000072033 001__ 72033
000072033 005__ 20171002115820.0
000072033 035__ $$9INSPIRETeX$$aAgostini:2017cav
000072033 035__ $$9arXiv$$aoai:arXiv.org:1709.00756
000072033 035__ $$9DESY$$zD17-kj37o
000072033 037__ $$9arXiv$$aarXiv:1709.00756$$chep-ex
000072033 100__ $$aAgostini, M.$$uGSSI, Aquila$$vGran Sasso Science Institute (INFN), 67100 L'Aquila, Italy
000072033 245__ $$9arXiv$$aImproved measurement of 8B solar neutrinos with 1.5 kt y of Borexino exposure
000072033 246__ $$9arXiv$$aImproved measurement of 8B solar neutrinos with 1.5 kt y of Borexino exposure
000072033 269__ $$c2017-09-03
000072033 300__ $$a13
000072033 500__ $$a*Temporary entry*
000072033 500__ $$9arXiv$$a13 pages, 14 figures, 4 tables
000072033 520__ $$9arXiv$$aWe report on an improved measurement of the $^8$B solar neutrino interaction rate with the Borexino detector at the Laboratori Nazionali del Gran Sasso. Neutrinos are detected via their elastic scattering on electrons in a large, radio-pure liquid scintillator target. Novel analysis approaches exploiting most of the active volume of the detector have enabled the collection of data from 1.5 kt$\cdot$y exposure between 2008 and 2016. The measured rate of solar neutrino-induced, scattered electrons above 3 MeV of energy is $0.220\substack{+0.015 \\ -0.016}\,(stat)\,\substack{+0.006 \\ -0.006}\,(syst)$~cpd/100~t, which corresponds to an observed solar neutrino flux assuming no neutrino flavor conversion of 2.55$\substack{+0.17 \\ -0.19}(stat)\substack{+0.07\\ -0.07}(syst)\times$10$^6$~cm$^{-2}\,$s$^{-1}$. If one assumes the $^8$B solar neutrino flux predicted by the high metallicity Standard Solar Model, the average $^8$B solar $\nu_e$ survival probability is 0.36$\pm$0.08 at the mean visible energy of 7.9~MeV, in good agreement with the MSW-LMA
000072033 540__ $$barXiv$$uhttp://arxiv.org/licenses/nonexclusive-distrib/1.0/
000072033 65017 $$2arXiv$$ahep-ex
000072033 65017 $$2INSPIRE$$aExperiment-HEP
000072033 65017 $$2arXiv$$aastro-ph.SR
000072033 65017 $$2INSPIRE$$aAstrophysics
000072033 693__ $$eBOREXINO
000072033 695__ $$2INSPIRE$$aneutrino: solar
000072033 695__ $$2INSPIRE$$aneutrino: flux
000072033 695__ $$2INSPIRE$$amodel: solar
000072033 695__ $$2INSPIRE$$aneutrino: interaction
000072033 695__ $$2INSPIRE$$aneutrino: flavor
000072033 695__ $$2INSPIRE$$ascintillation counter: liquid
000072033 695__ $$2INSPIRE$$ascintillation counter: target
000072033 695__ $$2INSPIRE$$aboron: semileptonic decay
000072033 695__ $$2INSPIRE$$aBorexino
000072033 695__ $$2INSPIRE$$aMSW effect
000072033 695__ $$2INSPIRE$$acosmic radiation: energy spectrum
000072033 695__ $$2INSPIRE$$aneutrino electron: elastic scattering
000072033 695__ $$2INSPIRE$$aGran Sasso
000072033 695__ $$2INSPIRE$$aexperimental results
000072033 700__ $$aAltenmüller, K.$$uMunich, Tech. U.$$vPhysik-Department and Excellence Cluster Universe, Technische Universität München, 85748 Garching, Germany
000072033 700__ $$aAppel, S.$$uMunich, Tech. U.$$vPhysik-Department and Excellence Cluster Universe, Technische Universität München, 85748 Garching, Germany
000072033 700__ $$aAtroshchenko, V.$$uKurchatov Inst., Moscow$$vNational Research Centre Kurchatov Institute, 123182 Moscow, Russia
