Tau Neutrinos at EeV Energies

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dc.creatorDutta, S. Iyer
dc.creatorMocioiu, I.
dc.creatorReno, M. H.
dc.creatorSarcevic, I.
dc.date2003-07-16
dc.date.accessioned2026-07-07T03:50:06Z
dc.date.available2026-07-07T03:50:06Z
dc.descriptionAstrophysical sources of ultrahigh energy neutrinos yield tau neutrino fluxes due to neutrino oscillations. At neutrino energies in the EeV range, radio Cherenkov detection methods show promise for detecting these fluxes. We quantify the tau neutrino contributions to the signal in, for example, a detector like the Radio Ice Cherenkov Experiment (RICE) for a Z-burst flux prediction. Tau neutrino regeneration in transit through the Earth, including energy loss, is evaluated.
dc.description4 pages, submitted to 28th International Cosmic Ray Conference, July 31-August 7, 2003, Tsukuba, Japan
dc.identifierhttps://arxiv.org/abs/hep-ph/0307210
dc.identifierhttp://arxiv.org/abs/hep-ph/0307210
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/42656
dc.subjectHigh Energy Physics - Phenomenology
dc.titleTau Neutrinos at EeV Energies
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