6533b853fe1ef96bd12acccd
RESEARCH PRODUCT
Confronting spin flavor solutions of the solar neutrino problem with current and future solar neutrino data
O. G. MirandaVictor B. SemikozT. I. RashbaJosé W. F. ValleJuan Barrancosubject
PhysicsNuclear and High Energy PhysicsParticle physicsOscillationSolar neutrinoFOS: Physical sciencesFísicaField (mathematics)Solar neutrino problemTable (information)Physics::GeophysicsHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Physics::Space PhysicsHigh Energy Physics::ExperimentNeutrinoBorexinoSpin-½description
We show that spin flavor precession solutions to the solar neutrino problem, although preferred by the latest solar data, are ruled out by the first results from the KamLAND reactor experiment, at more than 3_sigma. An illustrative chi2 plot comparing these descriptions with oscillations is given.
| year | journal | country | edition | language |
|---|---|---|---|---|
| 2002-07-26 | Physical Review D |