Home > Publications database > 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 |2 doi |
024 | 7 | _ | |a 2128/24870 |2 Handle |
024 | 7 | _ | |a WOS:000539995300191 |2 WOS |
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 |2 ORCID |
336 | 7 | _ | |a Conference Paper |0 33 |2 EndNote |
336 | 7 | _ | |a Journal Article |0 PUB:(DE-HGF)16 |2 PUB:(DE-HGF) |m journal |
336 | 7 | _ | |a INPROCEEDINGS |2 BibTeX |
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336 | 7 | _ | |a Contribution to a conference proceedings |b contrib |m contrib |0 PUB:(DE-HGF)8 |s 1589443738_11909 |2 PUB:(DE-HGF) |
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. |b 1 |
700 | 1 | _ | |a Appel, S. |b 2 |
700 | 1 | _ | |a Atroshchenko, V. |b 3 |
700 | 1 | _ | |a Bagdasarian, Z. |0 P:(DE-Juel1)156420 |b 4 |u fzj |
700 | 1 | _ | |a Basilico, D. |b 5 |
700 | 1 | _ | |a Bellini, G. |b 6 |
700 | 1 | _ | |a Benziger, J. |b 7 |
700 | 1 | _ | |a Bick, D. |b 8 |
700 | 1 | _ | |a Bonfini, G. |b 9 |
700 | 1 | _ | |a Bravo, D. |b 10 |
700 | 1 | _ | |a Caccianiga, B. |b 11 |
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700 | 1 | _ | |a Cappelli, L. |b 14 |
700 | 1 | _ | |a Cavalcante, P. |b 15 |
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700 | 1 | _ | |a Chepurnov, A. |b 17 |
700 | 1 | _ | |a Choi, K. |b 18 |
700 | 1 | _ | |a D'Angelo, D. |b 19 |
700 | 1 | _ | |a Davini, S. |b 20 |
700 | 1 | _ | |a Derbin, A. |b 21 |
700 | 1 | _ | |a Di Giacinto, A. |b 22 |
700 | 1 | _ | |a Di Marcello, V. |b 23 |
700 | 1 | _ | |a Ding, X. F. |b 24 |
700 | 1 | _ | |a Di Lüdovico, A. |b 25 |
700 | 1 | _ | |a Di Noto, L. |b 26 |
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700 | 1 | _ | |a Gabriele, F. |b 30 |
700 | 1 | _ | |a Galbiati, C. |b 31 |
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700 | 1 | _ | |a Ianni, Aldo |b 40 |
700 | 1 | _ | |a Ianni, Andrea |b 41 |
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700 | 1 | _ | |a Jeschke, D. |b 43 |
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700 | 1 | _ | |a Laubenstein, M. |b 48 |
700 | 1 | _ | |a Litvinovich, E. |b 49 |
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700 | 1 | _ | |a Lukyanchenko, G. |b 53 |
700 | 1 | _ | |a Lukyanchenko, L. |b 54 |
700 | 1 | _ | |a Machulin, I. |b 55 |
700 | 1 | _ | |a Manuzio, G. |b 56 |
700 | 1 | _ | |a Marcocci, S. |b 57 |
700 | 1 | _ | |a Maricic, J. |b 58 |
700 | 1 | _ | |a Martyn, J. |b 59 |
700 | 1 | _ | |a Meroni, E. |b 60 |
700 | 1 | _ | |a Meyer, M. |0 P:(DE-HGF)0 |b 61 |
700 | 1 | _ | |a Miramonti, L. |b 62 |
700 | 1 | _ | |a Misiaszek, M. |b 63 |
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700 | 1 | _ | |a Nieslony, M. |b 66 |
700 | 1 | _ | |a Oberauer, L. |b 67 |
700 | 1 | _ | |a Orekhov, V. |b 68 |
700 | 1 | _ | |a Ortica, F. |b 69 |
700 | 1 | _ | |a Pallavicini, M. |b 70 |
700 | 1 | _ | |a Papp, L. |b 71 |
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700 | 1 | _ | |a Pietrofaccia, L. |b 73 |
700 | 1 | _ | |a Pilipenko, N. |b 74 |
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700 | 1 | _ | |a Raikov, G. |b 76 |
700 | 1 | _ | |a Ranalli, M. T. |b 77 |
700 | 1 | _ | |a Ranucci, G. |b 78 |
700 | 1 | _ | |a Razeto, A. |b 79 |
700 | 1 | _ | |a Re, A. |b 80 |
700 | 1 | _ | |a Redchuk, Mariia |0 P:(DE-Juel1)171322 |b 81 |u fzj |
700 | 1 | _ | |a Romani, A. |b 82 |
700 | 1 | _ | |a Rossi, N. |0 P:(DE-HGF)0 |b 83 |
700 | 1 | _ | |a Rottenanger, S. |b 84 |
700 | 1 | _ | |a Schönert, S. |b 85 |
700 | 1 | _ | |a Semenov, D. |b 86 |
700 | 1 | _ | |a Skorokhvatov, M. |b 87 |
700 | 1 | _ | |a Smirnov, O. |b 88 |
700 | 1 | _ | |a Sotnikov, A. |b 89 |
700 | 1 | _ | |a Suvorov, Y. |b 90 |
700 | 1 | _ | |a Tartaglia, R. |b 91 |
700 | 1 | _ | |a Testera, G. |b 92 |
700 | 1 | _ | |a Thurn, J. |b 93 |
700 | 1 | _ | |a Unzhakov, E. |b 94 |
700 | 1 | _ | |a Vishneva, A. |b 95 |
700 | 1 | _ | |a Vogelaar, R. B. |b 96 |
700 | 1 | _ | |a von Feilitzsch, F. |b 97 |
700 | 1 | _ | |a Wojcik, M. |b 98 |
700 | 1 | _ | |a Wurm, M. |b 99 |
700 | 1 | _ | |a Zaimidoroga, O. |b 100 |
700 | 1 | _ | |a Zavatarelli, S. |b 101 |
700 | 1 | _ | |a Zuber and G. Zuzel, K. |b 102 |
700 | 1 | _ | |a Zavatarelli, S. |0 P:(DE-HGF)0 |b 103 |e Corresponding author |
773 | _ | _ | |a 10.1088/1742-6596/1468/1/012192 |0 PERI:(DE-600)2166409-2 |n 1 |p 012192 |t Journal of physics / Conference Series |v 1468 |y 2020 |x 1742-6588 |
856 | 4 | _ | |u https://iopscience.iop.org/article/10.1088/1742-6596/1468/1/012192/pdf |
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