Physics – High Energy Physics – High Energy Physics - Phenomenology
Scientific paper
2001-09-19
JHEP 0111:048,2001
Physics
High Energy Physics
High Energy Physics - Phenomenology
12 pages, 4 figures. v2: comments and references added, final version
Scientific paper
10.1088/1126-6708/2001/11/048
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.
Strumia Alessandro
Vissani Francesco
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