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 |
|---|---|
| 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 |
ASJC Scopus subject areas
- Nuclear and High Energy Physics
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Cite this
Kim, C. W., Nussinov, S., & Sze, W. K. (1987). Non-adiabatic resonant conversion of solar neutrinos in three generations. Physics Letters B, 184(4), 403-409. https://doi.org/10.1016/0370-2693(87)90188-2