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dc.contributor.authorLai, Kwang-Changen_US
dc.contributor.authorLin, Guey-Linen_US
dc.contributor.authorLiu, T. C.en_US
dc.date.accessioned2018-08-21T05:56:33Z-
dc.date.available2018-08-21T05:56:33Z-
dc.date.issued2012-01-01en_US
dc.identifier.issn1742-6588en_US
dc.identifier.urihttp://dx.doi.org/10.1088/1742-6596/375/5/052040en_US
dc.identifier.urihttp://hdl.handle.net/11536/146332-
dc.description.abstractThe future neutrino telescopes are expected to identify the flavors of astrophysical neutrinos and therefore determine the flavor ratio. The flavor ratio of astrophysical neutrinos observed at the Earth depends on both the initial flavor ratio at the source and flavor transitions taking place during the propagations of these neutrinos. We propose a model-independent way to parameterize the above flavor transitions, including standard oscillations and beyond. A systematical way is also described to probe those mechanisms taking advantage of R equivalent to phi(mu)/(phi(e) + phi(tau)) and S equivalent to phi(e)/phi(tau) the observables in neutrino telescope measurements.en_US
dc.language.isoen_USen_US
dc.titleClassifying and probing flavor transition mechanisms of astrophysical high energy neutrinosen_US
dc.typeProceedings Paperen_US
dc.identifier.doi10.1088/1742-6596/375/5/052040en_US
dc.identifier.journal12TH INTERNATIONAL CONFERENCE ON TOPICS IN ASTROPARTICLE AND UNDERGROUND PHYSICS (TAUP 2011), PTS 1-6en_US
dc.citation.volume375en_US
dc.contributor.department物理研究所zh_TW
dc.contributor.departmentInstitute of Physicsen_US
dc.identifier.wosnumberWOS:000307776500179en_US
Appears in Collections:Conferences Paper