000875085 001__ 875085
000875085 005__ 20230217124236.0
000875085 0247_ $$2doi$$a10.1103/PhysRevD.101.062001
000875085 0247_ $$2ISSN$$a0556-2821
000875085 0247_ $$2ISSN$$a1089-4918
000875085 0247_ $$2ISSN$$a1538-4500
000875085 0247_ $$2ISSN$$a1550-2368
000875085 0247_ $$2ISSN$$a1550-7998
000875085 0247_ $$2ISSN$$a2470-0010
000875085 0247_ $$2ISSN$$a2470-0029
000875085 0247_ $$2Handle$$a2128/24743
000875085 0247_ $$2altmetric$$aaltmetric:77152777
000875085 0247_ $$2WOS$$aWOS:000518459600001
000875085 037__ $$aFZJ-2020-01794
000875085 041__ $$aEnglish
000875085 082__ $$a530
000875085 1001_ $$0P:(DE-HGF)0$$aAgostini, M.$$b0
000875085 245__ $$aImproved measurement of B 8 solar neutrinos with 1.5 kt · y of Borexino exposure
000875085 260__ $$aMelville, NY$$c2020
000875085 264_1 $$2Crossref$$3online$$bAmerican Physical Society (APS)$$c2020-03-06
000875085 264_1 $$2Crossref$$3print$$bAmerican Physical Society (APS)$$c2020-03-01
000875085 3367_ $$2DRIVER$$aarticle
000875085 3367_ $$2DataCite$$aOutput Types/Journal article
000875085 3367_ $$0PUB:(DE-HGF)16$$2PUB:(DE-HGF)$$aJournal Article$$bjournal$$mjournal$$s1588172204_364
000875085 3367_ $$2BibTeX$$aARTICLE
000875085 3367_ $$2ORCID$$aJOURNAL_ARTICLE
000875085 3367_ $$00$$2EndNote$$aJournal Article
000875085 520__ $$aWe report on an improved measurement of the 8B solar neutrino interaction rate with the Borexino experiment at the Laboratori Nazionali del Gran Sasso. Neutrinos are detected via their elastic scattering on electrons in a large volume of liquid scintillator. The measured rate of scattered electrons above 3 MeV of energy is 0.223+0.015−0.016(stat)+0.006−0.006(syst) cpd/100 t, which corresponds to an observed solar neutrino flux assuming no neutrino flavor conversion of Φ^{ES}_{8B}=2.57+0.17−0.18(stat)+0.07−0.07(syst)×10^6 cm−2s−1. This measurement exploits the active volume of the detector in almost its entirety for the first time, and takes advantage of a reduced radioactive background following the 2011 scintillator purification campaign and of novel analysis tools providing a more precise modeling of the background. Additionally, we set a new limit on the interaction rate of solar hep neutrinos, searched via their elastic scattering on electrons as well as their neutral current-mediated inelastic scattering on carbon, 12C(ν,ν′) 12C* (Eγ= 15.1 MeV).
000875085 536__ $$0G:(DE-HGF)POF3-612$$a612 - Cosmic Matter in the Laboratory (POF3-612)$$cPOF3-612$$fPOF III$$x0
000875085 542__ $$2Crossref$$i2020-03-06$$uhttps://creativecommons.org/licenses/by/4.0/
000875085 588__ $$aDataset connected to CrossRef
000875085 65027 $$0V:(DE-MLZ)SciArea-230$$2V:(DE-HGF)$$aParticle Physics$$x0
000875085 65027 $$0V:(DE-MLZ)SciArea-200$$2V:(DE-HGF)$$aNuclear Physics$$x1
000875085 65017 $$0V:(DE-MLZ)GC-2001-2016$$2V:(DE-HGF)$$aNuclei and Particles$$x0
