Solar neutrino experiments and Borexino perspectives

Abstract

We present an updated analysis of all the data available about solar neutrinos, including the charged current SNO results. The best fit of the data is obtained in the Large Mixing Angle region, but different solutions are still possible. We also study the perspectives of Borexino and conclude that this experiment, with a parallel analysis of total rate and day-night asymmmetry, should be able to discriminate between the different possible solutions.

3 pages, Latex, talk given by V. Antonelli at TAUP 2001 Conference

References in corpus (2)

• Measurement of the rate of nu_e + d --> p + p + e^- interactions produced by 8B solar neutrinos at the Sudbury Neutrino Observatory
• Global analysis of Solar neutrino oscillation evidence including SNO and implications for Borexino

Cited by in corpus (9)

• Neutrino mass parameters from Kamland, SNO and other solar evidence
• Determination of Neutrino mixing parameters after SNO oscillation evidence
• KamLAND potentiality on the determination of Neutrino mixing parameters in the post SNO-NC era
• KamLAND, solar antineutrinos and the solar magnetic field
• KamLAND Bounds on Solar Antineutrinos and neutrino transition magnetic moments
• The solar neutrino puzzle: present situation and future scenarios
• KamLAND, solar antineutrinos and their magnetic moment
• Particle oscillations in external chaotic fields
• Neutrino transition magnetic moments and the solar magnetic field on the light of the Kamland evidence