000072033 700__ $$aBagdasarian, Z.$$uJulich, Forschungszentrum$$vIKP-2 Forschungzentrum Jülich, 52428 Jülich, Germany
000072033 700__ $$aBasilico, D.$$uINFN, Milan$$uMilan U.$$vDipartimento di Fisica, Università degli Studi e INFN, 20133 Milano, Italy
000072033 700__ $$aBellini, G.$$uINFN, Milan$$uMilan U.$$vDipartimento di Fisica, Università degli Studi e INFN, 20133 Milano, Italy
000072033 700__ $$aBenziger, J.$$uPrinceton U., Chem. Eng. Dept.$$vChemical Engineering Department, Princeton University, Princeton, NJ 08544, USA
000072033 700__ $$aBick, D.$$uHamburg U.$$vInstitut für Experimentalphysik, Universität Hamburg, 22761 Hamburg, Germany
000072033 700__ $$aBonfini, G.$$uGran Sasso$$vINFN Laboratori Nazionali del Gran Sasso, 67010 Assergi (AQ), Italy
000072033 700__ $$aBravo, D.$$uVirginia Tech.$$vPhysics Department, Virginia Polytechnic Institute and State University, Blacksburg, VA 24061, USA, Milano
000072033 700__ $$aCaccianiga, B.$$uINFN, Milan$$uMilan U.$$vDipartimento di Fisica, Università degli Studi e INFN, 20133 Milano, Italy
000072033 700__ $$aCalaprice, F.$$uPrinceton U.$$vPhysics Department, Princeton University, Princeton, NJ 08544, USA
000072033 700__ $$aCaminata, A.$$uGenoa U.$$uINFN, Genoa$$vDipartimento di Fisica, Università degli Studi e INFN, 16146 Genova, Italy
000072033 700__ $$aCaprioli, S.$$uINFN, Milan$$uMilan U.$$vDipartimento di Fisica, Università degli Studi e INFN, 20133 Milano, Italy
000072033 700__ $$aCarlini, M.$$uGran Sasso$$vINFN Laboratori Nazionali del Gran Sasso, 67010 Assergi (AQ), Italy
000072033 700__ $$aCavalcante, P.$$uGran Sasso$$vINFN Laboratori Nazionali del Gran Sasso, 67010 Assergi (AQ), Italy, Virginia
000072033 700__ $$aChepurnov, A.$$uSINP, Moscow$$vLomonosov Moscow State University Skobeltsyn Institute of Nuclear Physics, 119234 Moscow, Russia
000072033 700__ $$aChoi, K.$$uHawaii U.$$vDepartment of Physics and Astronomy, University of Hawaii, Honolulu, HI 96822, USA
000072033 700__ $$aCollica, L.$$uINFN, Milan$$uMilan U.$$vDipartimento di Fisica, Università degli Studi e INFN, 20133 Milano, Italy
000072033 700__ $$aD'Angelo, D.$$uINFN, Milan$$uMilan U.$$vDipartimento di Fisica, Università degli Studi e INFN, 20133 Milano, Italy
000072033 700__ $$aDavini, S.$$uGenoa U.$$uINFN, Genoa$$vDipartimento di Fisica, Università degli Studi e INFN, 16146 Genova, Italy
000072033 700__ $$aDerbin, A.$$uSt. Petersburg, INP$$vSt. Petersburg Nuclear Physics Institute NRC Kurchatov Institute, 188350 Gatchina, Russia
000072033 700__ $$aDing, X.F.$$uGSSI, Aquila$$vGran Sasso Science Institute (INFN), 67100 L'Aquila, Italy
000072033 700__ $$aDi Ludovico, A.$$uPrinceton U.$$vPhysics Department, Princeton University, Princeton, NJ 08544, USA
000072033 700__ $$aDi Noto, L.$$uGenoa U.$$uINFN, Genoa$$vDipartimento di Fisica, Università degli Studi e INFN, 16146 Genova, Italy
000072033 700__ $$aDrachnev, I.$$uGran Sasso$$uINFN, Trieste$$vGran Sasso Science Institute (INFN), 67100 L'Aquila, Italy, Peters
000072033 700__ $$aFomenko, K.$$uDubna, JINR$$vJoint Institute for Nuclear Research, 141980 Dubna, Russia
000072033 700__ $$aFormozov, A.$$uDubna, JINR$$vJoint Institute for Nuclear Research, 141980 Dubna, Russia, Milano, Lomonosov
000072033 700__ $$aFranco, D.$$uAPC, Paris$$vAstroParticule et Cosmologie, Université Paris Diderot, CNRS/IN2P3, CEA/IRFU, Observatoire de Paris, Sorbonne Paris Cité, 75205 Paris Cedex 13, France
