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dc.contributor.authorLin, Guey-Linen_US
dc.contributor.authorLiu, T. C.en_US
dc.contributor.authorLai, Kwang-Changen_US
dc.contributor.authorHuang, M. A.en_US
dc.date.accessioned2017-04-21T06:49:53Z-
dc.date.available2017-04-21T06:49:53Z-
dc.date.issued2010en_US
dc.identifier.urihttp://hdl.handle.net/11536/134867-
dc.description.abstractWe argue that an effective flavor discrimination in neutrino telescopes is the key to probe the flavor ratios of astrophysical neutrinos at the source and flavor transition mechanisms of these neutrinos during their propagations from the source to the Earth. We first discuss how well one can reconstruct the flavor ratios of astrophysical neutrinos at the source. We then discuss how to probe flavor transition mechanisms of propagating astrophysical neutrinos. In this regard, we propose a model independent parametrization for neutrino flavor transitions, with the neutrino oscillation as a special case.en_US
dc.language.isoen_USen_US
dc.titleDeterminations of flavor ratios and flavor transitions of astrophysical neutrinosen_US
dc.typeProceedings Paperen_US
dc.identifier.journal35TH INTERNATIONAL CONFERENCE OF HIGH ENERGY PHYSICS (ICHEP 2010)en_US
dc.contributor.department物理研究所zh_TW
dc.contributor.departmentInstitute of Physicsen_US
dc.identifier.wosnumberWOS:000392111500387en_US
dc.citation.woscount0en_US
Appears in Collections:Conferences Paper