Probing neutrino mixing angles with ultrahigh energy neutrino telescopes

Details Probing neutrino mixing angles with ultrahigh energy neutrino telescopes Probing neutrino mixing angles with ultrahigh energy neutrino telescopes

2005-01-20

arxiv.org/abs/hep-ph/0501191v2

Physics

High Energy Physics

High Energy Physics - Phenomenology

Replaced with revised version. Crucial change in the title (word "running" dropped). Abstract and content changed. Motivationa

Scientific paper

We point out that detecting $\nuebar$'s from distant astrophysical sources with the up-coming and future neutrino telescopes using the Glashow resonance channel $\nuebar e^{-}\to W^{-} \to$ anything, which occurs over a small energy window around the $\nuebar$ energy of $\sim6.3\pev$, offers a new way of measuring or setting limits on neutrino mixing angles, in particular the angle $\theta_{12}$, thereby providing an independent experimental probe of neutrino mixing angles. We also discuss how this exercise may throw light on the nature of the neutrino production mechanism in individual astrophysical sources.

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