Black Hole Bounces on the Road to Quantum Gravity

Quantum resolutions of the space-time singularity at the end of gravitational collapse may provide hints towards the properties of a final theory of Quantum-Gravity. The mechanism by which the singularity is avoided and replaced by a bounce depends on the specific behaviour of gravity in the strong...

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Bibliographic Details
Main Author: Daniele Malafarina
Format: Article
Language:English
Published: MDPI AG 2018-08-01
Series:Universe
Subjects:
Online Access:http://www.mdpi.com/2218-1997/4/9/92
Description
Summary:Quantum resolutions of the space-time singularity at the end of gravitational collapse may provide hints towards the properties of a final theory of Quantum-Gravity. The mechanism by which the singularity is avoided and replaced by a bounce depends on the specific behaviour of gravity in the strong field and may have implications for the geometry of the space-time also in the weak field. In the last few decades, several scenarios for black hole bounces have been proposed and I shall argue that the times are now mature to ask the question of whether such bounces can be observed in astrophysical phenomena.
ISSN:2218-1997