first real–time detection of solar pp neutrinos by borexino
Clicks: 192
ID: 158059
2016
Solar neutrinos have been pivotal to the discovery of neutrino flavour oscillations and are a unique tool to probe the reactions that keep the Sun shine. Although most of solar neutrino components have been directly measured, the neutrinos emitted by the keystone pp reaction, in which two protons fuse to make a deuteron, have so far eluded direct detection. The Borexino experiment, an ultra–pure liquid scintillator detector running at the Laboratori Nazionali del Gran Sasso in Italy, has now filled the gap, providing the first direct real time measurement of pp neutrinos and of the solar neutrino luminosity.
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Authors | ;Pallavicini M.;Bellini G.;Benziger J.;Bick D.;Bonfini G.;Bravo D.;Caccianiga B.;Calaprice F.;Caminata A.;Cavalcante P.;Chavarria A.;Chepurnov A.;D'Angelo D.;Davini S.;Derbin A.;Empl A.;Etenko A.;Fomenko K.;Franco D.;Gabriele F.;Galbiati C.;Gazzana S.;Ghiano C.;Giammarchi M.;Göger-Neff M.;Goretti A.;Gromov M.;Hagner C.;Hungerford E.;Ianni Al.;Ianni An.;Kayser M.;Kobychev V.;Korablëv D.;Korga G.;Kryn D.;Laubenstein M.;Lehnert B.;Lewke T.;Litvinovich E.;Lombardi F.;Lombardi P.;Ludhova L.;Lukyanchenko G.;Machulin I.;Manecki S.;Maneschg W.;Marcocci S.;Meindl Q.;Meroni E.;Meyer M.;Miramonti L.;Misiaszek M.;Montuschi M.;Mosteiro P.;Muratova V.;Oberauer L.;Obolensky M.;Ortica F.;Otis K.;Papp L.;Perasso L.;Pocar A.;Ranucci G.;Razeto A.;Re A.;Romani A.;Rossi N.;Saldanha R.;Salvo C.;Schönert S.;Simgen H.;Skorokhvatov M.;Smirnov O.;Sotnikov A.;Sukhotin S.;Suvorov Y.;Tartaglia R.;Testera G.;Vignaud D.;Vogelaar R.B.;Feilitzsch F. von;Wang H.;Winter J.;Wojcik M.;Wurm M.;Zaimidoroga O.;Zavatarelli S.;Zuber K.;Zuzel G. |
Journal | utilitas mathematica |
Year | 2016 |
DOI | 10.1051/epjconf/201612101001 |
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