Regular black holes with stable cores
Journal
Date Issued
2021
Author(s)
Abstract
Non-singular black hole geometries typically come with two spacetime
horizons: an (outer) event horizon and an (inner) Cauchy horizon. This nurtures
the speculation that they may be subject to a mass-inflation effect which
renders the Cauchy horizon unstable. We analyze the dynamics associated with
spherically symmetric, regular black holes taking the full backreaction between
the infalling matter and geometry into account. On this basis, we identify the
crucial features taming the growth of the mass function and diminishing the
curvature singularity at the Cauchy horizon. It is demonstrated explicitly that
the regular black hole solutions proposed by Hayward and obtained from
Asymptotic Safety satisfy these properties.
Volume
103
Issue
12
Issn Identifier
2470-0010
Rights
restricted
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