Non standard analysis of the solar neutrino anomaly (updated including the SNO day/night spectral data)
arXiv:hep-ph/0011307 · doi:10.1088/1126-6708/2000/12/016
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.
Version 5: addendum about the SNO NC data at pages 10, 11
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