Hauptseite > Publikationsdatenbank > The study of solar neutrinos and of non-standard neutrino interactions with Borexino > print

001     875087
005     20210130004844.0
024 7 _ |a 10.1088/1742-6596/1468/1/012192
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024 7 _ |a 2128/24870
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024 7 _ |a WOS:000539995300191
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037 _ _ |a FZJ-2020-01796
041 _ _ |a English
082 _ _ |a 530
100 1 _ |a Agostini, M.
|b 0
111 2 _ |a 16th International Conference on Topics in Astroparticle and Underground physics
|g TAUP2019
|c Toyama
|d 2019-09-09 - 2019-09-13
|w Japan
245 _ _ |a The study of solar neutrinos and of non-standard neutrino interactions with Borexino
260 _ _ |a Bristol
|c 2020
|b IOP Publ.
300 _ _ |a 012192
336 7 _ |a CONFERENCE_PAPER
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336 7 _ |a Conference Paper
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336 7 _ |a Journal Article
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336 7 _ |a INPROCEEDINGS
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520 _ _ |a The Borexino liquid scintillator neutrino observatory has a unique capability toperform high-precision solar neutrino observations thanks to its exceptional radiopurity andgood energy resolution (5% at 1 MeV). A comprehensive study of the pp-chain neutrinos waspresented that includes the direct measurements of 7Be, pp and pep neutrino fluxes with thehighest precision ever achieved (down to 2.8% in the 7Be component), the 8B with the lowestenergy threshold, the best limit on CNO neutrinos and the first Borexino limit on hep neutrinos.These results are important to validate the MSW-LMA oscillation paradigm across the full solarenergy range and to exclude possible Non-Standard neutrino Interactions (NSIs). In particularthe effects of neutrino-flavor-diagonal Neutral-Current (NC) interactions that modify the νeeand ντ e couplings while preserving their chiral and flavor structures, have been investigated. Atdetection, the shape of the electron-recoil spectrum is affected by changes in the νee and ντ ecouplings, quantified by the parameters εL/Re and εL/Rτ . New bounds to all four parameters wereobtained, quite stringent compared to the global ones. In particular, the best constraint to-dateon εLe was achieved. A comprehensive summary of all the recent results on solar neutrinos fromBorexino is reported in the present paper.
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700 1 _ |a Altenmüller, K.
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700 1 _ |a Zavatarelli, S.
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773 _ _ |a 10.1088/1742-6596/1468/1/012192
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856 4 _ |u https://iopscience.iop.org/article/10.1088/1742-6596/1468/1/012192/pdf
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