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Evaporating black-to-white hole

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arxiv 1905.07251 v2 pith:FNP3WBQV submitted 2019-05-17 gr-qc

Pierre Martin-Dussaud , Carlo Rovelli This is my paper · ORCID
classification gr-qc
keywords holeaccountback-reactionblackblack-to-whitecomponentconstructdiscuss
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We construct and discuss the form of the (effective) spacetime geometry inside a black hole undergoing a quantum transition to a white hole, taking into account the back-reaction of the component of the Hawking radiation falling into the hole.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Testing loop quantum gravity by quasi-periodic oscillations: rotating blackholes

    gr-qc 2024-12 conditional novelty 4.0 of 10

    QPO data from GRO J1655-40 constrain the LQG parameter λ in the BCY rotating black hole metric to 0.15 (equal mass) and 0.11 (unequal mass), both consistent with Kerr.

  2. The Case For Black Hole Remnants: A Review

    gr-qc 2024-11 unverdicted novelty 2.0 of 10

    A review arguing that black hole remnants remain viable and that the species and entropy objections to them are not decisive, so remnants could resolve the information paradox.

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