Neutrino transitional magnetic moment and non-Abelian discrete symmetry
- 1 September 1990
- journal article
- research article
- Published by American Physical Society (APS) in Physical Review D
- Vol. 42 (5) , 1599-1603
- https://doi.org/10.1103/physrevd.42.1599
Abstract
We propose a mechanism which naturally will give rise to a small mass but a large transitional magnetic moment for the neutrino such that the solar-neutrino deficit problem can be explained. The idea is a discrete version of Voloshin's SU(2) mechanism. An example of such a mechanism using the quaternion group is illustrated.Keywords
This publication has 22 references indexed in Scilit:
- Model for large transition magnetic moment of the electron neutrinoPhysical Review Letters, 1989
- Neutrino magnetic moment in the SU(3)L×U(1) modelPhysics Letters B, 1989
- A neutrino with a large magnetic moment and a naturally small massPhysics Letters B, 1989
- Neutrino masses and the Voloshin-Vysotsky-Okun solution to the solar-neutrino problemPhysical Review D, 1988
- New bounds on neutrino magnetic moments from stellar collapsePhysical Review D, 1988
- Limits on the Neutrino Magnetic Moment from SN1987APhysical Review Letters, 1988
- Limit on the Magnetic Moment of the Neutrino from Supernova 1987A ObservationsPhysical Review Letters, 1988
- Magnetic moment of Dirac neutrinosPhysical Review D, 1987
- Effect of neutrino magnetic moment on solar neutrino observationsAstrophysics and Space Science, 1971
- Search for Neutrinos from the SunPhysical Review Letters, 1968