000072033 700__ $$aGabriele, F.$$uGran Sasso$$vINFN Laboratori Nazionali del Gran Sasso, 67010 Assergi (AQ), Italy
000072033 700__ $$aGalbiati, C.$$uPrinceton U.$$vPhysics Department, Princeton University, Princeton, NJ 08544, USA
000072033 700__ $$aGhiano, C.$$uGran Sasso$$vINFN Laboratori Nazionali del Gran Sasso, 67010 Assergi (AQ), Italy
000072033 700__ $$aGiammarchi, M.$$uINFN, Milan$$uMilan U.$$vDipartimento di Fisica, Università degli Studi e INFN, 20133 Milano, Italy
000072033 700__ $$aGoretti, A.$$uPrinceton U.$$vPhysics Department, Princeton University, Princeton, NJ 08544, USA
000072033 700__ $$aGromov, M.$$uSINP, Moscow$$vLomonosov Moscow State University Skobeltsyn Institute of Nuclear Physics, 119234 Moscow, Russia
000072033 700__ $$aGuffanti, D.$$uGSSI, Aquila$$vGran Sasso Science Institute (INFN), 67100 L'Aquila, Italy
000072033 700__ $$aHagner, C.$$uHamburg U.$$vInstitut für Experimentalphysik, Universität Hamburg, 22761 Hamburg, Germany
000072033 700__ $$aHoudy, T.$$uAPC, Paris$$vAstroParticule et Cosmologie, Université Paris Diderot, CNRS/IN2P3, CEA/IRFU, Observatoire de Paris, Sorbonne Paris Cité, 75205 Paris Cedex 13, France
000072033 700__ $$aHungerford, E.$$uHouston U.$$vDepartment of Physics, University of Houston, Houston, TX 77204, USA
000072033 700__ $$aAldo Ianni\affiliation{INFN Laboratori Nazionali del Gran Sasso, 67010 Assergi (AQ), Italy$$uGran Sasso$$vINFN Laboratori Nazionali del Gran Sasso, 67010 Assergi (AQ), Italy
000072033 700__ $$aIanni, Andrea$$uPrinceton U.$$vPhysics Department, Princeton University, Princeton, NJ 08544, USA
000072033 700__ $$aJany, A.$$uJagiellonian U.$$vM. ~Smoluchowski Institute of Physics, Jagiellonian University, 30059 Krakow, Poland
000072033 700__ $$aJeschke, D.$$uMunich, Tech. U.$$vPhysik-Department and Excellence Cluster Universe, Technische Universität München, 85748 Garching, Germany
000072033 700__ $$aKobychev, V.$$uKiev, INR$$vKiev Institute for Nuclear Research, 03680 Kiev, Ukraine
000072033 700__ $$aKorablev, D.$$uDubna, JINR$$vJoint Institute for Nuclear Research, 141980 Dubna, Russia
000072033 700__ $$aKorga, G.$$uHouston U.$$vDepartment of Physics, University of Houston, Houston, TX 77204, USA
000072033 700__ $$aKryn, D.$$uAPC, Paris$$vAstroParticule et Cosmologie, Université Paris Diderot, CNRS/IN2P3, CEA/IRFU, Observatoire de Paris, Sorbonne Paris Cité, 75205 Paris Cedex 13, France
000072033 700__ $$aLaubenstein, M.$$uGran Sasso$$vINFN Laboratori Nazionali del Gran Sasso, 67010 Assergi (AQ), Italy
000072033 700__ $$aLitvinovich, E.$$uKurchatov Inst., Moscow$$vNational Research Centre Kurchatov Institute, 123182 Moscow, Russia, Kurchatovb
000072033 700__ $$aF.Lombardi\affiliation{INFN Laboratori Nazionali del Gran Sasso, 67010 Assergi (AQ), Italy$$uGran Sasso$$vINFN Laboratori Nazionali del Gran Sasso, 67010 Assergi (AQ), Italy
000072033 700__ $$aLombardi, P.$$uINFN, Milan$$uMilan U.$$vDipartimento di Fisica, Università degli Studi e INFN, 20133 Milano, Italy
000072033 700__ $$aLudhova, L.$$uJulich, Forschungszentrum$$uRWTH Aachen U.$$vIKP-2 Forschungzentrum Jülich, 52428 Jülich, Germany, RWTH
