Leptonic CP violation at neutrino telescopes
arXiv:1206.6886 · doi:10.1103/PhysRevD.86.067701
Abstract
With the advent of the recent measurements in neutrino physics, we investigate the role of high-energy neutrino flux ratios at neutrino telescopes for the possibility of determining the leptonic CP-violating phase δand the underlying pattern of the leptonic mixing matrix. We find that the flux ratios show a dependence of O(10 %) on the CP-violating phase, and for optimistic uncertainties on the flux ratios less than 10 %, they can be used to distinguish between CP-conserving and CP-violating values of the phase at 2σin a non-vanishing interval around the maximal value |δ|=π/2.
10 pages, 5 figures. Final version published in Phys. Rev. D
References in corpus (16)
- Observation of electron-antineutrino disappearance at Daya Bay
- Indication of Electron Neutrino Appearance from an Accelerator-produced Off-axis Muon Neutrino Beam
- Global status of neutrino oscillation parameters after Neutrino-2012
- Flavor Composition and Energy Spectrum of Astrophysical Neutrinos
- Flavor Ratios of Astrophysical Neutrinos: Implications for Precision Measurements
- Testing neutrino flavor mixing plus decay with neutrino telescopes
- How astrophysical neutrino sources could be used for early measurements of neutrino mass hierarchy and leptonic CP phase
- Implications of Leptonic Unitarity Violation at Neutrino Telescopes
- An Analysis of Cosmic Neutrinos: Flavor Composition at Source and Neutrino Mixing Parameters
- Neutrino flux ratios at neutrino telescopes: The role of uncertainties of neutrino mixing parameters and applications to neutrino decay
- Neutrino Telescopes as a Probe of Broken - Symmetry
- Probing deviations from tri-bimaximal mixing through ultra high energy neutrino signals
- Confusing Sterile Neutrinos with Deviation from Tribimaximal Mixing at Neutrino Telescopes
- On Probing theta_{23} in Neutrino Telescopes
- Probing CP violation in neutrino oscillations with neutrino telescopes
- Conflict between the identification of cosmic neutrino source and the sensitivity to mixing angles in neutrino telescope