Neutrinos from WIMP annihilations in the Sun including neutrino oscillations

First, for the propagation to the Earth, vacuum neutrino oscillations to the Earth are included in the same three-flavor neutrino setup. In addition, effects of the eccentricity of

For non-zero θ 13 , we have found that the adiabatic flavor transitions at the high MSW resonance results in the electron neutrinos mixing with the muon and tau neutrinos already

We also discuss the equivalence of using a Monte Carlo approach - suited for inclusion in neutrino telescope Monte Carlos - and the density matrix formalism.. Identification of

In the context of the MUED model, the spin-independent cross section for KK neutrinos scattering on protons [39] is larger than the limits set by direct detection experiments,

As was discussed earlier, at high neutrino energies, the muon neutrino will oscillate in a pure two- flavor vacuum scenario with the effective parameters given by Eqs.. In the case of

In this Letter, we study the matter effects on neutrino mixing and oscilla- tions in the limit where the matter density becomes infinite and the resulting neutrino

However, if the values of the parameters θ 12 , ∆m 2 , and A n−d were known with a larger accuracy, then the change due to non-zero θ 13 could, in principle, be used to determine

We find how the precision measurement of neutrino oscillation parameters can be altered by non-standard effects alone (not including non- standard interactions in the creation