000072033 700__ $$aLukyanchenko, G.$$uKurchatov Inst., Moscow$$vNational Research Centre Kurchatov Institute, 123182 Moscow, Russia
000072033 700__ $$aLukyanchenko, L.$$uKurchatov Inst., Moscow$$vNational Research Centre Kurchatov Institute, 123182 Moscow, Russia
000072033 700__ $$aMachulin, I.$$uKurchatov Inst., Moscow$$vNational Research Centre Kurchatov Institute, 123182 Moscow, Russia, Kurchatovb
000072033 700__ $$aManuzio, G.$$uGenoa U.$$uINFN, Genoa$$vDipartimento di Fisica, Università degli Studi e INFN, 16146 Genova, Italy
000072033 700__ $$aMarcocci, S.$$uGran Sasso$$uINFN, Trieste$$vGran Sasso Science Institute (INFN), 67100 L'Aquila, Italy, Genova
000072033 700__ $$aMartyn, J.$$uMainz U., Inst. Phys.$$uU. Mainz, PRISMA$$vInstitute of Physics and Excellence Cluster PRISMA, Johannes Gutenberg-Universität Mainz, 55099 Mainz, Germany
000072033 700__ $$aMeroni, E.$$uINFN, Milan$$uMilan U.$$vDipartimento di Fisica, Università degli Studi e INFN, 20133 Milano, Italy
000072033 700__ $$aMeyer, M.$$uDresden, Tech. U., ITP$$vDepartment of Physics, Technische Universität Dresden, 01062 Dresden, Germany
000072033 700__ $$aMiramonti, L.$$uINFN, Milan$$uMilan U.$$vDipartimento di Fisica, Università degli Studi e INFN, 20133 Milano, Italy
000072033 700__ $$aMisiaszek, M.$$uJagiellonian U.$$vM. ~Smoluchowski Institute of Physics, Jagiellonian University, 30059 Krakow, Poland
000072033 700__ $$aMuratova, V.$$uSt. Petersburg, INP$$vSt. Petersburg Nuclear Physics Institute NRC Kurchatov Institute, 188350 Gatchina, Russia
000072033 700__ $$aNeumair, B.$$uMunich, Tech. U.$$vPhysik-Department and Excellence Cluster Universe, Technische Universität München, 85748 Garching, Germany
000072033 700__ $$aOberauer, L.$$uMunich, Tech. U.$$vPhysik-Department and Excellence Cluster Universe, Technische Universität München, 85748 Garching, Germany
000072033 700__ $$aOpitz, B.$$uHamburg U.$$vInstitut für Experimentalphysik, Universität Hamburg, 22761 Hamburg, Germany
000072033 700__ $$aOrekhov, V.$$uKurchatov Inst., Moscow$$vNational Research Centre Kurchatov Institute, 123182 Moscow, Russia
000072033 700__ $$aOrtica, F.$$uINFN, Perugia$$uPerugia U.$$vDipartimento di Chimica, Biologia e Biotecnologie, Università degli Studi e INFN, 06123 Perugia, Italy
000072033 700__ $$aPallavicini, M.$$uGenoa U.$$uINFN, Genoa$$vDipartimento di Fisica, Università degli Studi e INFN, 16146 Genova, Italy
000072033 700__ $$aPapp, L.$$uMunich, Tech. U.$$vPhysik-Department and Excellence Cluster Universe, Technische Universität München, 85748 Garching, Germany
000072033 700__ $$aPenek, Ö.$$uJulich, Forschungszentrum$$uRWTH Aachen U.$$vIKP-2 Forschungzentrum Jülich, 52428 Jülich, Germany, RWTH
000072033 700__ $$aPilipenko, N.$$uSt. Petersburg, INP$$vSt. Petersburg Nuclear Physics Institute NRC Kurchatov Institute, 188350 Gatchina, Russia
000072033 700__ $$aPocar, A.$$uMassachusetts U., Amherst$$vAmherst Center for Fundamental Interactions and Physics Department, University of Massachusetts, Amherst, MA 01003, USA
000072033 700__ $$aPorcelli, A.$$uMainz U., Inst. Phys.$$uU. Mainz, PRISMA$$vInstitute of Physics and Excellence Cluster PRISMA, Johannes Gutenberg-Universität Mainz, 55099 Mainz, Germany
000072033 700__ $$aRanucci, G.$$uINFN, Milan$$uMilan U.$$vDipartimento di Fisica, Università degli Studi e INFN, 20133 Milano, Italy
