End of a black hole’s evaporation. II.

Farshid Soltani, Carlo Rovelli, and Pierre Martin-Dussaud
Phys. Rev. D 104, 066015 – Published 14 September 2021

Abstract

We derive an explicit expression for the transition amplitude from black to white hole horizon at the end of Hawking evaporation using covariant loop quantum gravity.

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  • Received 3 August 2021
  • Accepted 5 August 2021

DOI:https://doi.org/10.1103/PhysRevD.104.066015

© 2021 American Physical Society

Physics Subject Headings (PhySH)

  1. Research Areas
Gravitation, Cosmology & Astrophysics

Authors & Affiliations

Farshid Soltani1,2, Carlo Rovelli3,4,5, and Pierre Martin-Dussaud6

  • 1Department of Physics and Astronomy, University of Western Ontario, London, Ontario N6A 3K7, Canada
  • 2Dipartimento di Fisica, Sapienza Università di Roma, P.le Aldo Moro 5, I-00185 Roma, Italy, EU
  • 3AMU Université, Université de Toulon, CNRS, CPT, F-13288 Marseille, France, EU
  • 4Perimeter Institute, 31 Caroline Street N, Waterloo, Ontario N2L2Y5, Canada
  • 5The Rotman Institute of Philosophy, 1151 Richmond Street N, London N6A5B7, Canada
  • 6Institute for Gravitation and the Cosmos, The Pennsylvania State University, University Park, Pennsylvania 16802, USA

See Also

End of a black hole’s evaporation

Fabio D’Ambrosio, Marios Christodoulou, Pierre Martin-Dussaud, Carlo Rovelli, and Farshid Soltani
Phys. Rev. D 103, 106014 (2021)

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Issue

Vol. 104, Iss. 6 — 15 September 2021

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