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Pseudo Dirac neutrinos and the solar-neutrino problem

descriptionPublicationkeyboard_double_arrow_right Article 15 May 1992Publisher:American Physical Society (APS)Journal:Physical Review D, volume 45, pages R3316-R3320 (issn: 0556-2821,

Authors: Hisakazu Minakata; Hiroshi Nunokawa;

doi: 10.1103/physrevd.45.r3316

pmid: 10014294

Pseudo Dirac neutrinos and the solar-neutrino problem

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Abstract

Observational consequences of the pseudo-Dirac-neutrino hypothesis of Kobayashi, Lim, and Nojiri are examined in the context of the solar-neutrino problem. Detailed calculations are performed to obtain expected rates at the $^{37}\mathrm{Cl}$, Kamiokande II, and $^{71}\mathrm{Ga}$ detectors. In a region of parameters consistent with the former two experiments the $^{71}\mathrm{Ga}$ rate is predicted to be 50-65 solar-neutrino units.

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Tokyo Metropolitan University
Japan

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