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2011

First evidence of pep solar neutrinos by direct detection in Borexino

The Borexino Collaboration

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We observed, for the first time, solar neutrinos in the 1.0-1.5 MeV energy range.

We measured the rate of pep solar neutrino interactions in Borexino to be [3.1+-0.6(stat)+-0.3(syst)] counts/(day x 100 ton) and provided a constraint on the CNO solar neutrino interaction rate of <7.9 counts/(day x 100 ton) (95% C.L.).
The absence of the solar neutrino signal is disfavored at 99.97% C.L., while the absence of the pep signal is disfavored at 98% C.L.
This unprecedented sensitivity was achieved by adopting novel data analysis techniques for the rejection of cosmogenic 11C, the dominant background in the 1-2 MeV region.

First evidence of pep solar neutrinos by direct detection in Borexino · Around

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