Flavor Transition Mechanisms of Propagating Astrophysical Neutrinos -A Model Independent Parametrization

Details Flavor Transition Mechanisms of Propagating Astrophysical Neutrinos -A Model Independent Parametrization Flavor Transition Mechanisms of Propagating Astrophysical Neutrinos -A Model Independent Parametrization

2010-04-09

arxiv.org/abs/1004.1583v3

Phys.Rev.D82:103003,2010

Physics

High Energy Physics

High Energy Physics - Phenomenology

Matches the published version

Scientific paper

10.1103/PhysRevD.82.103003

One of the important goals for future neutrino telescopes is to identify the flavors of astrophysical neutrinos and therefore determine the flavor ratio. The flavor ratio of astrophysical neutrinos observed on the Earth depends on both the initial flavor ratio at the source and flavor transitions taking place during propagations of these neutrinos. We propose a model independent parametrization for describing the above flavor transitions. A few flavor transition models are employed to test our parametrization. The observational test for flavor transition mechanisms through our parametrization is discussed.

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