Probing neutrino oscillations from supernovae shock waves via the IceCube detector

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dc.creatorChoubey, Sandhya
dc.creatorHarries, N. P.
dc.creatorRoss, G. G.
dc.date2006-05-24
dc.date2006-09-27
dc.date.accessioned2026-07-07T11:26:57Z
dc.date.available2026-07-07T11:26:57Z
dc.descriptionThe time dependent neutrino oscillation signals due to the passage of a shock wave through the supernovae are analyzed for the case of three active neutrinos and also for the case that there are two additional sterile neutrinos. It is shown that, even without flavour identification and energy measurement, detailed information about the masses and mixing angles of the neutrinos may be obtained with a detector with excellent time resolution such as IceCube. Such a signal would also give important information about the nature of the shock wave within the supernovae.
dc.description30 pages, 15 figures, Version to appear in PRD
dc.identifierhttps://arxiv.org/abs/hep-ph/0605255
dc.identifierhttp://arxiv.org/abs/hep-ph/0605255
dc.identifierPhys.Rev.D74:053010,2006
dc.identifierdoi:10.1103/PhysRevD.74.053010
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/196000
dc.subjectHigh Energy Physics - Phenomenology
dc.subjectAstrophysics
dc.subjectHigh Energy Physics - Experiment
dc.subjectInstrumentation and Detectors
dc.titleProbing neutrino oscillations from supernovae shock waves via the IceCube detector
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