How unique are the MSW parameters ?
| dc.creator | Mohapatra, P. K. | |
| dc.date | 1992-12-14 | |
| dc.date.accessioned | 2026-07-07T03:55:52Z | |
| dc.date.available | 2026-07-07T03:55:52Z | |
| dc.description | We investigate the effect of a possible large frozen-in magnetic field in the core of the sun and a neutrino magnetic moment of the order of $10^{-10}$ Bohr magneton on the MSW parameters. Such a possibility can completely depolarize the $ν_{eL}$ resulting in a factor of half of the emitted number. This in combination with MSW can explain the present experimental data on solar neutrinos but with a different region of the parameter space than the regular MSW alone. In this scenario there is a larger region of parameter space allowed. There is a large strip of parameter space corresponding to adiabatic solution and no solution for large mixing angle region. The non-adiabatic region still remains as a solution but shifted and larger relative to the regular MSW. | |
| dc.description | 12 pages, 4 figures in two pages | |
| dc.identifier | https://arxiv.org/abs/hep-ph/9212258 | |
| dc.identifier | http://arxiv.org/abs/hep-ph/9212258 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/44721 | |
| dc.subject | High Energy Physics - Phenomenology | |
| dc.title | How unique are the MSW parameters ? | |
| dc.type | text |