Neutrino Observatories Can Characterize Cosmic Sources and Neutrino Properties

Details Neutrino Observatories Can Characterize Cosmic Sources and Neutrino Properties Neutrino Observatories Can Characterize Cosmic Sources and Neutrino Properties

2003-01-24

arxiv.org/abs/hep-ph/0301220v1

Phys.Rev.D67:073024,2003

Physics

High Energy Physics

High Energy Physics - Phenomenology

9 RevTeX pages, 4 figures

Scientific paper

10.1103/PhysRevD.67.073024

Neutrino telescopes that measure relative fluxes of ultrahigh-energy $\nu_{e}, \nu_{\mu}, \nu_{\tau}$ can give information about the location and characteristics of sources, about neutrino mixing, and can test for neutrino instability and for departures from CPT invariance in the neutrino sector. We investigate consequences of neutrino mixing for the neutrino flux arriving at Earth, and consider how terrestrial measurements can characterize distant sources. We contrast mixtures that arise from neutrino oscillations with those signaling neutrino decays. We stress the importance of measuring $\nu_{e}, \nu_{\mu}, \nu_{\tau}$ fluxes in neutrino observatories.

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