000072033 700__ $$aRazeto, A.$$uGran Sasso$$vINFN Laboratori Nazionali del Gran Sasso, 67010 Assergi (AQ), Italy
000072033 700__ $$aRe, A.$$uINFN, Milan$$uMilan U.$$vDipartimento di Fisica, Università degli Studi e INFN, 20133 Milano, Italy
000072033 700__ $$aRedchuk, M.$$uJulich, Forschungszentrum$$uRWTH Aachen U.$$vIKP-2 Forschungzentrum Jülich, 52428 Jülich, Germany, RWTH
000072033 700__ $$aRomani, A.$$uINFN, Perugia$$uPerugia U.$$vDipartimento di Chimica, Biologia e Biotecnologie, Università degli Studi e INFN, 06123 Perugia, Italy
000072033 700__ $$aRoncin, R.$$uGran Sasso$$vINFN Laboratori Nazionali del Gran Sasso, 67010 Assergi (AQ), Italy, APC
000072033 700__ $$aRossi, N.$$uGran Sasso$$vINFN Laboratori Nazionali del Gran Sasso, 67010 Assergi (AQ), Italy
000072033 700__ $$aSchönert, S.$$uMunich, Tech. U.$$vPhysik-Department and Excellence Cluster Universe, Technische Universität München, 85748 Garching, Germany
000072033 700__ $$aSemenov, D.$$uSt. Petersburg, INP$$vSt. Petersburg Nuclear Physics Institute NRC Kurchatov Institute, 188350 Gatchina, Russia
000072033 700__ $$aSkorokhvatov, M.$$uKurchatov Inst., Moscow$$vNational Research Centre Kurchatov Institute, 123182 Moscow, Russia, Kurchatovb
000072033 700__ $$aSmirnov, O.$$uDubna, JINR$$vJoint Institute for Nuclear Research, 141980 Dubna, Russia
000072033 700__ $$aSotnikov, A.$$uDubna, JINR$$vJoint Institute for Nuclear Research, 141980 Dubna, Russia
000072033 700__ $$aStokes, L.F.F.$$uGran Sasso$$vINFN Laboratori Nazionali del Gran Sasso, 67010 Assergi (AQ), Italy
000072033 700__ $$aSuvorov, Y.$$uUCLA$$vPhysics and Astronomy Department, University of California Los Angeles (UCLA), Los Angeles, California 90095, USA, Kurchatov
000072033 700__ $$aTartaglia, R.$$uGran Sasso$$vINFN Laboratori Nazionali del Gran Sasso, 67010 Assergi (AQ), Italy
000072033 700__ $$aTestera, G.$$uGenoa U.$$uINFN, Genoa$$vDipartimento di Fisica, Università degli Studi e INFN, 16146 Genova, Italy
000072033 700__ $$aThurn, J.$$uDresden, Tech. U., ITP$$vDepartment of Physics, Technische Universität Dresden, 01062 Dresden, Germany
000072033 700__ $$aToropova, M.$$uKurchatov Inst., Moscow$$vNational Research Centre Kurchatov Institute, 123182 Moscow, Russia
000072033 700__ $$aUnzhakov, E.$$uSt. Petersburg, INP$$vSt. Petersburg Nuclear Physics Institute NRC Kurchatov Institute, 188350 Gatchina, Russia
000072033 700__ $$aVishneva, A.$$uDubna, JINR$$vJoint Institute for Nuclear Research, 141980 Dubna, Russia
000072033 700__ $$aVogelaar, R.B.$$uVirginia Tech.$$vPhysics Department, Virginia Polytechnic Institute and State University, Blacksburg, VA 24061, USA
000072033 700__ $$avon Feilitzsch, F.$$uMunich, Tech. U.$$vPhysik-Department and Excellence Cluster Universe, Technische Universität München, 85748 Garching, Germany
000072033 700__ $$aWang, H.$$uUCLA$$vPhysics and Astronomy Department, University of California Los Angeles (UCLA), Los Angeles, California 90095, USA
000072033 700__ $$aWeinz, S.$$uMainz U., Inst. Phys.$$uU. Mainz, PRISMA$$vInstitute of Physics and Excellence Cluster PRISMA, Johannes Gutenberg-Universität Mainz, 55099 Mainz, Germany
000072033 700__ $$aWojcik, M.$$uJagiellonian U.$$vM. ~Smoluchowski Institute of Physics, Jagiellonian University, 30059 Krakow, Poland
