Phenomenological description of the interior of the Schwarzschild black hole

DOI10.1142/S0217751X15500918zbMath1325.83018arXiv1409.5784MaRDI QIDQ2946301

Publication date: 16 September 2015

Published in: International Journal of Modern Physics A (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1409.5784

zbMATH Keywords

Weyl anomaly backreaction black hole evaporation interior of black holes self-consistent solution of the semiclassical Einstein equation

Mathematics Subject Classification ID

Black holes (83C57) Methods of quantum field theory in general relativity and gravitational theory (83C47) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Exact solutions to problems in general relativity and gravitational theory (83C15)

Related Items (17)

Back reaction of 4D conformal fields on static black-hole geometry ⋮ The absence of horizon in black-hole formation ⋮ Obstruction of black hole singularity by quantum field theory effects ⋮ Comment on ``Self-consistent model of black hole formation and evaporation ⋮ Non-equilibrium thermodynamics of gravitational screens ⋮ Quantum fields during black hole formation: how good an approximation is the Unruh state? ⋮ On the near-horizon geometry of an evaporating black hole ⋮ UV and IR effects on Hawking radiation ⋮ A stringy effect on Hawking radiation ⋮ Static black holes with back reaction from vacuum energy ⋮ Gravitational wave echoes from macroscopic quantum gravity effects ⋮ Static black hole and vacuum energy: thin shell and incompressible fluid ⋮ Asymptotic states of black holes in KMY model ⋮ Trapping horizon and negative energy ⋮ The effective Tolman temperature in curved spacetimes ⋮ Role of evaporation in gravitational collapse ⋮ Planckian physics comes into play at Planckian distance from horizon

Cites Work

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