Relativistic Viscous Fluid Description of Microscopic Black Hole Wind

Details Relativistic Viscous Fluid Description of Microscopic Black Hole Wind Relativistic Viscous Fluid Description of Microscopic Black Hole Wind

2000-08-15

arxiv.org/abs/astro-ph/0008222v3

Phys.Rev.Lett.86:1670-1673,2001

Astronomy and Astrophysics

Astrophysics

11 pages, revtex

Scientific paper

10.1103/PhysRevLett.86.1670

Microscopic 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.

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