000875085 65017 $$0V:(DE-MLZ)GC-2004-2016$$2V:(DE-HGF)$$aBasic research$$x1
000875085 7001_ $$0P:(DE-HGF)0$$aAltenmüller, K.$$b1
000875085 7001_ $$0P:(DE-HGF)0$$aAppel, S.$$b2
000875085 7001_ $$0P:(DE-HGF)0$$aAtroshchenko, V.$$b3
000875085 7001_ $$0P:(DE-Juel1)156420$$aBagdasarian, Z.$$b4
000875085 7001_ $$0P:(DE-HGF)0$$aBasilico, D.$$b5
000875085 7001_ $$0P:(DE-HGF)0$$aBellini, G.$$b6
000875085 7001_ $$0P:(DE-HGF)0$$aBenziger, J.$$b7
000875085 7001_ $$0P:(DE-HGF)0$$aBick, D.$$b8
000875085 7001_ $$0P:(DE-HGF)0$$aBravo, D.$$b9
000875085 7001_ $$0P:(DE-HGF)0$$aCaccianiga, B.$$b10
000875085 7001_ $$0P:(DE-HGF)0$$aCalaprice, F.$$b11
000875085 7001_ $$0P:(DE-HGF)0$$aCaminata, A.$$b12
000875085 7001_ $$0P:(DE-HGF)0$$aCavalcante, P.$$b13
000875085 7001_ $$0P:(DE-HGF)0$$aChepurnov, A.$$b14
000875085 7001_ $$0P:(DE-HGF)0$$aD’Angelo, D.$$b15
000875085 7001_ $$0P:(DE-HGF)0$$aDavini, S.$$b16
000875085 7001_ $$0P:(DE-HGF)0$$aDerbin, A.$$b17
000875085 7001_ $$0P:(DE-HGF)0$$aDi Giacinto, A.$$b18
000875085 7001_ $$0P:(DE-HGF)0$$aDi Marcello, V.$$b19
000875085 7001_ $$0P:(DE-HGF)0$$aDing, X. F.$$b20
000875085 7001_ $$0P:(DE-HGF)0$$aDi Ludovico, A.$$b21
000875085 7001_ $$0P:(DE-HGF)0$$aDi Noto, L.$$b22
000875085 7001_ $$0P:(DE-HGF)0$$aDrachnev, I.$$b23
000875085 7001_ $$0P:(DE-HGF)0$$aFormozov, A.$$b24
000875085 7001_ $$00000-0001-5604-2531$$aFranco, D.$$b25
000875085 7001_ $$0P:(DE-HGF)0$$aGalbiati, C.$$b26
000875085 7001_ $$0P:(DE-HGF)0$$aGschwender, M.$$b27
000875085 7001_ $$0P:(DE-HGF)0$$aGhiano, C.$$b28
000875085 7001_ $$0P:(DE-HGF)0$$aGiammarchi, M.$$b29
000875085 7001_ $$0P:(DE-HGF)0$$aGoretti, A.$$b30
000875085 7001_ $$0P:(DE-HGF)0$$aGromov, M.$$b31
000875085 7001_ $$0P:(DE-HGF)0$$aGuffanti, D.$$b32
000875085 7001_ $$0P:(DE-HGF)0$$aHagner, C.$$b33
000875085 7001_ $$0P:(DE-HGF)0$$aHoudy, T.$$b34
000875085 7001_ $$0P:(DE-HGF)0$$aHungerford, E.$$b35
000875085 7001_ $$0P:(DE-HGF)0$$aIanni, Aldo$$b36
000875085 7001_ $$0P:(DE-HGF)0$$aIanni, Andrea$$b37
000875085 7001_ $$0P:(DE-HGF)0$$aJany, A.$$b38
000875085 7001_ $$0P:(DE-HGF)0$$aJeschke, D.$$b39
000875085 7001_ $$0P:(DE-HGF)0$$aKobychev, V.$$b40
000875085 7001_ $$0P:(DE-HGF)0$$aKorga, G.$$b41
000875085 7001_ $$0P:(DE-Juel1)173900$$aKumaran, Sindhujha$$b42
000875085 7001_ $$0P:(DE-HGF)0$$aLachenmaier, T.$$b43
000875085 7001_ $$0P:(DE-HGF)0$$aLaubenstein, M.$$b44
000875085 7001_ $$0P:(DE-HGF)0$$aLitvinovich, E.$$b45
000875085 7001_ $$0P:(DE-HGF)0$$aLombardi, P.$$b46
000875085 7001_ $$0P:(DE-HGF)0$$aLomskaya, I.$$b47
000875085 7001_ $$0P:(DE-Juel1)168122$$aLudhova, Livia$$b48$$eCorresponding author
000875085 7001_ $$0P:(DE-HGF)0$$aLukyanchenko, G.$$b49
000875085 7001_ $$0P:(DE-HGF)0$$aLukyanchenko, L.$$b50
000875085 7001_ $$0P:(DE-HGF)0$$aMachulin, I.$$b51
000875085 7001_ $$0P:(DE-HGF)0$$aMarcocci, S.$$b52
000875085 7001_ $$0P:(DE-HGF)0$$aMartyn, J.$$b53
