Cosmic Neutrinos

dc.creatorQuigg, Chris
dc.date2008-01-31
dc.date2008-02-08
dc.date.accessioned2026-07-07T09:19:12Z
dc.date.available2026-07-07T09:19:12Z
dc.descriptionI recall the place of neutrinos in the electroweak theory and summarize what we know about neutrino mass and flavor change. I next review the essential characteristics expected for relic neutrinos and survey what we can say about the neutrino contribution to the dark matter of the Universe. Then I discuss the standard-model interactions of ultrahigh-energy neutrinos, paying attention to the consequences of neutrino oscillations, and illustrate a few topics of interest to neutrino observatories. I conclude with short comments on the remote possibility of detecting relic neutrinos through annihilations of ultrahigh-energy neutrinos at the $Z$ resonance.
dc.description27 pages, 16 figures, uses RevTeX, lecture at 2007 SLAC Summer Institute; added references, footnote clarified
dc.identifierhttps://arxiv.org/abs/0802.0013
dc.identifierhttp://arxiv.org/abs/0802.0013
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/154303
dc.subjectHigh Energy Physics - Phenomenology
dc.subjectAstrophysics
dc.titleCosmic Neutrinos
dc.typetext

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