Four-Neutrino Oscillations
| dc.creator | Barger, V. | |
| dc.date | 1998-08-18 | |
| dc.date.accessioned | 2026-07-07T04:04:33Z | |
| dc.date.available | 2026-07-07T04:04:33Z | |
| dc.description | Models with three active neutrinos and one sterile neutrino can naturally account for maximal oscillations of atmospheric neutrinos, explain the solar neutrino deficit, and accommodate the results of the LSND experiment. The models predict either $ν_e\toν_τ$ or $ν_e\toν_s$ oscillations in long-baseline experiments with the atmospheric $δm^2$ scale and amplitude determined by the LSND oscillations. | |
| dc.description | 9 pages, Latex2.09, uses sprocl.sty and epsf.sty, 6 postscript files included. Talk presented at the 6th International Symposium on Particles, Strings and Cosmology (PASCOS98), Northeastern University, Boston, March 1998 | |
| dc.identifier | https://arxiv.org/abs/hep-ph/9808353 | |
| dc.identifier | http://arxiv.org/abs/hep-ph/9808353 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/48143 | |
| dc.subject | High Energy Physics - Phenomenology | |
| dc.title | Four-Neutrino Oscillations | |
| dc.type | text |