Akademik Veri Yönetim Sistemi
JOURNAL OF PHYSICS G-NUCLEAR AND PARTICLE PHYSICS, cilt.31, sa.9, ss.1123-1131, 2005 (SCI-Expanded)
Assuming neutrinos are Majorana particles having non-zero transit ion magnetic moments, a global analysis of solar neutrino data, together with the new KamLAND data, is presented in the resonant spin flavour precession (RSFP) framework. We used Wood-Saxon and Gaussian shaped magnetic field profiles throughout the entire Sun. For each magnetic field profile, allowed regions from solar data combined with the new KamLAND data are examined at 95% confidence level (CL). We show that all allowed regions are in the large mixing angle (LMA) region and remain the same as the mu B value is increased for both magnetic field profiles, contrary to the Dirac case studied in our previous work. The electron antineutrino flux from the Sun is calculated, and via the results obtained several limits are set for mu B.