Evaporation of a nonsingular Reissner–Nordström black hole and the information loss problem

One of the attractive solutions to the information loss problem is that the event horizon does not appear in the process of gravitational collapse and subsequent evaporation once the spacetime singularity is regularized by some mechanism, as pointed out by Hayward and Frolov. In this paper, we exami...

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Published inProgress of theoretical and experimental physics Vol. 2023; no. 10
Main Authors Sueto, Kensuke, Yoshino, Hirotaka
Format Journal Article
LanguageEnglish
Published Oxford Oxford University Press 01.10.2023
Subjects
Black holes
Gravity
Metric system
Radiation
Spacetime
Theory of relativity
Online AccessGet full text
ISSN2050-3911
2050-3911
DOI10.1093/ptep/ptad111

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Abstract One of the attractive solutions to the information loss problem is that the event horizon does not appear in the process of gravitational collapse and subsequent evaporation once the spacetime singularity is regularized by some mechanism, as pointed out by Hayward and Frolov. In this paper, we examine whether this Hayward–Frolov scenario holds for the evaporation of a charged black hole. The process of collapse and evaporation is modeled with the charged Vaidya spacetime and two kinds of regularization of the central singularity are considered. Analyzing the spacetime structure of the evaporating black hole, we find that the appropriately regularized evaporating Reissner–Nordström “black hole” has no event and Cauchy horizons, indicating the possibility that the Hayward–Frolov scenario may have sufficient generality as the solution to the information loss problem. In addition, the properties of the nonsingular evaporating Reissner–Nordström black hole are examined in detail.
AbstractList One of the attractive solutions to the information loss problem is that the event horizon does not appear in the process of gravitational collapse and subsequent evaporation once the spacetime singularity is regularized by some mechanism, as pointed out by Hayward and Frolov. In this paper, we examine whether this Hayward–Frolov scenario holds for the evaporation of a charged black hole. The process of collapse and evaporation is modeled with the charged Vaidya spacetime and two kinds of regularization of the central singularity are considered. Analyzing the spacetime structure of the evaporating black hole, we find that the appropriately regularized evaporating Reissner–Nordström “black hole” has no event and Cauchy horizons, indicating the possibility that the Hayward–Frolov scenario may have sufficient generality as the solution to the information loss problem. In addition, the properties of the nonsingular evaporating Reissner–Nordström black hole are examined in detail.
Author Sueto, Kensuke
Yoshino, Hirotaka
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Snippet One of the attractive solutions to the information loss problem is that the event horizon does not appear in the process of gravitational collapse and...
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SubjectTerms Black holes
Gravity
Metric system
Radiation
Spacetime
Theory of relativity
Title Evaporation of a nonsingular Reissner–Nordström black hole and the information loss problem
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