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arXiv · hep-ph/0109172

Which solar neutrino experiment after KamLAND and Borexino?

Alessandro Strumia·Francesco Vissani
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Abstract

We estimate how well we will know the parameters of solar neutrino oscillations after KamLAND and Borexino. The expected error on Delta m^2 is few per-mille in the VO and QVO regions, few per-cent in the LMA region, and around 10% in the LOW region. The expected error on sin^2 2theta is around 5%. KamLAND and Borexino will tell unambiguously which specific new measurement, dedicated to pp solar neutrinos, is able to contribute to the determination of theta and perhaps of Delta m^2. The present data suggest as more likely outcomes: no measurement, or the total pp rate, or its day/night variation.

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Alessandro Strumia, Francesco Vissani. 2001-10-24. Which solar neutrino experiment after KamLAND and Borexino?. https://doi.org/10.1088/1126-6708%2F2001%2F11%2F048

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