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- W2415817070 abstract "Our knowledge of the high-energy universe is undergoing a period of rapid change as new astronomical detectors of high-energy radiation start to operate at their design sensitivities. Now is a boomtime for high-energy as- trophysics, with new discoveries from Swift and HESS, re- sults from MAGIC and VERITAS starting to be reported, the upcoming launches of the γ -ray space telescopes GLAST and AGILE, and anticipated data releases from IceCube and Auger. A formalism for calculating statistical properties of cos- mological γ -ray sources is presented. Application is made to model calculations of the statistical distributions of γ -ray and neutrino emission from (i) beamed sources, specifi- cally, long-duration GRBs, blazars, and extragalactic mi- croquasars, and (ii) unbeamed sources, including normal galaxies, starburst galaxies and clusters. Expressions for the integrated intensities of faint beamed and unbeamed high- energy radiation sources are also derived. A toy model for the background intensity of radiation from dark-matter an- nihilation taking place in the early universe is constructed. Estimates for the γ -ray fluxes of local group galaxies, star- burst, and infrared luminous galaxies are briefly reviewed. Because the brightest extragalactic γ -ray sources are flaring sources, and these are the best targets for sources of PeV-EeV neutrinos and ultra-high energy cosmic rays, rapidly slewing all-sky telescopes like MAGIC and an all- sky γ -ray observatory beyond Milagro will be crucial for optimal science return in the multi-messenger age." @default.
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- W2415817070 date "2007-01-01" @default.
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- W2415817070 title "γ Rays and neutrinos from beyond the galaxy" @default.
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