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| 001 | 315076 | ||
| 005 | 20211110140029.0 | ||
| 020 | _ | _ | |a 978-3-945931-08-0 |
| 024 | 7 | _ | |2 datacite_doi |a 10.3204/DESY-PROC-2016-05/11 |
| 024 | 7 | _ | |2 ISSN |a 1435-8077 |
| 037 | _ | _ | |a PUBDB-2016-05611 |
| 041 | _ | _ | |a English |
| 100 | 1 | _ | |0 P:(DE-HGF)0 |a Mauri, Nicoletta |b 0 |e Corresponding author |
| 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 atmospheric muon charge ratio: a probe to constrain the atmospheric $\nu_{\mu}$/$\bar{\nu}_{\mu}$ ratio |
| 260 | _ | _ | |a Hamburg |b Verlag Deutsches Elektronen-Synchrotron |c 2016 |
| 295 | 1 | 0 | |a Mauri, Nicoletta "The atmospheric muon charge ratio: a probe to constrain the atmospheric $\nu_{\mu}$/$\bar{\nu}_{\mu}$ ratio" 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 47-54 |
| 336 | 7 | _ | |2 ORCID |a CONFERENCE_PAPER |
| 336 | 7 | _ | |0 33 |2 EndNote |a Conference Paper |
| 336 | 7 | _ | |2 BibTeX |a INPROCEEDINGS |
| 336 | 7 | _ | |2 DRIVER |a conferenceObject |
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| 336 | 7 | _ | |0 PUB:(DE-HGF)8 |2 PUB:(DE-HGF) |a Contribution to a conference proceedings |b contrib |m contrib |s 1480065718_25198 |
| 336 | 7 | _ | |0 PUB:(DE-HGF)7 |2 PUB:(DE-HGF) |a Contribution to a book |m contb |
| 490 | 0 | _ | |0 PERI:(DE-600)2450075-6 |a DESY-PROC |
| 520 | _ | _ | |a The atmospheric muon charge ratio, defined as the number of positive over negative charged muons, is an important observable to shed light on the physics of cosmic ray interactions in atmosphere. It allows studying the features of high-energy hadronic interactions in the forward region and the composition of primary cosmic rays. In particular, the TeV muon charge ratio provides sensitivity to the charge ratio of high energy kaons, the principal parents of atmospheric neutrinos. In this paper the results from the OPERA experiment in the TeV energy range are reviewed. |
| 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 |
| 856 | 4 | _ | |u https://bib-pubdb1.desy.de/record/315076/files/fulltext.pdf |y OpenAccess |
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