000875085 7001_ $$0P:(DE-HGF)0$$aMeroni, E.$$b54
000875085 7001_ $$0P:(DE-HGF)0$$aMeyer, M.$$b55
000875085 7001_ $$0P:(DE-HGF)0$$aMiramonti, L.$$b56
000875085 7001_ $$0P:(DE-HGF)0$$aMisiaszek, M.$$b57
000875085 7001_ $$0P:(DE-HGF)0$$aMuratova, V.$$b58
000875085 7001_ $$0P:(DE-HGF)0$$aNeumair, B.$$b59
000875085 7001_ $$0P:(DE-HGF)0$$aNieslony, M.$$b60
000875085 7001_ $$0P:(DE-HGF)0$$aNugmanov, R.$$b61
000875085 7001_ $$0P:(DE-HGF)0$$aOberauer, L.$$b62
000875085 7001_ $$0P:(DE-HGF)0$$aOrekhov, V.$$b63
000875085 7001_ $$0P:(DE-HGF)0$$aOrtica, F.$$b64
000875085 7001_ $$0P:(DE-HGF)0$$aPallavicini, M.$$b65
000875085 7001_ $$0P:(DE-HGF)0$$aPapp, L.$$b66
000875085 7001_ $$0P:(DE-Juel1)171602$$aPenek, Ömer$$b67
000875085 7001_ $$0P:(DE-HGF)0$$aPietrofaccia, L.$$b68
000875085 7001_ $$0P:(DE-HGF)0$$aPilipenko, N.$$b69
000875085 7001_ $$0P:(DE-HGF)0$$aPocar, A.$$b70
000875085 7001_ $$0P:(DE-HGF)0$$aRaikov, G.$$b71
000875085 7001_ $$0P:(DE-HGF)0$$aRanalli, M. T.$$b72
000875085 7001_ $$0P:(DE-HGF)0$$aRanucci, G.$$b73$$eCorresponding author
000875085 7001_ $$0P:(DE-HGF)0$$aRazeto, A.$$b74
000875085 7001_ $$0P:(DE-HGF)0$$aRe, A.$$b75
000875085 7001_ $$0P:(DE-Juel1)171322$$aRedchuk, Mariia$$b76
000875085 7001_ $$0P:(DE-HGF)0$$aRomani, A.$$b77
000875085 7001_ $$0P:(DE-HGF)0$$aRossi, N.$$b78
000875085 7001_ $$0P:(DE-HGF)0$$aRottenanger, S.$$b79
000875085 7001_ $$0P:(DE-HGF)0$$aSchönert, S.$$b80
000875085 7001_ $$0P:(DE-HGF)0$$aSemenov, D.$$b81
000875085 7001_ $$0P:(DE-HGF)0$$aSkorokhvatov, M.$$b82
000875085 7001_ $$0P:(DE-HGF)0$$aSmirnov, O.$$b83
000875085 7001_ $$0P:(DE-HGF)0$$aSotnikov, A.$$b84
000875085 7001_ $$0P:(DE-HGF)0$$aSuvorov, Y.$$b85
000875085 7001_ $$0P:(DE-HGF)0$$aTartaglia, R.$$b86
000875085 7001_ $$0P:(DE-HGF)0$$aTestera, G.$$b87
000875085 7001_ $$0P:(DE-HGF)0$$aThurn, J.$$b88
000875085 7001_ $$0P:(DE-HGF)0$$aUnzhakov, E.$$b89
000875085 7001_ $$0P:(DE-HGF)0$$aVishneva, A.$$b90
000875085 7001_ $$0P:(DE-HGF)0$$aVogelaar, R. B.$$b91
000875085 7001_ $$0P:(DE-HGF)0$$avon Feilitzsch, F.$$b92
000875085 7001_ $$0P:(DE-HGF)0$$aWojcik, M.$$b93
000875085 7001_ $$0P:(DE-HGF)0$$aWurm, M.$$b94
000875085 7001_ $$0P:(DE-HGF)0$$aZavatarelli, S.$$b95
000875085 7001_ $$0P:(DE-HGF)0$$aZuber, K.$$b96
000875085 7001_ $$0P:(DE-HGF)0$$aZuzel, G.$$b97
000875085 77318 $$2Crossref$$3journal-article$$a10.1103/physrevd.101.062001$$bAmerican Physical Society (APS)$$d2020-03-06$$n6$$p062001$$tPhysical Review D$$v101$$x2470-0010$$y2020
000875085 773__ $$0PERI:(DE-600)2844732-3$$a10.1103/PhysRevD.101.062001$$gVol. 101, no. 6, p. 062001$$n6$$p062001$$tPhysical review / D$$v101$$x2470-0010$$y2020
000875085 8564_ $$uhttps://juser.fz-juelich.de/record/875085/files/PhysRevD.101.062001.pdf$$yOpenAccess
000875085 8564_ $$uhttps://juser.fz-juelich.de/record/875085/files/PhysRevD.101.062001.pdf?subformat=pdfa$$xpdfa$$yOpenAccess
