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

^*Corresponding author for this work

Research output: Contribution to journal › Article › peer-review

34 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
Externally published	Yes

ASJC Scopus subject areas

Nuclear and High Energy Physics

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10.1016/0370-2693(87)90188-2

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@article{cbc0cea6b44b4791904405cbc3d87761,

title = "Non-adiabatic resonant conversion of solar neutrinos in three generations",

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.",

author = "Kim, \{C. W.\} and S. Nussinov and Sze, \{W. K.\}",

note = "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.).",

year = "1987",

month = feb,

day = "5",

doi = "10.1016/0370-2693(87)90188-2",

language = "English",

volume = "184",

pages = "403--409",

journal = "Physics Letters B",

issn = "0370-2693",

publisher = "Elsevier BV",

number = "4",

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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.

UR - https://www.scopus.com/pages/publications/0000924495

UR - https://www.scopus.com/pages/publications/0000924495#tab=citedBy

U2 - 10.1016/0370-2693(87)90188-2

DO - 10.1016/0370-2693(87)90188-2

M3 - Article

AN - SCOPUS:0000924495

SN - 0370-2693

VL - 184

SP - 403

EP - 409

JO - Physics Letters B

JF - Physics Letters B

IS - 4

ER -

Non-adiabatic resonant conversion of solar neutrinos in three generations

Abstract

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