Abstract
Department of Energy and Resources, National United University, Miao-Li 36003, TaiwanE-mail:mahuang@nuu.edu.twWe argue that an effective flavor discrimination in neutrino telescopes is the key to probe theflavor ratios of astrophysical neutrinos at the source and fla vor transition mechanisms of theseneutrinos during their propagations from the source to the Earth. We first discuss how well onecan reconstruct the flavor ratios of astrophysical neutrino s at the source. We then discuss howto probe flavor transition mechanisms of propagating astrop hysical neutrinos. In this regard, wepropose a model independent parametrization for neutrino fl avor transitions, with the neutrinooscillation as a special case.35th International Conference of High Energy Physics - ICHEP2010,July 22-28, 2010Paris France
Sign-in/Register to access full text options 
Free) 
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a call
