Hawking-like radiation from evolving black holes and compact horizonless objects

DOI10.1007/JHEP02(2011)003zbMath1294.83034arXiv1011.5911OpenAlexW2070101104WikidataQ59619495 ScholiaQ59619495MaRDI QIDQ407286

Matt Visser, Stefano Liberati, Sebastiano Sonego, Carlos Barceló

Publication date: 29 August 2014

Published in: Journal of High Energy Physics (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1011.5911

zbMATH Keywords

black holesspacetime singularitiesmodels of quantum gravity2D gravity

Mathematics Subject Classification ID

Black holes (83C57) Quantization of the gravitational field (83C45) Methods of quantum field theory in general relativity and gravitational theory (83C47) Space-time singularities, cosmic censorship, etc. (83C75)

Related Items (20)

Non-singular rotating black hole with a time delay in the center ⋮ The absence of horizon in black-hole formation ⋮ Hawking versus Unruh effects, or the difficulty of slowly crossing a black hole horizon ⋮ Black holes turn white fast, otherwise stay black: no half measures ⋮ Thermality of the Hawking flux ⋮ Comment on ``Self-consistent model of black hole formation and evaporation ⋮ On the viability of regular black holes ⋮ Hawking radiation in Lorentz violating gravity: a tale of two horizons ⋮ Quantum vacuum effects on the formation of black holes ⋮ Energy levels of a scalar particle in a static gravitational field close to the black hole limit ⋮ Entropy bounds for uncollapsed rotating bodies ⋮ Thermal Hawking radiation of black hole with supertranslation field ⋮ Gravitational wave echoes from macroscopic quantum gravity effects ⋮ Opening the Pandora’s box at the core of black holes ⋮ Analogue gravity ⋮ The trans-Planckian problem as a guiding principle ⋮ Entropy bounds in terms of the \(w\) parameter ⋮ A model of the collapse and evaporation of charged black holes ⋮ Grey-body factors, irreversibility and multiple island saddles ⋮ Evading the trans-Planckian problem with Vaidya spacetimes

Cites Work

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• Particle creation by black holes
• Naked and thunderbolt singularities in black hole evaporation
• Penrose diagram for a transient black hole
• Hawking-Like Radiation Does Not Require a Trapped Region
• Properties of black hole radiation from tunnelling
• Particle production in time-dependent gravitational fields: the expanding mass shell
• Hawking Radiation without Black Hole Entropy
• Hawking radiation in different coordinate settings: complex paths approach
• More general sudden singularities
• Acoustic black holes: horizons, ergospheres and Hawking radiation
• Sudden future singularities
• Hawking Radiation As Tunneling
• Black hole explosions?
• Dynamical origin of black-hole radiance
• Production and decay of evolving horizons
• Quasi-particle creation by analogue black holes
• Black hole evaporation: a paradigm
• ON HAWKING RADIATION AS TUNNELING WITH BACK-REACTION
• ESSENTIAL AND INESSENTIAL FEATURES OF HAWKING RADIATION
• Necessary and sufficient conditions for big bangs, bounces, crunches, rips, sudden singularities and extremality events
• Analogue gravity
• Quantum Fields in Curved Space

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