We present a model for high-energy flares in accreting black holes based on the injection in a magnetized corona of a non-thermal population of relativistic particles. Coupled transport equations are solved for all species of particles and the electromagnetic and neutrino output is predicted for the case of Galactic black holes.
Información general
Fecha de publicación:2010
Idioma del documento:Inglés
Revista:Proceedings of the International Astronomical Union; vol. 6, no. S275
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