Neutrino Flavor Goniometry by High Energy Astrophysical Beams

Abstract

It is shown how high energy neutrino beams from very distant sources can be utilized to learn about many properties of neutrinos such as lifetimes, mass hierarchy, mixing, minuscule pseudo-Dirac mass splittings; in addition, the production mechanism of neutrinos in astrophysical sources can also be elucidated.

22 pages. Presented at the COSPA 2007, Taipei, November 2007; to be published in the proceedings. Added references

References in corpus (7)

• Phenomenology with Massive Neutrinos
• Flavor Composition and Energy Spectrum of Astrophysical Neutrinos
• Testing neutrino flavor mixing plus decay with neutrino telescopes
• Confusing Sterile Neutrinos with Deviation from Tribimaximal Mixing at Neutrino Telescopes
• On Probing theta_{23} in Neutrino Telescopes
• Search for Matter-Dependent Atmospheric Neutrino Oscillations in Super-Kamiokande
• Probing CP violation in neutrino oscillations with neutrino telescopes

Cited by in corpus (12)

• Cosmogenic Neutrinos: parameter space and detectabilty from PeV to ZeV
• Neutrino Decays over Cosmological Distances and the Implications for Neutrino Telescopes
• Energy dependent neutrino flavor ratios from cosmic accelerators on the Hillas plot
• Testing neutrino flavor mixing plus decay with neutrino telescopes
• Inferring the flavor of high-energy astrophysical neutrinos at their sources
• Implications of Leptonic Unitarity Violation at Neutrino Telescopes
• An Analysis of Cosmic Neutrinos: Flavor Composition at Source and Neutrino Mixing Parameters
• Galactic Neutrino Communication
• Theoretical Overview of Neutrino Properties
• Testing the Bimodal/Schizophrenic Neutrino Hypothesis in Neutrinoless Double Beta Decay and Neutrino Telescopes
• Interaction of Dirac and Majorana Neutrinos with Weak Gravitational Fields
• Lectures on neutrino phenomenology