Relativistic phase transitions in the radiation flow of primordial black holes and high-energy gamma bursts

Details Relativistic phase transitions in the radiation flow of primordial black holes and high-energy gamma bursts Relativistic phase transitions in the radiation flow of primordial black holes and high-energy gamma bursts

Jun 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004aspc..312..453l&link_type=abstract

Third Rome Workshop on Gamma-Ray Bursts in the Afterglow Era ASP Conference Series, Volume 312, Proceedings of the conference he

Astronomy and Astrophysics

Astronomy

4

Scientific paper

It is shown that during PBH evolution a quasistatic configuration "PBH + restructured vacuum" is formed as a result of relativistic phase transitions in the radiation flow of the PBH. Explosion of such a configuration at the final stage of evolution of the PBH leads to formation of the supershort burst of gamma radiation with the spectrum having maximums of intensity at 100 MeV and 100 GeV, which agree with the scale of the relativistic phase transitions in the Standard Model of the elementary particles.

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