Correlated Neutrino Oscillations

Simple item page
dc.creatorMa, Ernest
dc.date1995-07-03
dc.date.accessioned2026-07-07T03:57:50Z
dc.date.available2026-07-07T03:57:50Z
dc.descriptionIn solar neutrino oscillations, if $ν_e$ has a significant third massive component, the allowed parameter space in $Δm^2$ and $\sin^2 2 θ$ for the first two components is shown to be greatly increased. This third component may be correlated to atmospheric neutrino oscillations, as shown in a specific predictive seesaw model of the $3 \times 3$ neutrino mass matrix. Possible variations to include the recent LSND results are briefly discussed.
dc.description6 pages, 1 figure not included, talk given at Valencia 95
dc.identifierhttps://arxiv.org/abs/hep-ph/9507209
dc.identifierhttp://arxiv.org/abs/hep-ph/9507209
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/45603
dc.subjectHigh Energy Physics - Phenomenology
dc.titleCorrelated Neutrino Oscillations
dc.typetext

Files

Collections

arXiv