Solar neutrino oscillations and indications of matter effects in the Sun

7 April 2003

journal article
research article
Published by American Physical Society (APS) in Physical Review D

Vol. 67 (7) , 073001
https://doi.org/10.1103/physrevd.67.073001

Abstract

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 Antineutrino 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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