A Preliminary Look at the Physics Reach of a Solar Neutrino TPC: Time-Independent Two Neutrino Oscillations

Simple item page
dc.creatorBonvicini, G.
dc.creatorCheu, E.
dc.creatorDolbeau, J.
dc.creatorGorodetzki, P.
dc.creatorKessler, R.
dc.creatorPaolone, V.
dc.creatorProsper, H.
dc.date2001-09-21
dc.date.accessioned2026-07-07T03:45:20Z
dc.date.available2026-07-07T03:45:20Z
dc.descriptionThis paper will discuss the physics reach of a solar neutrino TPC containing many tons of He4 under high pressure. Particular attention is given to the LMA and SMA solutions, which are allowed by current data, and which are characterized by a lack of time-dependent phenomena (either summer-winter or day-night asymmetries). In this case, the physics of neutrino masses and mixing is all contained in the energy dependence of the electron neutrino survival probability, (or in its reciprocal, the electron neutrino disappearance probability).
dc.description19 pages, 12 figures
dc.identifierhttps://arxiv.org/abs/hep-ph/0109199
dc.identifierhttp://arxiv.org/abs/hep-ph/0109199
dc.identifiereConf C010630 (2001) E603
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/40893
dc.subjectHigh Energy Physics - Phenomenology
dc.titleA Preliminary Look at the Physics Reach of a Solar Neutrino TPC: Time-Independent Two Neutrino Oscillations
dc.typetext

Files

Collections

arXiv