High energy astrophysical neutrino flux and modified dispersion relations

TY - JOUR

T1 - High energy astrophysical neutrino flux and modified dispersion relations

AU - Alba, J. L. Bazo

AU - Bustamante, M.

AU - Gago, A. M.

AU - Miranda, O. G.

N1 - Accepted for publication in the Int. J. Mod. Phys. A -- Typo in online version of abstract corrected

PY - 2009/7/11

Y1 - 2009/7/11

N2 - Motivated by the interest in searches for violation of CPT invariance, we study its possible effects in the flavour ratios of high-energy neutrinos coming from cosmic accelerators. In particular, we focus on the effect of an energy independent new physics contribution to the neutrino flavour oscillation phase and explore whether it is observable in future detectors. Such a contribution could be related not only to CPT violation but also to a nonuniversal coupling of neutrinos to a torsion field. We conclude that this extra phase contribution only becomes observable, in the best case, at energies greater than 10^{16.5} GeV, which is about five orders of magnitude higher than the most energetic cosmological neutrinos to be detected in the near future. Therefore, if these effects are present only in the oscillation phase, they are going to be unobservable, unless a new mechanism or source capable to produce neutrinos of such energy were detected.

AB - Motivated by the interest in searches for violation of CPT invariance, we study its possible effects in the flavour ratios of high-energy neutrinos coming from cosmic accelerators. In particular, we focus on the effect of an energy independent new physics contribution to the neutrino flavour oscillation phase and explore whether it is observable in future detectors. Such a contribution could be related not only to CPT violation but also to a nonuniversal coupling of neutrinos to a torsion field. We conclude that this extra phase contribution only becomes observable, in the best case, at energies greater than 10^{16.5} GeV, which is about five orders of magnitude higher than the most energetic cosmological neutrinos to be detected in the near future. Therefore, if these effects are present only in the oscillation phase, they are going to be unobservable, unless a new mechanism or source capable to produce neutrinos of such energy were detected.

KW - hep-ph

U2 - 10.1142/S0217751X09047429

DO - 10.1142/S0217751X09047429

M3 - Journal article

SN - 0217-751X

VL - 24

JO - International Journal of Modern Physics A

JF - International Journal of Modern Physics A

IS - 31

M1 - 5819

ER -