Relativistic viscous fluid description of microscopic black hole wind

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Abstract

The controversy over whether the particles scatter from each other after being emitted is reviewed. It is shown that a self-consistent description is afforded by the application of relativistic viscous fluid equations, at least towards the end of the black hole's existence and under some assumptions.

Original languageEnglish (US)
Pages (from-to)1670-1673
Number of pages4
JournalPhysical review letters
Volume86
Issue number9
DOIs
StatePublished - Feb 26 2001

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