Non-adiabatic resonant conversion of solar neutrinos in three generations

C. W. Kim; S. Nussinov; W. K. Sze

doi:10.1016/0370-2693(87)90188-2

Non-adiabatic resonant conversion of solar neutrinos in three generations

C. W. Kim, S. Nussinov, W. K. Sze

Department of Physics

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35 Citations (Scopus)

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	https://doi.org/10.1016/0370-2693(87)90188-2
Publication status	Published - 1987 Feb 5

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ASJC Scopus subject areas

Nuclear and High Energy Physics

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

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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.

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10.1016/0370-2693(87)90188-2