Matter Accretion Versus Semiclassical Bounce in Schwarzschild Interior

Matter Accretion Versus Semiclassical Bounce in Schwarzschild Interior

We discuss the properties of the previously constructed model of a Schwarzschild black hole interior where the singularity is replaced by a regular bounce, ultimately leading to a white hole. We assume that the black hole is young enough so that the Hawking radiation may be neglected. The model is s...

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Bibliographic Details
Main Authors: Kirill Bronnikov, Sergey Bolokhov, Milena Skvortsova
Format: Article
Language:English
Published: MDPI AG 2020-10-01
Series:Universe
Subjects:
general relativity
semiclassical gravity
quantum corrections
bounce solution
Schwarzschild black hole
particle creation
Online Access:https://www.mdpi.com/2218-1997/6/10/178

Internet

https://www.mdpi.com/2218-1997/6/10/178

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