Non standard analysis of the solar neutrino anomaly (updated including the SNO day/night spectral data)

Abstract

Continuing previous work, a model independent analysis of the solar neutrino anomaly is performed in terms of neutrino oscillations, allowing a comparison with the predictions of the Standard Solar Model. SMA and LMA solutions emerge also in this case, although somewhat different from the standard ones. The significance of the NC/CC double ratio measurable in SNO is illustrated in this context.

Comments: Version 5: addendum about the SNO NC data at pages 10, 11