Matter effects for `just so' oscillations
| dc.creator | Narayan, Mohan | |
| dc.creator | Sankar, S. Uma | |
| dc.date | 2000-04-21 | |
| dc.date.accessioned | 2026-07-07T03:41:13Z | |
| dc.date.available | 2026-07-07T03:41:13Z | |
| dc.description | We study the effect of the matter term on the evolution of the solar neutrinos when the neutrino parameters are those of the `just-so' case. The extreme non-adiabatic effects at the edge of the sun reduce the expression for the survival probability in the just-so case to that of the vacuum case. This conclusion is independent of the width of the extreme non-adiabatic region, which is a function of the density profile of the sun beyond $r > 0.9 R_s$. However, in its propagation, neutrino encounters regions of moderate (non-extreme) non-adiabticity. Neutrino traversal through these regions give corrections to the survival probability which are profile dependent. | |
| dc.description | 11 pages including one figure | |
| dc.identifier | https://arxiv.org/abs/hep-ph/0004204 | |
| dc.identifier | http://arxiv.org/abs/hep-ph/0004204 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/39533 | |
| dc.subject | High Energy Physics - Phenomenology | |
| dc.title | Matter effects for `just so' oscillations | |
| dc.type | text |