Semiclassical black holes and horizon singularities

In spherical symmetry, solutions of the semiclassical Einstein equations belong to one of two possible classes. Both classes contain solutions that - depending on the dynamic behavior of the horizon - describe evaporating physical black holes or expanding white holes (trapped/anti-trapped regions th...

Full description

Bibliographic Details
Main Authors: Dahal, P.K (Author), Murk, S. (Author), Terno, D.R (Author)
Format: Article
Language:English
Published: American Institute of Physics Inc. 2022
Online Access:View Fulltext in Publisher