Neutrino Flavor Goniometry by High Energy Astrophysical Beams

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dc.creatorPakvasa, Sandip
dc.date2008-03-12
dc.date2008-05-17
dc.date.accessioned2026-07-07T11:49:02Z
dc.date.available2026-07-07T11:49:02Z
dc.descriptionIt is shown how high energy neutrino beams from very distant sources can be utilized to learn about many properties of neutrinos such as lifetimes, mass hierarchy, mixing, minuscule pseudo-Dirac mass splittings; in addition, the production mechanism of neutrinos in astrophysical sources can also be elucidated.
dc.description22 pages. Presented at the COSPA 2007, Taipei, November 2007; to be published in the proceedings. Added references
dc.identifierhttps://arxiv.org/abs/0803.1701
dc.identifierhttp://arxiv.org/abs/0803.1701
dc.identifierMod.Phys.Lett.A23:1313-1324,2008
dc.identifierdoi:10.1142/S0217732308027680
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/203096
dc.subjectHigh Energy Physics - Phenomenology
dc.subjectAstrophysics
dc.subjectHigh Energy Physics - Experiment
dc.titleNeutrino Flavor Goniometry by High Energy Astrophysical Beams
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