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Journal of High Energy Physics

, 2016:157 | Cite as

Black holes turn white fast, otherwise stay black: no half measures

  • Carlos Barceló
  • Raúl Carballo-RubioEmail author
  • Luis J. Garay
Open Access
Regular Article - Theoretical Physics

Abstract

Recently, various authors have proposed that the dominant ultraviolet effect in the gravitational collapse of massive stars to black holes is the transition between a black-hole geometry and a white-hole geometry, though their proposals are radically different in terms of their physical interpretation and characteristic time scales [1, 2]. Several decades ago, it was shown by Eardley that white holes are highly unstable to the accretion of small amounts of matter, being rapidly turned into black holes [3]. Studying the crossing of null shells on geometries describing the black-hole to white-hole transition, we obtain the conditions for the instability to develop in terms of the parameters of these geometries. We conclude that transitions with long characteristic time scales are pathologically unstable: occasional perturbations away from the perfect vacuum around these compact objects, even if being imperceptibly small, suffocate the white-hole explosion. On the other hand, geometries with short characteristic time scales are shown to be robust against perturbations, so that the corresponding processes could take place in real astrophysical scenarios. This motivates a conjecture about the transition amplitudes of different decay channels for black holes in a suitable ultraviolet completion of general relativity.

Keywords

Black Holes Models of Quantum Gravity Spacetime Singularities 

Notes

Open Access

This article is distributed under the terms of the Creative Commons Attribution License (CC-BY 4.0), which permits any use, distribution and reproduction in any medium, provided the original author(s) and source are credited.

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Copyright information

© The Author(s) 2016

Authors and Affiliations

  • Carlos Barceló
    • 1
  • Raúl Carballo-Rubio
    • 1
    • 2
    Email author
  • Luis J. Garay
    • 3
    • 4
  1. 1.Instituto de Astrofísica de Andalucía (IAA-CSIC)GranadaSpain
  2. 2.Departamento de Geometría y Topología, Facultad de CienciasUniversidad de GranadaGranadaSpain
  3. 3.Departamento de Física Teórica IIUniversidad Complutense de MadridMadridSpain
  4. 4.Instituto de Estructura de la Materia (IEM-CSIC)MadridSpain

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