000072033 700__ $$aWurm, M.$$uMainz U., Inst. Phys.$$uU. Mainz, PRISMA$$vInstitute of Physics and Excellence Cluster PRISMA, Johannes Gutenberg-Universität Mainz, 55099 Mainz, Germany
000072033 700__ $$aYokley, Z.$$uVirginia Tech.$$vPhysics Department, Virginia Polytechnic Institute and State University, Blacksburg, VA 24061, USA
000072033 700__ $$aZaimidoroga, O.$$uDubna, JINR$$vJoint Institute for Nuclear Research, 141980 Dubna, Russia
000072033 700__ $$aZavatarelli, S.$$uGenoa U.$$uINFN, Genoa$$vDipartimento di Fisica, Università degli Studi e INFN, 16146 Genova, Italy
000072033 700__ $$aZuber, K.$$uDresden, Tech. U., ITP$$vDepartment of Physics, Technische Universität Dresden, 01062 Dresden, Germany
000072033 700__ $$aZuzel, G.$$uJagiellonian U.$$vM. ~Smoluchowski Institute of Physics, Jagiellonian University, 30059 Krakow, Poland
000072033 710__ $$gBorexino
000072033 8564_ $$s19170$$uhttp://inspirehep.net/record/1621429/files/fig_map.png$$y00000 Relative  variation [\%], from Monte Carlo simulations, of the light yield with respect to the detector center, as function of the event reconstructed position (z vs R$_{xy}$=$\sqrt{x^2+y^2}$). The correspondent systematic error was estimated  in $\sigma$=1.9\%, using $^{241}$Am-$^9$Be calibration data.
000072033 8564_ $$s21510$$uhttp://inspirehep.net/record/1621429/files/fig_intshapes.png$$y00008 Comparison of the radial distributions from unoscillated and oscillated neutrinos in the LE and HE ranges. Oscillated and unoscillated spectra are almost indistinguishable, confirming the negligible dependence of the radial distribution on the energy spectrum. The MSW-LMA parameters used for simulating oscillating neutrinos are $\Delta$m$^2$=7.50$\times$10$^{-5}$~eV$^2$, sin$^2$($\theta_{12}$)=0.306, and sin$^2$($\theta_{13}$)=0.02166~\cite{Esteban:2016qun}.
000072033 8564_ $$s23495$$uhttp://inspirehep.net/record/1621429/files/fig_radialfitHE.png$$y00009 Fit of the event radial distribution in the HE range, [2950, 8500] p.e..
000072033 8564_ $$s28951$$uhttp://inspirehep.net/record/1621429/files/fig_radialfitLE.png$$y00010 Fit of the event radial distribution in the LE range, [1650, 2950] p.e..
000072033 8564_ $$s3859$$uhttp://inspirehep.net/record/1621429/files/fig_energy.png$$y00002 Energy spectrum of residual events after selection cuts in the LE (red) and HE (blue) ranges.  A z-cut at 2.5~m is applied to the LE region (see text) causing the step in the number of selected events visible at 2950 pe.  No events are found in the HE sub-range [6000, 8500] p.e..
000072033 8564_ $$s4023$$uhttp://inspirehep.net/record/1621429/files/fig_externals.png$$y00005 Radial distribution of $^8$B candidates (black dots) compared with the Monte Carlo (red) one for events with Q$>$2950 pe ($\sim$5MeV).  The excess at large radii is an indication for the additional high energy external background component induced by radiogenic neutron captures on detector materials.
000072033 8564_ $$s40268$$uhttp://inspirehep.net/record/1621429/files/fig_neutrons.png$$y00006 Predicted energy spectra and fluxes of neutrons produced via ($\alpha$, n) reactions and spontaneous fissions,  from  $^{238}$U, $^{235}$U, and $^{232}$Th contaminations in SSS and in PMT glasses.
