Measurement of the Charge Ratio of Atmospheric Muons With the Cms Detector

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Karapınar, Güler

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GOLD

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Yes

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Abstract

We present a measurement of the ratio of positive to negative muon fluxes from cosmic ray interactions in the atmosphere, using data collected by the CMS detector both at ground level and in the underground experimental cavern at the CERN LHC. Muons were detected in the momentum range from 5 GeV/c to 1 TeV/c. The surface flux ratio is measured to be 1.2766 +/- 0.0032 (stat.) +/- 0.0032 (syst.), independent of the muon momentum, below 100 GeV/c. This is the most precise measurement to date. At higher momenta the data are consistent with an increase of the charge ratio, in agreement with cosmic ray shower models and compatible with previous measurements by deep-underground experiments. (C) 2010 Published by Elsevier B.V.

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Keywords

CMS, Physics, Muon, Cosmic rays, Charge ratio, Muon, flux ratio measured, LHC, CMS, Charge ratio, PARTICLE PHYSICS; LARGE HADRON COLLIDER; CMS, High Energy Physics - Experiment, High Energy Physics - Experiment (hep-ex), Particle and Plasma Physics, [PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex], info:eu-repo/classification/ddc/530, Sea-level, 0105 Mathematical Physics, CMS, muon atmosphere, Physics, ddc:530, COSMIC RAYS; CMS, sea-level, CERN LHC Coll, cosmic radiation, Physical Sciences, Physique des particules élémentaires, PARTICLE PHYSICS, physics, SEA-LEVEL, FLUX, Nuclear and High Energy Physics, [PHYS.HEXP] Physics [physics]/High Energy Physics - Experiment [hep-ex], cms, Particles & Fields, FOS: Physical sciences, Astronomy & Astrophysics, 530, physics; charge ratio; cms; cosmic rays; muon, charge ratio, cosmic rays, muon, 0201 Astronomical and Space Sciences, Nuclear, muon momentum, Cosmic rays, Flux, Science & Technology, Charge ratio; CMS; Cosmic rays; Muon; Physics; Nuclear and High Energy Physics, Molecular, LARGE HADRON COLLIDER, SEA-LEVEL; FLUX, flux, 0202 Atomic, MULTIDISCIPLINARY

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01 natural sciences, 0103 physical sciences

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OpenCitations Citation Count
39

Volume

692

Issue

2

Start Page

83

End Page

104
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52

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519

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