Abstract
The survival probability of solar electron neutrinos after non-adiabatic passage through the resonance-oscillation region in the Sun is discussed for the case of three generations. A method to calculate three-generation Landau-Zener transition probabilities between adiabatic states is described. We also discuss how the Landua-Zener probability is modified in the extreme non-adiabatic case.
Original language | English |
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Pages (from-to) | 403-409 |
Number of pages | 7 |
Journal | Physics Letters B |
Volume | 184 |
Issue number | 4 |
DOIs | |
Publication status | Published - 1987 Feb 5 |
Externally published | Yes |
ASJC Scopus subject areas
- Nuclear and High Energy Physics