Statistical treatment of detection cross-section uncertainties in the analysis of solar neutrino data

Details Statistical treatment of detection cross-section uncertainties in the analysis of solar neutrino data Statistical treatment of detection cross-section uncertainties in the analysis of solar neutrino data

2000-06-02

arxiv.org/abs/hep-ph/0006026v2

Phys.Lett. B488 (2000) 339-343

Physics

High Energy Physics

High Energy Physics - Phenomenology

12 pages. Corrected Figures 4 and 5 (vacuum oscillations)

Scientific paper

10.1016/S0370-2693(00)00866-2

We propose a modification to the standard statistical treatment of the detection cross-section uncertainties in the analysis of solar neutrino data. We argue that the uncertainties of the energy-averaged cross sections of the different neutrino fluxes in the same experiment should be treated as correlated. We show that the resulting allowed regions for the neutrino oscillation parameters are significantly larger than the ones obtained with uncorrelated uncertainties.

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