The Schwarzschild singularity: a semiclassical bounce?
arXiv:1808.03717 · doi:10.1134/S0202289318040060
Abstract
We discuss the opportunity that the singularity inside a Schwarzschild black hole could be replaced by a regular bounce, described as a regular minimum of the spherical radius (instead of zero) and a regular maximum of the longitudinal scale (instead of infinity) in the corresponding Kantowski-Sachs metric. Such a metric in a vicinity of the bounce is shown to be a solution to the Einstein equations with the stress-energy tensor representing vacuum polarization of quantum matter fields, described by a combination of curvature-quadratic terms in the effective action. The indefinite parameters of the model can be chosen in such a way that it remains a few orders of magnitude apart from the Planck scale (say, on the GUT scale), that is, in a semiclassical regime.
arXiv comment6 pages, no figures. 5 references and some comments added
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Cited by in corpus (5)
- Bouncing compact objects. Part II: Effective theory of a pulsating Planck star
- Black Hole as a Quantum Field Configuration
- Overtones' outburst and Hawking evaporation of Kazakov-Solodukhin quantum corrected black hole
- Asymptotically flat vacuum solutions in order-reduced semiclassical gravity
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