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000838451 0247_ $$2doi$$a10.1088/1742-6596/798/1/012114
000838451 0247_ $$2ISSN$$a1742-6588
000838451 0247_ $$2ISSN$$a1742-6596
000838451 0247_ $$2Handle$$a2128/15631
000838451 0247_ $$2WOS$$aWOS:000403476900114
000838451 037__ $$aFZJ-2017-07054
000838451 041__ $$aEnglish
000838451 082__ $$a530
000838451 1001_ $$0P:(DE-HGF)0$$aJeschke, D.$$b0$$eCorresponding author
000838451 1112_ $$a2nd International Conference on Particle Physics and Astrophysics$$cMoscow$$d2016-10-10 - 2016-10-14$$gICPPA 2016$$wRussia
000838451 245__ $$aRecent Results from Borexino
000838451 260__ $$aBristol$$bIOP Publ.$$c2017
000838451 300__ $$a2 - 6
000838451 3367_ $$2ORCID$$aCONFERENCE_PAPER
000838451 3367_ $$033$$2EndNote$$aConference Paper
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000838451 3367_ $$0PUB:(DE-HGF)8$$2PUB:(DE-HGF)$$aContribution to a conference proceedings$$bcontrib$$mcontrib$$s1508320966_25974
000838451 520__ $$aThe Borexino experiment is taking data since 2007 at the Laboratori Nazionali del Gran Sasso in Italy accomplishing outstanding achievements in the field of neutrino physics. Its success is strongly based on the unprecedented ultra-high radio-purity of the inner scintillator core. The main features of the detector and the impressive results for solar and geo-neutrinos obtained by Borexino so far are summarized. The main focus is laid on the most recent results, i.e. the first real-time measurement of the solar pp neutrino flux and the detection of the signal induced by geo-neutrinos with a significance as high as 5.9σ. The measurement of the pp neutrino flux represents a direct probe of the major mechanism of energy production in the Sun and its observation at a significance of 10σ proves the stability of the Sun over a time of at least 105 years. It further puts Borexino in the unique position of being capable to test the MSW-LMA paradigm across the whole solar energy range. The geo-neutrino data allow to infer information concerning important geophysical properties of the Earth that are also discussed. The perspectives of the final stage of the Borexino solar neutrino program that are centered on the goal of measuring the CNO neutrinos that so far escaped any observation are outlined.
000838451 536__ $$0G:(DE-HGF)POF3-612$$a612 - Cosmic Matter in the Laboratory (POF3-612)$$cPOF3-612$$fPOF III$$x0
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000838451 7001_ $$aBellini, G.$$b5
000838451 7001_ $$aBenziger, J.$$b6
000838451 7001_ $$aBick, D.$$b7
000838451 7001_ $$aBonfini, G.$$b8
000838451 7001_ $$aBravo, D.$$b9
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000838451 7001_ $$aJeschke, D.$$b38
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000838451 7001_ $$avon Feilitzsch, F.$$b88
000838451 7001_ $$aWang, H.$$b89
000838451 7001_ $$aWeinz, S.$$b90
000838451 7001_ $$aWinter, J.$$b91
000838451 7001_ $$aWojcik, M.$$b92
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000838451 773__ $$0PERI:(DE-600)2166409-2$$a10.1088/1742-6596/798/1/012114$$gVol. 798, p. 012114 -$$p012114 -$$tJournal of physics / Conference Series$$v798$$x1742-6596$$y2017
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