The fate of black hole horizons in semiclassical gravity

DOI10.1016/J.PHYSLETB.2018.09.027zbMath1404.83038arXiv1712.09914OpenAlexW2777056652WikidataQ129223087 ScholiaQ129223087MaRDI QIDQ1632139

Debajyoti Sarkar, Clément Berthiere, Sergey N. Solodukhin

Publication date: 13 December 2018

Published in: Physics Letters. B (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1712.09914

Mathematics Subject Classification ID

Black holes (83C57) Quantization of the gravitational field (83C45)

Related Items (6)

Tunneling of massless and massive particles from a quantum deformed Schwarzschild black hole surrounded by quintessence ⋮ Back reaction of 4D conformal fields on static black-hole geometry ⋮ Logarithmic terms in entropy of Schwarzschild black holes in higher loops ⋮ Reissner–Nordström geometry counterpart in semiclassical gravity ⋮ Strong field lensing by Damour-Solodukhin wormhole ⋮ Wormholes in conformal gravity

Cites Work

• Firewalls as artefacts of inconsistent truncations of quantum geometries
• Wormholes as black hole foils
• Quantum Fields in Curved Space
• Planckian \(\text{AdS}_2\times S_2\) space is an exact solution of the semiclassical Einstein equations

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