Neutrino Observatories Can Characterize Cosmic Sources and Neutrino Properties

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dc.creatorBarenboim, Gabriela
dc.creatorQuigg, Chris
dc.date2003-01-24
dc.date.accessioned2026-07-07T13:11:34Z
dc.date.available2026-07-07T13:11:34Z
dc.descriptionNeutrino telescopes that measure relative fluxes of ultrahigh-energy $ν_{e}, ν_μ, ν_τ$ can give information about the location and characteristics of sources, about neutrino mixing, and can test for neutrino instability and for departures from CPT invariance in the neutrino sector. We investigate consequences of neutrino mixing for the neutrino flux arriving at Earth, and consider how terrestrial measurements can characterize distant sources. We contrast mixtures that arise from neutrino oscillations with those signaling neutrino decays. We stress the importance of measuring $ν_{e}, ν_μ, ν_τ$ fluxes in neutrino observatories.
dc.description9 RevTeX pages, 4 figures
dc.identifierhttps://arxiv.org/abs/hep-ph/0301220
dc.identifierhttp://arxiv.org/abs/hep-ph/0301220
dc.identifierPhys.Rev.D67:073024,2003
dc.identifierdoi:10.1103/PhysRevD.67.073024
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/229321
dc.subjectHigh Energy Physics - Phenomenology
dc.subjectAstrophysics
dc.titleNeutrino Observatories Can Characterize Cosmic Sources and Neutrino Properties
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