On the interior of (quantum) black holes
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10.1016/j.physletb.2013.06.031
Inclou dades d'ús des de 2022
Cita com:
hdl:2117/20319
Tipus de documentArticle
Data publicació2013-06-20
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Abstract
Different approaches to quantum gravity conclude that black holes may possess an
inner horizon, in addition to the (quantum corrected) outer ‘Schwarzschild’ horizon.
In this paper we assume the existence of this inner horizon and explain the physical
process that might lead to the tunneling of particles through it. It is shown that the
tunneling would produce a flux of particles with a spectrum that deviates from the pure
thermal one. Under the appropriate approximation the extremely high temperature of
this horizon is calculated for an improved quantum black hole. It is argued that the
flux of particles tunneled through the horizons affects the dynamics of the black hole
interior leading to an endogenous instability.
Descripció
Published in Physics letters B by ELSEVIER. The original publication is available at http://www.sciencedirect.com/science/article/pii/S0370269313005066
CitacióTorres, R. On the interior of (quantum) black holes. "Physics letters B", 20 Juny 2013, vol. 724, núm. 4-5, p. 338-345.
ISSN0370-2693
Versió de l'editorhttp://www.sciencedirect.com/science/article/pii/S0370269313005066
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