Probing Pseudo-Dirac Neutrino through Detection of Neutrino Induced Muons from GRB Neutrinos

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dc.creatorMajumdar, Debasish
dc.date2006-07-31
dc.date.accessioned2026-07-07T11:58:50Z
dc.date.available2026-07-07T11:58:50Z
dc.descriptionThe possibility to verify the pseudo-Dirac nature of neutrinos is investigated here via the detection of ultra high energy neutrinos from distant cosmological objects like GRBs. The very long baseline and the energy range from $\sim$ TeV to $\sim$ EeV for such neutrinos invokes the likelihood to probe very small pseude-Dirac splittings. The expected secondary muons from such neutrinos that can be detected by a kilometer scale detector such as ICECUBE is calculated. The pseudo-Dirac nature, if exists, will show a considerable departure from flavour oscillation scenario in the total yield of the secondary muons induced by such neutrinos.
dc.description11 pages, 3figures
dc.identifierhttps://arxiv.org/abs/hep-ph/0607344
dc.identifierhttp://arxiv.org/abs/hep-ph/0607344
dc.identifierPramana70:51-60,2008
dc.identifierdoi:10.1007/s12043-008-0004-5
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/206357
dc.subjectHigh Energy Physics - Phenomenology
dc.titleProbing Pseudo-Dirac Neutrino through Detection of Neutrino Induced Muons from GRB Neutrinos
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