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Expressions for Neutrino Wave Functions and Transition Probabilities at Three Neutrino Oscillations in Vacuum and Some of Their Applications

Kh. M. Beshtoev
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Abstract

We have considered three neutrino transitions and oscillations in the general case and obtained expressions for neutrino wave functions in three cases: with CP violation, without CP violations and the case when $ν_e \leftrightarrow ν_τ$ transitions are absent (some works indicate on this possibility). Then using the existing experimental data some analysis has been fulfilled. This analysis definitely has shown that transitions $ν_e \leftrightarrow ν_τ$ cannot be closed for the Solar neutrinos. However, this possibility may be realized by using the mechanism of resonance enhancement neutrino oscillations in matter (the Sun). But this possibility is not confirmed by the Solar neutrinos spectrum (the Solar neutrinos spectrum is not distorted) and the Day-Night effect (this effect is not observed). It was found out that the probability of $ν_e \leftrightarrow ν_e$ neutrino transitions is positive defined value only if the angle of $ν_e, ν_τ$ mixing $β\le 15^o ÷17^o$.

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Kh. M. Beshtoev. 2005-08-10. Expressions for Neutrino Wave Functions and Transition Probabilities at Three Neutrino Oscillations in Vacuum and Some of Their Applications. https://arxiv.org/abs/hep-ph/0508122

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