High Energy Radiation from Black Holes in Gamma Ray Bursts

Details High Energy Radiation from Black Holes in Gamma Ray Bursts High Energy Radiation from Black Holes in Gamma Ray Bursts

Feb 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aps..aprk13001d&link_type=abstract

American Physical Society, APS April Meeting 2010, February 13-16, 2010, abstract #K13.001

Physics

Scientific paper

Gamma ray bursts are sources of broadband radio-through-gamma radiation that are thought to occur during the formation of black holes from stellar core collapse or compact-object coalescence. Particles accelerated in the shock waves of relativistic plasma ejected from GRB sources make cosmic rays, gamma rays and neutrinos. Signatures of ultra-high energy cosmic rays in GRBs should reveal characteristic hadronic emissions. In this talk, contrasting leptonic and hadronic emission signatures in the electromagnetic spectrum of GRBs are considered as a probe of particle acceleration in GRBs. )

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