Flavor identification of astronomical high energy neutrinos and the accuracy of mixing angles

Details Flavor identification of astronomical high energy neutrinos and the accuracy of mixing angles Flavor identification of astronomical high energy neutrinos and the accuracy of mixing angles

Nov 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aipc.1078..388h&link_type=abstract

SUPERSYMMETRY AND THE UNIFICATION OF FUNDAMENTAL INTERACTIONS. AIP Conference Proceedings, Volume 1078, pp. 388-390 (2008).

Physics

Neutrino Mass And Mixing, Decays Of Muons, Electromagnetic Decays

Scientific paper

Typical initial neutrino fluxes from pion decays may be different depending on energy, since the muon decays can be excluded due to the electromagnetic energy loss. However, the specification of the initial flux ratio is limited by the accuracy of neutrino mixing parameters. We will discuss the expected measurement of relative flavors at future neutrino telescopes, focusing on the ambiguity in current neutrino parameters.

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