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Day-night effect in solar neutrino oscillations with three flavors

Mattias Blennow·Tommy Ohlsson·Hakan Snellman
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Abstract

We investigate the effects of a nonzero leptonic mixing angle $θ_{13}$ on the solar neutrino day-night asymmetry. Using a constant matter density profile for the Earth and well-motivated approximations, we derive analytical expressions for the $ν_e$ survival probabilities for solar neutrinos arriving directly at the detector and for solar neutrinos which have passed through the Earth. Furthermore, we numerically study the effects of a non-zero $θ_{13}$ on the day-night asymmetry at detectors and find that they are small. Finally, we show that if the uncertainties in the parameters $θ_{12}$ and $Δm^2$ as well as the uncertainty in the day-night asymmetry itself were much smaller than they are today, this effect could, in principle, be used to determine $θ_{13}$.

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Mattias Blennow, Tommy Ohlsson, Hakan Snellman. 2004-03-11. Day-night effect in solar neutrino oscillations with three flavors. https://doi.org/10.1103/physrevd.69.073006

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