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. 2008 Aug 29;101(9):091302.
doi: 10.1103/PhysRevLett.101.091302. Epub 2008 Aug 29.

Direct measurement of the 7Be solar neutrino flux with 192 days of borexino data

C Arpesella  1 H O BackM BalataG BelliniJ BenzigerS BonettiA BrigattiB CaccianigaL CadonatiF CalapriceC CarraroG CecchetA ChavarriaM ChenF Dalnoki-VeressD D'AngeloA de BariA de BellefonH de KerretA DerbinM DeutschA di CredicoG di PietroR EisensteinF EliseiA EtenkoR FernholzK FomenkoR FordD FrancoB FreudigerC GalbiatiF GattiS GazzanaM GiammarchiD GiugniM Goeger-NeffT GoldbrunnerA GorettiC GriebC HagnerW HampelE HardingS HardyF X HartmanT HertrichG HeusserAldo IanniAndrea IanniM JoyceJ KikoT KirstenV KobychevG KorgaG KorschinekD KrynV LagomarsinoP LamarcheM LaubensteinC LendvaiM LeungT LewkeE LitvinovichB LoerP LombardiL LudhovaI MachulinS MalvezziS ManeckiJ ManeiraW ManeschgI MannoD ManuzioG ManuzioA MartemianovF MasettiU MazzucatoK McCartyD McKinseyQ MeindlE MeroniL MiramontiM MisiaszekD MontanariM E MonzaniV MuratovaP MusicoH NederA NelsonL NiedermeierL OberauerM ObolenskyM OrsiniF OrticaM PallaviciniL PappS ParmeggianoL PerassoA PocarR S RaghavanG RanucciW RauA RazetoE ResconiP RissoA RomaniD RountreeA SabelnikovR SaldanhaC SalvoD SchimizziS SchönertT ShuttH SimgenM SkorokhvatovO SmirnovA SonnenscheinA SotnikovS SukhotinY SuvorovR TartagliaG TesteraD VignaudS VitaleR B VogelaarF von FeilitzschR von HentigT von HentigM WojcikM WurmO ZaimidorogaS ZavatarelliG ZuzelBorexino Collaboration
Affiliations

Direct measurement of the 7Be solar neutrino flux with 192 days of borexino data

C Arpesella et al. Phys Rev Lett. .

Abstract

We report the direct measurement of the 7Be solar neutrino signal rate performed with the Borexino detector at the Laboratori Nazionali del Gran Sasso. The interaction rate of the 0.862 MeV 7Be neutrinos is 49+/-3stat+/-4syst counts/(day.100 ton). The hypothesis of no oscillation for 7Be solar neutrinos is inconsistent with our measurement at the 4sigma C.L. Our result is the first direct measurement of the survival probability for solar nu(e) in the transition region between matter-enhanced and vacuum-driven oscillations. The measurement improves the experimental determination of the flux of 7Be, pp, and CNO solar nu(e), and the limit on the effective neutrino magnetic moment using solar neutrinos.

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