000875085 909CO $$ooai:juser.fz-juelich.de:875085$$pdnbdelivery$$pdriver$$pVDB$$popen_access$$popenaire
000875085 9101_ $$0I:(DE-588b)5008462-8$$6P:(DE-Juel1)156420$$aForschungszentrum Jülich$$b4$$kFZJ
000875085 9101_ $$0I:(DE-588b)5008462-8$$6P:(DE-Juel1)173900$$aForschungszentrum Jülich$$b42$$kFZJ
000875085 9101_ $$0I:(DE-588b)36225-6$$6P:(DE-Juel1)173900$$aRWTH Aachen$$b42$$kRWTH
000875085 9101_ $$0I:(DE-588b)5008462-8$$6P:(DE-Juel1)168122$$aForschungszentrum Jülich$$b48$$kFZJ
000875085 9101_ $$0I:(DE-588b)36225-6$$6P:(DE-Juel1)168122$$aRWTH Aachen$$b48$$kRWTH
000875085 9101_ $$0I:(DE-588b)5008462-8$$6P:(DE-Juel1)171602$$aForschungszentrum Jülich$$b67$$kFZJ
000875085 9101_ $$0I:(DE-588b)36225-6$$6P:(DE-Juel1)171602$$aRWTH Aachen$$b67$$kRWTH
000875085 9101_ $$0I:(DE-588b)5008462-8$$6P:(DE-Juel1)171322$$aForschungszentrum Jülich$$b76$$kFZJ
000875085 9101_ $$0I:(DE-588b)36225-6$$6P:(DE-Juel1)171322$$aRWTH Aachen$$b76$$kRWTH
000875085 9131_ $$0G:(DE-HGF)POF3-612$$1G:(DE-HGF)POF3-610$$2G:(DE-HGF)POF3-600$$3G:(DE-HGF)POF3$$4G:(DE-HGF)POF$$aDE-HGF$$bForschungsbereich Materie$$lMaterie und Universum$$vCosmic Matter in the Laboratory$$x0
000875085 9141_ $$y2020
000875085 915__ $$0StatID:(DE-HGF)0200$$2StatID$$aDBCoverage$$bSCOPUS
000875085 915__ $$0LIC:(DE-HGF)CCBY4$$2HGFVOC$$aCreative Commons Attribution CC BY 4.0
000875085 915__ $$0StatID:(DE-HGF)0600$$2StatID$$aDBCoverage$$bEbsco Academic Search
000875085 915__ $$0StatID:(DE-HGF)0100$$2StatID$$aJCR$$bPHYS REV D : 2016
000875085 915__ $$0StatID:(DE-HGF)0150$$2StatID$$aDBCoverage$$bWeb of Science Core Collection
000875085 915__ $$0StatID:(DE-HGF)0110$$2StatID$$aWoS$$bScience Citation Index
000875085 915__ $$0StatID:(DE-HGF)0111$$2StatID$$aWoS$$bScience Citation Index Expanded
000875085 915__ $$0StatID:(DE-HGF)9900$$2StatID$$aIF < 5
000875085 915__ $$0StatID:(DE-HGF)0510$$2StatID$$aOpenAccess
000875085 915__ $$0StatID:(DE-HGF)0030$$2StatID$$aPeer Review$$bASC
000875085 915__ $$0StatID:(DE-HGF)1150$$2StatID$$aDBCoverage$$bCurrent Contents - Physical, Chemical and Earth Sciences
000875085 915__ $$0StatID:(DE-HGF)0300$$2StatID$$aDBCoverage$$bMedline
000875085 915__ $$0StatID:(DE-HGF)0199$$2StatID$$aDBCoverage$$bClarivate Analytics Master Journal List
000875085 915__ $$0StatID:(DE-HGF)0570$$2StatID$$aSCOAP3
000875085 920__ $$lyes
000875085 9201_ $$0I:(DE-Juel1)IKP-2-20111104$$kIKP-2$$lExperimentelle Hadrondynamik$$x0
000875085 980__ $$ajournal
000875085 980__ $$aVDB
000875085 980__ $$aUNRESTRICTED
000875085 980__ $$aI:(DE-Juel1)IKP-2-20111104
000875085 9801_ $$aFullTexts
000875085 999C5 $$2Crossref$$9-- missing cx lookup --$$a10.1038/s41586-018-0624-y
000875085 999C5 $$2Crossref$$9-- missing cx lookup --$$a10.1103/PhysRevLett.101.091302
000875085 999C5 $$2Crossref$$9-- missing cx lookup --$$a10.1103/PhysRevLett.108.051302
