High-Energy Neutrinos from Extragalactic Cosmic-Ray Sources

Details High-Energy Neutrinos from Extragalactic Cosmic-Ray Sources High-Energy Neutrinos from Extragalactic Cosmic-Ray Sources

Aug 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011nuphs.217..291m&link_type=abstract

Nuclear Physics B Proceedings Supplements, Volume 217, Issue 1, p. 291-293.

Physics

Nuclear Physics

Scientific paper

High-energy neutrinos, which can uniquely identify the production of hadronic cosmic rays and especially probe dense sources, are detectable by the nearly-completed IceCube and the planned KM3Net. We discuss high-energy neutrino emission from powerful extragalactic cosmic-ray accelerators such as active galaxies, gamma-ray bursts, clusters of galaxies and magnetars. We take a view of future prospects for those potential neutrino sources.

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