Journal Article

FZJ-2019-02023

http://join2-wiki.gsi.de/foswiki/pub/Main/Artwork/join2_logo100x88.png Solar Neutrinos Spectroscopy with Borexino Phase-II

Miramonti, L. (Corresponding author) ; Agostini, M. ; Altenmueller, K. ; Appel, S. ; Atroshchenko, V. ; Bagdasarian, Z.FZJ* ; Basilico, D. ; Bellini, G. ; Benziger, J. ; Bick, D. ; Bolognino, I. ; Bonfini, G. ; Bravo, D. ; Caccianiga, B. ; Calaprice, F. ; Caminata, A. ; Caprioli, S. ; Carlini, M. ; Cavalcante, P. ; Cavanna, F. ; Chepurnov, A. ; Choi, K. ; Collica, L. ; Davini, S. ; Derbin, A. ; Ding, X. ; Di Ludovico, A. ; Di Noto, L. ; Drachnev, I. ; Fomenko, K. ; Formozov, A. ; Franco, D. ; Gabriele, F. ; Galbiati, C. ; Gschwender, M. ; Ghiano, C. ; Giammarchi, M. ; Goretti, A. ; Gromov, M. ; Guffanti, D. ; Hagner, C. ; Houdy, T. ; Hungerford, E. ; Ianni, A. ; Ianni, A. ; Jany, A. ; Jeschke, D. ; Kobychev, V. ; Korablev, D. ; Korga, G. ; Lachenmaier, T. ; Laubenstein, M. ; Litvinovich, E. ; Lombardi, F. ; Lombardi, P. ; Ludhova, L.FZJ* ; Lukyanchenko, G. ; Lukyanchenko, L. ; Machulin, I. ; Manuzio, G. ; Marcocci, S. ; Maricic, J. ; Martyn, J. ; Meroni, E. ; Meyer, M. ; Misiaszek, M. ; Muratova, V. ; Neumair, B. ; Oberauer, L. ; Opitz, B. ; Orekhov, V. ; Ortica, F. ; Pallavicini, M. ; Papp, L. ; Penek, O.FZJ* ; Pietrofaccia, L. ; Pilipenko, N. ; Pocar, A. ; Porcelli, A. ; Raikov, G. ; Ranucci, G. ; Razeto, A. ; Re, A. ; Redchuk, M.FZJ* ; Romani, A. ; Rossi, N. ; Rottenanger, S. ; Schöenert, S. ; Semenov, D. ; Skorokhvatov, M. ; Smirnov, O. ; Sotnikov, A. ; Stokes, L. ; Suvorov, Y. ; Tartaglia, R. ; Testera, G. ; Thurn, J. ; Toropova, M. ; Unzhakov, E. ; Vishneva, A. ; Vogelaar, B. ; von Feilitzsch, F. ; Weinz, S. ; Wojcik, M. ; Wurm, M. ; Yokley, Z. ; Zaimidoroga, O. ; Zavatarelli, S. ; Zuber, K. ; Zuzel, G.

2018
MDPI Basel

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Please use a persistent id in citations: http://hdl.handle.net/2128/21882  doi:10.3390/universe4110118

Abstract: Solar neutrinos have played a central role in the discovery of the neutrino oscillation mechanism. They still are proving to be a unique tool to help investigate the fusion reactions that power stars and further probe basic neutrino properties. The Borexino neutrino observatory has been operationally acquiring data at Laboratori Nazionali del Gran Sasso in Italy since 2007. Its main goal is the real-time study of low energy neutrinos (solar or originated elsewhere, such as geo-neutrinos). The latest analysis of experimental data, taken during the so-called Borexino Phase-II (2011-present), will be showcased in this talk—yielding new high-precision, simultaneous wide band flux measurements of the four main solar neutrino components belonging to the “pp” fusion chain (pp, pep, 7 Be, 8 B), as well as upper limits on the remaining two solar neutrino fluxes (CNO and hep)

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Contributing Institute(s):

1. Experimentelle Hadrondynamik (IKP-2)

Research Program(s):

1. 612 - Cosmic Matter in the Laboratory (POF3-612) (POF3-612)

Appears in the scientific report 2019

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Database coverage:
; ; ; Clarivate Analytics Master Journal List ; DOAJ Seal ; Emerging Sources Citation Index ; Web of Science Core Collection

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