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Cosmic Neutrino Pevatrons: A Brand New Pathway to Astronomy, Astrophysics, and Particle Physics

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arxiv 1312.6587 v3 pith:Z6ARHDDL submitted 2013-12-23 astro-ph.HE hep-exhep-ph

Cosmic Neutrino Pevatrons: A Brand New Pathway to Astronomy, Astrophysics, and Particle Physics

Luis A. Anchordoqui , Vernon Barger , Ilias Cholis , Haim Goldberg , Dan Hooper , Alexander Kusenko , John G. Learned , Danny Marfatia
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Sandip Pakvasa Thomas C. Paul Thomas J. Weiler
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classification astro-ph.HE hep-exhep-ph
keywords neutrinobeencosmicdataeithericecubephysicsquestion
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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The announcement by the IceCube Collaboration of the observation of 28 cosmic neutrino candidates has been greeted with a great deal of justified excitement. The data reported so far depart by 4.3\sigma from the expected atmospheric neutrino background, which raises the obvious question: "Where in the Cosmos are these neutrinos coming from?" We review the many possibilities which have been explored in the literature to address this question, including origins at either Galactic or extragalactic celestial objects. For completeness, we also briefly discuss new physics processes which may either explain or be constrained by IceCube data.

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    High-energy astrophysical neutrinos enable stringent tests of physics beyond the Standard Model at energies and baselines unreachable by other means.