Relativistic Viscous Fluid Description of Microscopic Black Hole Wind

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dc.creatorKapusta, J. I.
dc.date2000-08-15
dc.date2001-05-25
dc.date.accessioned2026-07-07T12:00:43Z
dc.date.available2026-07-07T12:00:43Z
dc.descriptionMicroscopic black holes explode with their temperature varying inversely as their mass. Such explosions would lead to the highest temperatures in the present universe, all the way to the Planck energy. Whether or not a quasi-stationary shell of matter undergoing radial hydrodynamic expansion surrounds such black holes is been controversial. In this paper relativistic viscous fluid equations are applied to the problem. It is shown that a self-consistent picture emerges of a fluid just marginally kept in local thermal equilibrium; viscosity is a crucial element of the dynamics.
dc.description11 pages, revtex
dc.identifierhttps://arxiv.org/abs/astro-ph/0008222
dc.identifierhttp://arxiv.org/abs/astro-ph/0008222
dc.identifierPhys.Rev.Lett.86:1670-1673,2001
dc.identifierdoi:10.1103/PhysRevLett.86.1670
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/206879
dc.subjectAstrophysics
dc.titleRelativistic Viscous Fluid Description of Microscopic Black Hole Wind
dc.typetext

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