry and consider two examples, the Schwarzschild -- de Sitter black hole and the Bañados--Teitelboim--Zanelli (BTZ) black hole. In the BTZ case we were also able to show that this approach works for the spinning black hole which has only axial symmetry.
format Preprint
id arxiv_https___arxiv_org_abs_2311_07403
institution arXiv
publishDate 2023
record_format arxiv
spellingShingle Moving mirrors and event horizons in non-flat background geometry
Ievlev, Evgenii
General Relativity and Quantum Cosmology
High Energy Physics - Theory
Moving mirrors have been used for a long time as simple models for studying various properties of black hole radiation, such as the thermal spectrum and entanglement entropy. These models are typically constructed to mimic the collapse of a spherically symmetric distribution of matter in the Minkowski background. We generalize this correspondence to the case of non-trivial background geometry and consider two examples, the Schwarzschild -- de Sitter black hole and the Bañados--Teitelboim--Zanelli (BTZ) black hole. In the BTZ case we were also able to show that this approach works for the spinning black hole which has only axial symmetry.
title Moving mirrors and event horizons in non-flat background geometry
topic General Relativity and Quantum Cosmology
High Energy Physics - Theory
url https://arxiv.org/abs/2311.07403