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.

arXiv comment22 pages. Presented at the COSPA 2007, Taipei, November 2007; to be published in the proceedings. Added references

References in corpus (27)

• Phenomenology with Massive Neutrinos
• Detecting Nutau Oscillations as PeV Energies
• Detecting Tau Neutrino Oscillations at PeV Energies
• Neutrinos from propagation of ultra-high energy protons
• Flavor Composition and Energy Spectrum of Astrophysical Neutrinos
• Neutrino Oscillations as a Probe of Dark Energy
• Do solar neutrinos decay?
• A High Sensitivity Search for ${\bar{\nu }}_e$'s from the Sun and Other Sources at KamLAND
• CPT-odd Resonances in Neutrino Oscillations
• Galactic Point Sources of TeV Antineutrinos
• CMB Signals of Neutrino Mass Generation
• Neutrino Observatories Can Characterize Cosmic Sources and Neutrino Properties
• Sensitivity to ${\theta }_{13}$ and $\delta$ in the Decaying Astrophysical Neutrino Scenario
• Neutrinos as a Diagnostic of High Energy Astrophysical Processes
• Probing Quantum Decoherence with High-Energy Neutrinos
• Testing neutrino flavor mixing plus decay with neutrino telescopes
• Measuring the 13-mixing angle and the CP phase with neutrino telescopes
• Pseudo-Dirac Scenario for Neutrino Oscillations
• High Energy Cosmic Neutrinos and the Equivalence Principle
• 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
• Testing neutrino magnetic moments with AGNs
• Testing neutrino instability with active galactic nuclei
• Neutrino Flavor Conversion in Random Magnetic Fields
• On the measurement of B(E2, 0+ -> 2+) using intermediate-energy Coulomb excitation

Cited by in corpus (24)

• Cosmogenic Neutrinos: parameter space and detectabilty from PeV to ZeV
• Cosmic Neutrino Pevatrons: A Brand New Pathway to Astronomy, Astrophysics, and Particle Physics
• Simplified models for photohadronic interactions in cosmic accelerators
• Neutrino Decays over Cosmological Distances and the Implications for Neutrino Telescopes
• Energy dependent neutrino flavor ratios from cosmic accelerators on the Hillas plot
• The Glashow resonance at IceCube: signatures, event rates and $pp$ vs. $p\gamma$ interactions
• Inferring the flavor of high-energy astrophysical neutrinos at their sources
• Testing neutrino flavor mixing plus decay with neutrino telescopes
• Systematics in the Interpretation of Aggregated Neutrino Flux Limits and Flavor Ratios from Gamma-Ray Bursts
• Implications of Leptonic Unitarity Violation at Neutrino Telescopes
• Flavor Composition of UHE Neutrinos at Source and at Neutrino Telescopes
• An Analysis of Cosmic Neutrinos: Flavor Composition at Source and Neutrino Mixing Parameters
• Universe's Worth of Electrons to Probe Long-Range Interactions of High-Energy Astrophysical Neutrinos
• Interplay of energy dependent astrophysical neutrino flavor ratios and new physics effects
• Galactic Neutrino Communication
• Theoretical Overview of Neutrino Properties
• Using High-Energy Neutrinos As Cosmic Magnetometers
• Testing the Bimodal/Schizophrenic Neutrino Hypothesis in Neutrinoless Double Beta Decay and Neutrino Telescopes
• Feasibility of Determining Diffuse Ultra-High Energy Cosmic Neutrino Flavor Ratio through ARA Neutrino Observatory
• Constraints on the Ultra-High Energy Neutrino Flux from Gamma-Ray Bursts from a Prototype Station of the Askaryan Radio Array
• Interaction of Dirac and Majorana Neutrinos with Weak Gravitational Fields
• Lectures on neutrino phenomenology
• On the possibility of neutrino flavor identification at the highest energies
• Neutrinos from Cosmic Accelerators Including Magnetic Field and Flavor Effects