TY - JOUR
T1 - Non-adiabatic resonant conversion of solar neutrinos in three generations
AU - Kim, C. W.
AU - Nussinov, S.
AU - Sze, W. K.
N1 - Funding Information:
The authors would like to thank L. Madansky, M. Suskin and D. Wurmser for discussions. One of us (S.N.) wishes to thank the Department of Physics and Astronomy, the Johns Hopkins University for its hospitality. This work was supported in part by the National Science Foundation (C.W.K. and W.K.S.) and the U.S. Department of Energy Grant No. DE-FG02-85 ER40211 (S.N.).
PY - 1987/2/5
Y1 - 1987/2/5
N2 - 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.
AB - 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.
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U2 - 10.1016/0370-2693(87)90188-2
DO - 10.1016/0370-2693(87)90188-2
M3 - Article
AN - SCOPUS:0000924495
VL - 184
SP - 403
EP - 409
JO - Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics
JF - Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics
SN - 0370-2693
IS - 4
ER -