Global analysis of solar neutrinos (assumed to be Majorana particles) together with the new KamLAND data
arXiv:hep-ph/0702057 · doi:10.1088/0954-3899/31/9/013
Abstract
Assuming neutrinos are Majorana particles having non-zero transition magnetic moments, a global analysis of solar neutrino data, together with the new KamLAND data, is presented in the resonant spin flavor precession (RSFP) framework. The allowed regions from solar data combined with new KamLAND data are examined at 0.95 confidence level (CL). The electron antineutrino flux from the Sun is calculated, and via the results obtained several limits are set for muB.
13 pages, 6 figures
References in corpus (6)
- Measurement of Neutrino Oscillation with KamLAND: Evidence of Spectral Distortion
- Measurement of the Total Active 8B Solar Neutrino Flux at the Sudbury Neutrino Observatory with Enhanced Neutral Current Sensitivity
- Getting the most from the statistical analysis of solar neutrino oscillations
- Constraining the neutrino magnetic moment with anti-neutrinos from the Sun
- Search for anti-electron-neutrinos from the Sun at Super-Kamiokande-I
- Resonance Spin Flavour Precession of Solar Neutrinos After SNO NC Data