Conflict between the identification of cosmic neutrino source and the sensitivity to mixing angles in neutrino telescope

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dc.creatorHwang, Ggyoung-Riun
dc.creatorSiyeon, Kim
dc.date2007-11-20
dc.date2008-12-10
dc.date.accessioned2026-07-07T12:48:18Z
dc.date.available2026-07-07T12:48:18Z
dc.descriptionNeutrino fluxes at telescopes depend on both initial fluxes out of astronomical bursts and flavor mixing during their travel to the earth. However, since the information on the initial composition requires better precision in mixing angles and vice versa, the neutrino detection at telescopes for itself cannot provide solutions to the both problems. Thus, a probability to be measured at long baseline oscillation is considered as a complement to the telescope, and problems like source identification and parameter degeneracy are examined under a few assumptions.
dc.description17 pages with 7 figures, published version
dc.identifierhttps://arxiv.org/abs/0711.3122
dc.identifierhttp://arxiv.org/abs/0711.3122
dc.identifierPhys.Rev.D78:093008,2008
dc.identifierdoi:10.1103/PhysRevD.78.093008
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/222007
dc.subjectHigh Energy Physics - Phenomenology
dc.titleConflict between the identification of cosmic neutrino source and the sensitivity to mixing angles in neutrino telescope
dc.typetext

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