Information conservation in de Sitter tunneling

Fuente: arXiv
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Autor principal: Tan, Baoyu
Formato: Preprint
Publicado: 2024
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author Tan, Baoyu
author_facet Tan, Baoyu
contents In this paper, we consider the three most general cases of progressive de Sitter spacetime. The charged and magnetic particles tunnel into the magnetically charged Reissner-Nordström de Sitter black hole (the most general case of a static black hole), the Kerr-Newman-Kasuya de Sitter black hole (the most general case of a rotating black hole), and Bardeen de Sitter black hole (black hole without singularities). We use Parikh-Wilczek method to calculate the radiation spectra of these black holes respectively, and find that they deviate from the pure thermal spectra, satisfying the unitary principle. Our results support the conservation of information and are generally true for all asymptotic de Sitter space-times.
format Preprint
id arxiv_https___arxiv_org_abs_2409_03653
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Information conservation in de Sitter tunneling
Tan, Baoyu
General Relativity and Quantum Cosmology
In this paper, we consider the three most general cases of progressive de Sitter spacetime. The charged and magnetic particles tunnel into the magnetically charged Reissner-Nordström de Sitter black hole (the most general case of a static black hole), the Kerr-Newman-Kasuya de Sitter black hole (the most general case of a rotating black hole), and Bardeen de Sitter black hole (black hole without singularities). We use Parikh-Wilczek method to calculate the radiation spectra of these black holes respectively, and find that they deviate from the pure thermal spectra, satisfying the unitary principle. Our results support the conservation of information and are generally true for all asymptotic de Sitter space-times.
title Information conservation in de Sitter tunneling
topic General Relativity and Quantum Cosmology
url https://arxiv.org/abs/2409.03653