Hot matter from exploding black holes

Research output: Contribution to journalArticlepeer-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 languageEnglish (US)
Pages (from-to)831-834
Number of pages4
JournalNuclear Physics A
Volume774
Issue number1-4
DOIs
StatePublished - 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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