We present a review of past measurements of the vertical atmospheric muon charge ratio above 1 TeV. In particular we focus on the latest OPERA data which conrm with a higher statistical signicance a drop of the charge ratio above 3 TeV. We attempt to interpret the result in terms of possible physical mechanisms that could manifest itself in this energy region.

N. Mauri, M. Sioli (2012). A new interpretation of the high energy atmospheric muon charge ratio. JOURNAL OF PHYSICS. CONFERENCE SERIES, 375(part 5), 1-5 [10.1088/1742-6596/375/1/052018].

A new interpretation of the high energy atmospheric muon charge ratio

MAURI, NICOLETTA;SIOLI, MAXIMILIANO
2012

Abstract

We present a review of past measurements of the vertical atmospheric muon charge ratio above 1 TeV. In particular we focus on the latest OPERA data which conrm with a higher statistical signicance a drop of the charge ratio above 3 TeV. We attempt to interpret the result in terms of possible physical mechanisms that could manifest itself in this energy region.
2012
N. Mauri, M. Sioli (2012). A new interpretation of the high energy atmospheric muon charge ratio. JOURNAL OF PHYSICS. CONFERENCE SERIES, 375(part 5), 1-5 [10.1088/1742-6596/375/1/052018].
N. Mauri; M. Sioli
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11585/128738
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