Work

Dynamical horizons and black hole soft hair

Year: 2025
Type: article
Abstract: In the present work, quasilocal Brown-York charges are derived that coincide in the large sphere limit with the conserved supertranslation hair and superrotation charges introduced by Hawking, Perry and Strominger in [45, 46]. Given these charges, a general scenario is outlined in which a non-rotating black hole completely evaporates after its collapse due to particle creation effects, whereby a genuine one-way traversable event horizon is never formed, but merely a two-way traversable dynamical (resp. future trapping) horizon. The formation of such a dynamical horizon has the consequence, as is demonstrated, that quasilocal energy transported by the considered charges, and thus information, can continuously escape through the black hole horizon to infinity; a mechanism which, as is argued, could possibly prevent information loss once the black hole formation and evaporation process comes to an end.
Author: Albert Huber
Language: English
Open Access status: hybrid
Estimated APC paid: $3,160
OpenAlex ID: W4417095610
FWCI: 0.473
Cites: 68
Cited by: 1
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