Black hole inner horizon evaporation in semiclassical gravity

DOI10.1088/1361-6382/ABF89CzbMath1480.83070arXiv2011.07331OpenAlexW3154354155MaRDI QIDQ5163286

Raúl Carballo-Rubio, Valentin Boyanov, Luis J. Garay, Carlos Barceló

Publication date: 3 November 2021

Published in: Classical and Quantum Gravity (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/2011.07331

zbMATH Keywords

black holessemiclassical gravityHawking evaporationinner horizon instability

Mathematics Subject Classification ID

Black holes (83C57) Quantum field theory on curved space or space-time backgrounds (81T20) Semiclassical techniques, including WKB and Maslov methods applied to problems in quantum theory (81Q20) Asymptotic procedures (radiation, news functions, (mathcal{H} )-spaces, etc.) in general relativity and gravitational theory (83C30) Approximation procedures, weak fields in general relativity and gravitational theory (83C25)

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Cites Work

• Particle creation by black holes
• On the viability of regular black holes
• Inner structure of a charged black hole: An exact mass-inflation solution
• Structure of the singularity inside a realistic rotating black hole
• Internal Geometry of an Evaporating Black Hole
• Black Hole Singularities: A Numerical Approach
• Quantum instability of the Cauchy horizon in Reissner–Nordström–deSitter spacetime
• Opening the Pandora’s box at the core of black holes
• Black hole explosions?
• The Large Scale Structure of Space-Time
• On Continued Gravitational Contraction
• Quantum Fields in Curved Space
• General Relativity

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