The End of a Black Hole's Evaporation -- Part I

Carlo Rovelli; Fabio D'Ambrosio; Farshid Soltani; Marios Christodoulou; Pierre Martin-Dussaud

The End of a Black Hole's Evaporation -- Part I

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arxiv 2009.05016 v2 pith:OSNEJ5RL submitted 2020-09-10 gr-qc

Fabio D'Ambrosio , Marios Christodoulou , Pierre Martin-Dussaud , Carlo Rovelli , Farshid Soltani This is my paper · ORCID

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At the end of Hawking evaporation, the horizon of a black hole enters a physical region where quantum gravity cannot be neglected. The physics of this region has not been much explored. We characterise its physics and introduce a technique to study it.

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Analog charged black hole formation via percolation: Exploring cosmic censorship and Hoop conjecture
gr-qc 2025-02 reject novelty 4.0 of 10

A Fock-space percolation model of a chiral spin chain is claimed to reproduce charged-black-hole scaling exponents, with exponential cluster growth proposed as the key formation criterion.

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