1996/07/31 by R. J. Protheroe, Protheroe, R. J.
Physics and Astronomy · #Astrophysics (astro-ph) #FOS: Physical sciences #astro-ph
paper · pdf · doi:10.48550/arxiv.astro-ph/9607165
4 pages, 2 figures, to appear in Accretion Phenomena and Related Outflows, IAU Colloq. 163, ed. D. Wickramashinghe et al., 1996
arxiv created 1996/07/31 · arxiv updated 2009/12/01
I describe a model of energetic gamma ray and neutrino emission in blazars which is consistent with most of the gamma-ray observations, and use this model to estimate the diffuse intensity of high energy neutrinos from blazars.