Neutrinos in Stochastic Media: From Sun to Core-Collapse Supernovae
| dc.creator | Balantekin, A. B. | |
| dc.date | 2001-09-18 | |
| dc.date.accessioned | 2026-07-07T11:09:09Z | |
| dc.date.available | 2026-07-07T11:09:09Z | |
| dc.description | Recent work on neutrino propagation in stochastic media and its implications for the Sun and core-collapse supernovae are reviewed. It is shown that recent results from Sudbury Neutrino Observatory and SuperKamiokande combined with a best global fit value of $δm^2= 5\times 10^{-5}$ eV$^2$ and $\tan^2 θ= 0.3$ rule out solar electron density fluctuations of a few percent or more. It is argued that solar neutrino experiments may be able to rule out even smaller fluctuations in the near future. | |
| dc.description | 4 pages, to be published in the proceedings of the International Nuclear Physics Conference (INPC 2001): Nuclear Physics And The 21st Century, 30 Jul - 3 Aug 2001, Berkeley, California | |
| dc.identifier | https://arxiv.org/abs/hep-ph/0109163 | |
| dc.identifier | http://arxiv.org/abs/hep-ph/0109163 | |
| dc.identifier | AIPConf.Proc.610:969-972,2002 | |
| dc.identifier | doi:10.1063/1.1470265 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/190371 | |
| dc.subject | High Energy Physics - Phenomenology | |
| dc.title | Neutrinos in Stochastic Media: From Sun to Core-Collapse Supernovae | |
| dc.type | text |