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dc.contributor.authorLiu, T. C.en_US
dc.contributor.authorLai, Kwang-Changen_US
dc.contributor.authorLin, Guey-Linen_US
dc.date.accessioned2014-12-08T15:30:26Z-
dc.date.available2014-12-08T15:30:26Z-
dc.date.issued2013-01-20en_US
dc.identifier.issn0217-7323en_US
dc.identifier.urihttp://dx.doi.org/10.1142/S0217732313400051en_US
dc.identifier.urihttp://hdl.handle.net/11536/21763-
dc.description.abstractDue to flavor transition mechanisms in neutrino propagations, both neutrino oscillation and decay, neutrinos flavor ratio at astrophysical sources can quite different from observed ratios on the Earth.(1) We use the recent global fitting result of the mixing angle values(2) to determine the allowed neutrino flavor ratios on the Earth for standard neutrino oscillation and general decay mechanisms. In this analysis, four types of the neutrino decay mechanisms can be distinguished from the oscillation case easily with arbitrary initial neutrino flavor ratio and the other four types of neutrino decay mechanisms can be distinguished from the oscillation case with the specified source. The rest types of neutrino decays strongly overlap with the oscillation and cannot be identified.en_US
dc.language.isoen_USen_US
dc.subjectNeutrinoen_US
dc.subjectmixing angleen_US
dc.titleNEUTRINO FLAVOR RATIOS ON THE EARTH FOR DECAY AND OSCILLATION SCENARIOSen_US
dc.typeArticleen_US
dc.identifier.doi10.1142/S0217732313400051en_US
dc.identifier.journalMODERN PHYSICS LETTERS Aen_US
dc.citation.volume28en_US
dc.citation.issue2en_US
dc.citation.epageen_US
dc.contributor.department物理研究所zh_TW
dc.contributor.departmentInstitute of Physicsen_US
dc.identifier.wosnumberWOS:000316900100005-
dc.citation.woscount0-
Appears in Collections:Articles