The Emission of Ultra-High Energy Cosmic Rays from Electromagnetic Black Holes

Details The Emission of Ultra-High Energy Cosmic Rays from Electromagnetic Black Holes The Emission of Ultra-High Energy Cosmic Rays from Electromagnetic Black Holes

Feb 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005tmgm.meet.2437c&link_type=abstract

The Tenth Marcel Grossmann Meeting. Proceedings of the MG10 Meeting held at Brazilian Center for Research in Physics (CBPF), Rio

Physics

Scientific paper

It is by now clear that gamma-ray bursts originate from a spherically symmetric collapse of a massive star into a black hole endowed with electromagnetic structure (EMBH). Such theoretical approach has been confirmed to a very high level of accuracy in the explanation of the time variability, of the spectra and in the afterglow of GRBs. Here we consider EMBH as a source of UHECRs. It will be shown that such senario is coherent with the expected UHECRs flux, the observed events at 1020 eV and we will developp new idea about the origin doublet and triplet events.

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