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| 001 | 315080 | ||
| 005 | 20211110140029.0 | ||
| 020 | _ | _ | |a 978-3-945931-08-0 |
| 024 | 7 | _ | |2 datacite_doi |a 10.3204/DESY-PROC-2016-05/5 |
| 024 | 7 | _ | |2 ISSN |a 1435-8077 |
| 037 | _ | _ | |a PUBDB-2016-05615 |
| 041 | _ | _ | |a English |
| 100 | 1 | _ | |0 P:(DE-HGF)0 |a Lozza, Valentina |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 The SNO+ experiment: current status and future prospects |
| 260 | _ | _ | |a Hamburg |b Verlag Deutsches Elektronen-Synchrotron |c 2016 |
| 295 | 1 | 0 | |a Lozza, Valentina "The SNO+ experiment: current status and future prospects" 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 87-94 |
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| 490 | 0 | _ | |0 PERI:(DE-600)2450075-6 |a DESY-PROC |
| 520 | _ | _ | |a SNO+ is a multi-purpose neutrino experiment whose main physics goal is the search for the neutrinoless double-beta ($0\nu\beta\beta$) decay of $^{130}$Te. With an initial loading of 0.5\% (by weight) of natural tellurium SNO+ is expected to reach a sensitivity on the $0\nu\beta\beta$ lifetime of the order of 10$^{26}$ years at 90\% C.L. in a 5-year run. Along with the $0\nu\beta\beta$ decay search, SNO+ has the capability to measure the low energy solar neutrinos, like pep and CNO neutrinos. It has also an extraordinary opportunity to do the first measurement of the supernova $\nu_x$ energy spectrum. |
| 700 | 1 | _ | |0 P:(DE-HGF)0 |a SNO+ Collaboration |b 1 |e Collaboration author |
| 787 | 0 | _ | |0 PUBDB-2016-05604 |a Dahmke, Stefan K.G. et. al. |d Deutsches Elektronen-Synchrotron, DESY |i isPartOf |r DESY-PROC-2016-05 |t Proceedings, Magellan Workshop: Connecting Neutrino Physics and Astronomy: Hamburg, Germany, March 17-18, 2016 |
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