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Non-linear effects in high energy hadronic interactions. hep-ph/0501093 (2005)

by S Ostapchenko
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SLAC-PUB-14593 Momentum spectrum of cosmic muons at a depth of 320 mwe

by N. O. Hashim, C. Grupen, S. Luitz, A. Mailov, F. Maciuc, A. -s. Müller, A. Putzer, H. -g. S, S. Schmeling, M. Schmelling, R. Tcaciuc, H. Wachsmuth, Th. Ziegler, K. Zuber
"... Cosmic muons are produced through interactions of primary cosmic radiation in the atmosphere. They are a component of extensive air showers which can also be measured underground. The CosmoALEPH experiment used the ALEPH detector at the European Laboratory for Particle Physics, CERN, to measure cosm ..."
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Cosmic muons are produced through interactions of primary cosmic radiation in the atmosphere. They are a component of extensive air showers which can also be measured underground. The CosmoALEPH experiment used the ALEPH detector at the European Laboratory for Particle Physics, CERN, to measure cosmic muon events at a depth of 320 mwe underground. The momentum spectrum and charge ratio of the cosmic muons are measured. The results are compared with the expectations from MC simulations based on different hadronic interaction models. 1.
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...ervable in EAS that can be used for testing theoretical hadronic interaction models. Further work is in progress to compare the data with updated models for high energy interactions such as QGSJET-II =-=[19]-=- and NEXUS 3 [20] which will be included in the next version of CORSIKA[15, 21]. A more detailed analysis of the detector acceptance and trigger efficiency as function of muon momentum for inclined mu...

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