Sarkar, Utpal (1987) Pseudo-Dirac solar neutrinos? Physical Review D - Particles, Fields, Gravitation and Cosmology, 35 (4). pp. 1528-1530. ISSN 1550-7998
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Official URL: http://prd.aps.org/abstract/PRD/v35/i4/p1528_1
Related URL: http://dx.doi.org/10.1103/PhysRevD.35.1528
Abstract
The compatibility of a recent possible explanation of the solar-neutrino puzzle and the result of Boris et al. on limits on neutrino mass is discussed. It is shown that if the electron and muon Majorana neutrinos combine to form a pseudo-Dirac particle of mass ~35 eV, then the radiative corrections will generate a mass-square difference 3×10−5 eV, which explains why Davis and his collaborators find fewer solar neutrinos than predicted. This idea can be naturally embedded in superstring theories.
| Item Type: | Article |
|---|---|
| Source: | Copyright of this article belongs to The American Physical Society. |
| ID Code: | 45465 |
| Deposited On: | 28 Jun 2011 04:56 |
| Last Modified: | 28 Jun 2011 04:56 |
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