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- W2549116499 abstract "The charge ratio of cosmic muons has important information in both atmospheric neutrinos anomaly and hadronic interactions. We measured the muon charge ratio (Rμ = Nμ+ /Nμ− ) in the cosmic rays flux at the momenta range 0.76-1.60 GeV/c at Sharif University of Technology in Tehran (35 ◦ 43 � N , 51 ◦ 20 � E) and 1200 m above sea level (890 gcm −2 ) by using a cosmic ray telescope. We used the delayed coincidence method based on reduced mean life time of negative muon due to nuclear capture in matter. By finding Rμ in different time intervals, we indicated 3 week time interval is proper to obtain Rμ and in this time interval, Rμ =1 .18±0.03. So we compared the experimental data to predictions of CORSIKA simulations using high energy interaction model (QGSJET-II) and two low energy interaction models (URQMD and GHEISHA) in the energy range from 10 12 eV to 10 16 eV for primary particles. We obtained Rμ=1.04 with QGSJET-URQMD models and Rμ=1.06 with QGSJET-GHEISHA models. From the measurement of muons flux in different zenithal and azimuthal angles, the muon angular distribution is obtained as I(θ )= I(0) cos n θ. So the influence of the geomagnetic field leads to a dependence of the muon flux on the azimuth angle (East-West effect), in particular for low energy muons." @default.
- W2549116499 created "2016-11-30" @default.
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- W2549116499 date "2011-01-01" @default.
- W2549116499 modified "2023-09-27" @default.
- W2549116499 title "Measurement of the Atmospheric Muon Charge Ratio by Using a Cosmic Ray Telescope" @default.
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