arXiv · hep-ph/0601091
A Lithium Experiment in the Program of Solar Neutrino Research
Abstract
The experiments sensitive to pp-neutrinos from the Sun are very perspective for the precise measurement of a mixing angle $θ_{12}$. A $ν$e$^{-}$ scattering experiment (Xmass) and/or a charged-current experiment (the indium detector) can measure the flux of electron pp-neutrinos. One can find the total flux of pp-neutrinos from a luminosity constraint after the contribution of $^7$Be and CNO neutrinos to the total luminosity of the Sun are measured. The radiochemical experiment utilizing a lithium target has the high sensitivity to the CNO neutrinos, thus, it has a good promise for the precise measurement of a mixing angle and for the test of a current theory of the evolution of the stars.
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A. Kopylov, I. Orekhov, V. Petukhov, A. Solomatin. 2006-01-12. A Lithium Experiment in the Program of Solar Neutrino Research. https://doi.org/10.1134/s1063778806110044
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