Adiabatic resonant oscillations of solar neutrinos in three generations

C. W. Kim, Wah-Keung Sze

研究成果: 雜誌貢獻文章

43 引文 斯高帕斯(Scopus)

摘要

The Mikheyev-Smirnov-Wolfenstein model of resonant solar-neutrino oscillations is discussed for three generations of leptons. Assuming adiabatic transitions, bounds for the and e-neutrinos mass-squared difference 21,0 are obtained as a function of the mixing angle theta1. The allowed region in the 21,0-theta1 plot that would solve the solar-neutrino problem is shown to be substantially larger than that of the two-generation case. In particular, the difference between the two- and three-generation cases becomes significant for theta1 larger than 20°.

原文英語
頁(從 - 到)1404-1408
頁數5
期刊Physical Review D
35
發行號4
DOIs
出版狀態已發佈 - 1987 一月 1

ASJC Scopus subject areas

  • Nuclear and High Energy Physics
  • Physics and Astronomy (miscellaneous)

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