Hot matter from exploding black holes

J. I. Kapusta

doi:10.1016/j.nuclphysa.2006.06.146

Hot matter from exploding black holes

J. I. Kapusta

Physics and Astronomy (Twin Cities)

Research output: Contribution to journal › Article › peer-review

Abstract

The relativistic viscous fluid equations describing the outflow of high temperature matter created via Hawking radiation from microscopic black holes are solved numerically for a realistic equation of state. We focus on black holes with initial temperatures greater than 100 GeV and lifetimes less than 6 days. The spectra of photons and neutrinos are calculated for energies greater than 1 GeV. The most promising route for the observation of these black holes is to search for point sources emitting gamma rays or neutrinos of ever-increasing energy.

Original language	English (US)
Pages (from-to)	831-834
Number of pages	4
Journal	Nuclear Physics A
Volume	774
Issue number	1-4
DOIs	https://doi.org/10.1016/j.nuclphysa.2006.06.146
State	Published - Aug 7 2006

Bibliographical note

Funding Information:
∗This work was supported by the US Department of Energy under grant DE-FG02-87ER40328.

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Hot matter from exploding black holes

Abstract

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