Physics – High Energy Physics – High Energy Physics - Phenomenology
Scientific paper
2002-11-26
Phys.Rev.D67:073001,2003
Physics
High Energy Physics
High Energy Physics - Phenomenology
Updated to include the first KamLAND data. One figure added
Scientific paper
10.1103/PhysRevD.67.073001
Assuming the current best-fit solutions to the solar neutrino problem at large mixing angle, we briefly illustrate how prospective data from the Sudbury Neutrino Observatory (SNO) and from the Kamioka Liquid scintillator Anti-Neutrino Detector (KamLAND) can increase our confidence in the occurrence of standard matter effects on active neutrino flavor oscillations in the Sun, which are starting to emerge from current data.
Fogli Gian Luigi
Lisi Eligio
Palazzo Antonio
Rotunno Anna Maria
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