A possible connection between gamma-ray bursts and single black holes

G. M. Beskin, A. Shearer, A. Golden, C. Bartolini, A. Guarnieri, A. Piccioni, N. Masetti

Research output: Contribution to journalArticle

1 Scopus citations

Abstract

We consider Single Black Holes (SBHs) of 103 M as possible parent objects for cosmological GRBs. The latter are the result of the energy release of SBHs magnetosphere inhomogeneities. The percolation nature of this release yields a unique power law for the GRBs energy distribution that is E (with β = 1.7-1.8), i.e. the same observed in solar flares, flare stars and X-ray sources. The number of GRBs per year per galaxy is about 10-2-10-1 with total energy 1047-1050 ergs for beaming factor of about 10-4-10-5.

Original languageEnglish (US)
Pages (from-to)509-510
Number of pages2
JournalAstronomy and Astrophysics Supplement Series
Volume138
Issue number3
DOIs
StatePublished - Sep 1999

Keywords

  • Black hole physics
  • Gamma-rays: bursts

ASJC Scopus subject areas

  • Physics and Astronomy(all)

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    Beskin, G. M., Shearer, A., Golden, A., Bartolini, C., Guarnieri, A., Piccioni, A., & Masetti, N. (1999). A possible connection between gamma-ray bursts and single black holes. Astronomy and Astrophysics Supplement Series, 138(3), 509-510. https://doi.org/10.1051/aas:1999329