Solar neutrino oscillations and indications of matter effects in the Sun

Physics – High Energy Physics – High Energy Physics - Phenomenology

Scientific paper

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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.

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