000315076 001__ 315076
000315076 005__ 20211110140029.0
000315076 0247_ $$2datacite_doi$$a10.3204/DESY-PROC-2016-05/11
000315076 0247_ $$2ISSN$$a1435-8077
000315076 020__ $$a978-3-945931-08-0
000315076 037__ $$aPUBDB-2016-05611
000315076 041__ $$aEnglish
000315076 1001_ $$0P:(DE-HGF)0$$aMauri, Nicoletta$$b0$$eCorresponding author
000315076 1112_ $$0C16-03-17$$2inspire$$aMagellan Workshop$$cHamburg$$d2016-03-17 - 2016-03-18$$wGermany
000315076 245__ $$aThe atmospheric muon charge ratio: a probe to constrain the atmospheric $\nu_{\mu}$/$\bar{\nu}_{\mu}$ ratio
000315076 260__ $$aHamburg$$bVerlag Deutsches Elektronen-Synchrotron$$c2016
000315076 29510 $$aMauri, 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
000315076 300__ $$a47-54
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000315076 4900_ $$0PERI:(DE-600)2450075-6$$aDESY-PROC
000315076 520__ $$aThe 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.
000315076 7870_ $$0PUBDB-2016-05604$$aDahmke, Stefan K.G. et. al.$$dDeutsches Elektronen-Synchrotron, DESY$$iisPartOf$$rDESY-PROC-2016-05$$tProceedings, Magellan Workshop: Connecting Neutrino Physics and Astronomy: Hamburg, Germany, March 17-18, 2016
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