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001     315081
005     20211110140030.0
020 _ _ |a 978-3-945931-08-0
024 7 _ |2 datacite_doi
|a 10.3204/DESY-PROC-2016-05/30
024 7 _ |2 ISSN
|a 1435-8077
037 _ _ |a PUBDB-2016-05616
041 _ _ |a English
100 1 _ |0 P:(DE-HGF)0
|a Marcocci, S.
|b 0
111 2 _ |0 C16-03-17
|2 inspire
|a Magellan Workshop
|c Hamburg
|d 2016-03-17 - 2016-03-18
|w Germany
245 _ _ |a Measurement of solar neutrino fluxes with Borexino
260 _ _ |a Hamburg
|b Verlag Deutsches Elektronen-Synchrotron
|c 2016
295 1 0 |a "Measurement of solar neutrino fluxes with Borexino" in Proceedings, Magellan Workshop: Connecting Neutrino Physics and Astronomy / Dahmke, Stefan K.G., Meyer, Mikko, Vanhoefer, Laura (eds.), Deutsches Elektronen-Synchrotron, DESY : 2016 ; Magellan Workshop, 2016-03-17 - 2016-03-18, Hamburg
300 _ _ |a 95-104
336 7 _ |2 ORCID
|a CONFERENCE_PAPER
336 7 _ |0 33
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|a Conference Paper
336 7 _ |2 BibTeX
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490 0 _ |0 PERI:(DE-600)2450075-6
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520 _ _ |a Solar neutrinos have been of extraordinary importance for the discovery of neutrino oscillations and allow to study directly the Sun's innermost core. The Borexino experiment, located in the Gran Sasso National Laboratory, is an ultra-pure liquid scintillator detector conceived for the real time spectroscopy of low energy solar neutrinos. We review Borexino's results and we discuss its upcoming future, since the precision era of solar neutrino measurements has just started.
536 _ _ |0 G:(EU-Grant)320873
|a SOX - SOX: Short distance neutrino Oscillations with BoreXino (320873)
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|t Proceedings, Magellan Workshop: Connecting Neutrino Physics and Astronomy: Hamburg, Germany, March 17-18, 2016
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|b 81
910 1 _ |0 I:(DE-HGF)0
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|b 82
910 1 _ |0 I:(DE-HGF)0
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|b 82
910 1 _ |0 I:(DE-HGF)0
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|b 83
910 1 _ |0 I:(DE-HGF)0
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|b 84
910 1 _ |0 I:(DE-HGF)0
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910 1 _ |0 I:(DE-HGF)0
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|b 87
910 1 _ |0 I:(DE-HGF)0
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|b 88
910 1 _ |0 I:(DE-HGF)0
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910 1 _ |0 I:(DE-HGF)0
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910 1 _ |0 I:(DE-HGF)0
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|b 92
910 1 _ |0 I:(DE-HGF)0
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|b 93
910 1 _ |0 I:(DE-HGF)0
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910 1 _ |0 I:(DE-HGF)0
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Marc 21