000072033 8564_ $$s4131$$uhttp://inspirehep.net/record/1621429/files/fig_peeLZ.png$$y00013 Electron neutrino survival probability as function of the neutrino energy and Borexino measurements, assuming  the low-Z B16(AGSS09met) SSM  \cite{Vinyoles:2016djt, Asplund:2009fu}. Color codes and explanation are the same of Figure \ref{fig:peeHZ}.
000072033 8564_ $$s4203$$uhttp://inspirehep.net/record/1621429/files/fig_peeHZ.png$$y00012 Electron neutrino survival probability as function of the neutrino energy, evaluated for the $^8$B neutrino source assuming the high-Z B16(GS98) SSM  \cite{Vinyoles:2016djt, Grevesse1998} and the flavor conversion parameters from the MSW-LMA solution ($\Delta$m$_{12}^2$=7.50$\times$10$^{-5}$ eV$^2$,  tan$^2\theta_{12}$=0.441, and  tan$^2\theta_{13}$=0.022 \cite{Esteban:2016qun}). Dots represent the Borexino results from $pp$ (red), $^7$Be (blue), $pep$ (azure),  and $^8$B neutrino measurements (black for the LE+HE range, and grey for the separate sub-ranges). $pp$ and $^8$B dots are set at the mean energy of detected neutrinos, weighted on the detection range in electron recoil energy.  The error bars include experimental and theoretical uncertainties.
000072033 8564_ $$s4737$$uhttp://inspirehep.net/record/1621429/files/fig_thresholds.png$$y00001 Detection efficiencies and associated uncertainties (due to the electron energy scale determination) of the LE ([1650, 2950] p.e., red line) and HE ([2950, 8500] p.e., blue line) ranges as a function of electron energy.  The detection efficiency equals 1 up to the 8500 p.e. upper edge of the HE range.
000072033 8564_ $$s5703$$uhttp://inspirehep.net/record/1621429/files/fig_bi212.png$$y00004 Radial distributions of $^{212}$Bi events occurring in the scintillator, selected with the fast $^{212}$BiPo coincidences, with no energy degradation for the $\alpha$ decay (black dots). A uniform bulk distribution of simulated $^{212}$Bi events is shown in red. The difference (green) between the two spectra corresponds to $^{212}$Bi events resulting from emanation and diffusion from the nylon vessel. The distribution of \textit{emanation} $^{208}$Tl is shown in blue. The $^{212}$Bi distribution (mostly a pure $\beta$ decay, $Q=2.25$ MeV) is wider than that of $^{208}$Tl ($\beta+\gamma$ decay, $Q=5$ MeV) due to poorer spatial resolution at lower energy. See text for details.
000072033 8564_ $$s8174$$uhttp://inspirehep.net/record/1621429/files/fig_neutrinos.png$$y00011 The $^8$B neutrino energy spectrum (black) and the portions of the same spectrum contributing to the LE (red), HE (blue), and LE+HE (green) energy windows used in this analysis.  No flavor transformation is assumed. The error bands are obtained by combining statistical and systematic uncertainties of the measured rates.
000072033 8564_ $$s8690$$uhttp://inspirehep.net/record/1621429/files/fig_tl208radial.png$$y00003 Radial distributions of simulated $^8$B $\nu$ events and $^{208}$Tl decays, with [1650, 2950] p.e. energy cut. The two spectra are normalized to the number of reconstructed events.  The difference is due to $^{208}$Tl emission $\gamma$-rays, escaping the scintillator.
000072033 8564_ $$s9740$$uhttp://inspirehep.net/record/1621429/files/fig_extshapes.png$$y00007 Reconstructed radial distributions of  simulated events with energy falling in  the LE range and generated by neutron captures on carbon in the buffer (red), and on iron in the SSS (black).
000072033 8564_ $$s812860$$uhttp://inspirehep.net/record/1621429/files/arXiv:1709.00756.pdf
000072033 909CO $$ooai:inspirehep.net:1621429$$pINSPIRE:HEP
000072033 980__ $$aCORE
000072033 980__ $$aarXiv
000072033 980__ $$aCiteable
000072033 980__ $$aHEP
000072033 999C6 $$a0-1-1-1-0-0-0$$t2017-09-05 07:57:02$$vInvenio/1.1.2.1260-aa76f refextract/1.5.44$$vcontent.pdf;1
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