Neutrino Flavor Ratio on Earth and at Astrophysical Sources

Details Neutrino Flavor Ratio on Earth and at Astrophysical Sources Neutrino Flavor Ratio on Earth and at Astrophysical Sources

2010-04-07

arxiv.org/abs/1004.1030v1

Progress in Particle and Nuclear Physics, 64 (2010), pp. 420-422

Physics

High Energy Physics

High Energy Physics - Phenomenology

3 pages, 8 figures. Talk presented by T.C. Liu in ERICE 2009, Sicily.

Scientific paper

10.1016/j.ppnp.2009.12.064

We present the reconstruction of neutrino flavor ratios at astrophysical sources. For distinguishing the pion source and the muon-damped source to the 3$\sigma$ level, the neutrino flux ratios, $R\equiv\phi(\nu_\mu)/(\phi(\nu_e)+\phi(\nu_\tau))$ and $S\equiv\phi(\nu_e)/\phi(\nu_\tau)$, need to be measured in accuracies better than 10%.

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