Cosmic Tau Neutrinos

Simple item page
dc.creatorHusain, Athar
dc.date2000-04-09
dc.date.accessioned2026-07-07T03:41:07Z
dc.date.available2026-07-07T03:41:07Z
dc.descriptionThe collisions between accelerated protons and the photons present in cosmos can be a main source of high-energy neutrinos (E \geq 10^6 GeV) of all flavors above the atmospheric neutrino background. I discuss here the possibility of photohadronic production of high-energy cosmic tau neutrinos in an astrophysical site and study some of the effects of vacuum neutrino flavor mixing on their subsequent propagation. I also discuss the prospects for observations of these high-energy cosmic tau neutrinos in new large neutrino telescopes
dc.description5 pages, Latex, talk given at YITP Workshop on Theoretical Problems related to Neutrino Oscillations, 28 February-01 March, 2000, Kyoto, Japan (to appear in its proceedings)
dc.identifierhttps://arxiv.org/abs/hep-ph/0004083
dc.identifierhttp://arxiv.org/abs/hep-ph/0004083
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/39512
dc.subjectHigh Energy Physics - Phenomenology
dc.subjectAstrophysics
dc.titleCosmic Tau Neutrinos
dc.typetext

Files

Collections

arXiv