000875085 999C5 $$2Crossref$$9-- missing cx lookup --$$a10.1038/nature13702
000875085 999C5 $$2Crossref$$9-- missing cx lookup --$$a10.1103/PhysRevD.89.112007
000875085 999C5 $$2Crossref$$9-- missing cx lookup --$$a10.1103/PhysRevD.82.033006
000875085 999C5 $$2Crossref$$9-- missing cx lookup --$$a10.3847/1538-4357/835/2/202
000875085 999C5 $$1S. P. Mikheev$$2Crossref$$oS. P. Mikheev 1985$$y1985
000875085 999C5 $$1S. P. Mikheev$$2Crossref$$oS. P. Mikheev 1985$$y1985
000875085 999C5 $$2Crossref$$9-- missing cx lookup --$$a10.1103/PhysRevD.17.2369
000875085 999C5 $$2Crossref$$9-- missing cx lookup --$$a10.1088/1748-0221/6/05/P05005
000875085 999C5 $$2Crossref$$9-- missing cx lookup --$$a10.1016/j.nima.2008.11.076
000875085 999C5 $$2Crossref$$9-- missing cx lookup --$$a10.1088/1748-0221/7/10/P10018
000875085 999C5 $$2Crossref$$9-- missing cx lookup --$$a10.1016/j.astropartphys.2017.10.003
000875085 999C5 $$2Crossref$$9-- missing cx lookup --$$a10.1088/1475-7516/2013/08/049
000875085 999C5 $$2Crossref$$9-- missing cx lookup --$$a10.1016/j.nima.2007.09.036
000875085 999C5 $$2Crossref$$9-- missing cx lookup --$$a10.1103/PhysRevC.81.025807
000875085 999C5 $$2Crossref$$9-- missing cx lookup --$$a10.1016/S0927-6505(00)00103-1
000875085 999C5 $$2Crossref$$9-- missing cx lookup --$$a10.1103/PhysRevC.71.055805
000875085 999C5 $$2Crossref$$9-- missing cx lookup --$$a10.1016/S0927-6505(01)00179-7
000875085 999C5 $$2Crossref$$9-- missing cx lookup --$$a10.1016/j.nima.2017.12.047
000875085 999C5 $$2Crossref$$9-- missing cx lookup --$$a10.1016/S0168-9002(97)00048-X
000875085 999C5 $$1A. J. Koning$$2Crossref$$9-- missing cx lookup --$$a10.1051/ndata:07767$$y2008
000875085 999C5 $$2Crossref$$9-- missing cx lookup --$$a10.1016/j.nima.2017.09.007
000875085 999C5 $$2Crossref$$9-- missing cx lookup --$$a10.1103/PhysRev.89.1288
000875085 999C5 $$2Crossref$$9-- missing cx lookup --$$a10.1016/S0168-583X(00)00694-7
000875085 999C5 $$2Crossref$$9-- missing cx lookup --$$a10.1103/PhysRevC.73.025503
000875085 999C5 $$2Crossref$$9-- missing cx lookup --$$a10.1007/JHEP01(2017)087
000875085 999C5 $$2Crossref$$9-- missing cx lookup --$$a10.1103/PhysRevD.94.052010
000875085 999C5 $$2Crossref$$9-- missing cx lookup --$$a10.1023/A:1005161325181
000875085 999C5 $$2Crossref$$9-- missing cx lookup --$$a10.1103/PhysRevD.73.112001
000875085 999C5 $$2Crossref$$9-- missing cx lookup --$$a10.1086/508768
000875085 999C5 $$2Crossref$$9-- missing cx lookup --$$a10.1016/j.astropartphys.2016.10.004
000875085 999C5 $$2Crossref$$9-- missing cx lookup --$$a10.1016/j.nima.2009.12.009
000875085 999C5 $$2Crossref$$9-- missing cx lookup --$$a10.1103/PhysRevD.92.023004
000875085 999C5 $$2Crossref$$9-- missing cx lookup --$$a10.1016/j.astropartphys.2005.03.006
000875085 999C5 $$2Crossref$$9-- missing cx lookup --$$a10.1103/PhysRevD.57.3873