Spin-flavour conversions of neutrinos in collapsing stars
| dc.creator | Husain, Athar | |
| dc.date | 1999-02-02 | |
| dc.date.accessioned | 2026-07-07T04:06:21Z | |
| dc.date.available | 2026-07-07T04:06:21Z | |
| dc.description | I discuss in some detail the spin-flavour conversions of neutrinos in the almost isotopically neutral region of collapsing stars along with the resulting experimental signatures. In particular, I show that for realistic magnetic field strength, the observable effects may exist for neutrino magnetic moment, $μ\sim (2-3)\times 10^{-14}μ_B$ ($μ_B$ is the Bohr magneton) with relevant neutrino mass squared difference, $Δm^2 \sim (10^{-9}-10^{-8}) eV^2$. | |
| dc.description | 5 pages, Latex (uses sprocl.sty), No figures, Talk presented at Second Meeting on New Worlds in Astroparticle Physics (NW 98),Faro, Portugal, 3-5 September, 1998 (to appear in its proceedings) | |
| dc.identifier | https://arxiv.org/abs/hep-ph/9902222 | |
| dc.identifier | http://arxiv.org/abs/hep-ph/9902222 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/48736 | |
| dc.subject | High Energy Physics - Phenomenology | |
| dc.subject | Astrophysics | |
| dc.title | Spin-flavour conversions of neutrinos in collapsing stars | |
| dc.type | text |