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author Bendavid, Joshua L.
Busza, Wit
Butz, Erik M.
Cali, Ivan Amos
Chan, M.
D'Enterria, David
Everaerts, Pieter Bruno Bart
Gomez-Ceballos, Guillelmo
Goncharov, Maxim
Hahn, Kristian Allan
Kim, Y.
Klute, Markus
Li, W.
Ma, Teng
Nahn, Steven
Paus, Christoph M. E.
Rudolph, Matthew Scott
Stephans, George S. F.
Wenger, Edward Allen
Wyslouch, Boleslaw
Yilmaz, Yetkin
Yoon, A. S.
Zanetti, Marco
Roland, Christof E
Sumorok, Konstanty C
Xie, Si
Alver, Burak Han
Bauer, Gerry P
Harris, Philip Coleman
Lee, Yen-Jie
Loizides, Constantinos
Luckey Jr, P David
author2 Massachusetts Institute of Technology. Department of Physics
author_facet Massachusetts Institute of Technology. Department of Physics
Bendavid, Joshua L.
Busza, Wit
Butz, Erik M.
Cali, Ivan Amos
Chan, M.
D'Enterria, David
Everaerts, Pieter Bruno Bart
Gomez-Ceballos, Guillelmo
Goncharov, Maxim
Hahn, Kristian Allan
Kim, Y.
Klute, Markus
Li, W.
Ma, Teng
Nahn, Steven
Paus, Christoph M. E.
Rudolph, Matthew Scott
Stephans, George S. F.
Wenger, Edward Allen
Wyslouch, Boleslaw
Yilmaz, Yetkin
Yoon, A. S.
Zanetti, Marco
Roland, Christof E
Sumorok, Konstanty C
Xie, Si
Alver, Burak Han
Bauer, Gerry P
Harris, Philip Coleman
Lee, Yen-Jie
Loizides, Constantinos
Luckey Jr, P David
author_sort Bendavid, Joshua L.
collection MIT
description 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.
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spelling mit-1721.1/960522023-02-26T05:56:00Z Measurement of the charge ratio of atmospheric muons with the CMS detector Bendavid, Joshua L. Busza, Wit Butz, Erik M. Cali, Ivan Amos Chan, M. D'Enterria, David Everaerts, Pieter Bruno Bart Gomez-Ceballos, Guillelmo Goncharov, Maxim Hahn, Kristian Allan Kim, Y. Klute, Markus Li, W. Ma, Teng Nahn, Steven Paus, Christoph M. E. Rudolph, Matthew Scott Stephans, George S. F. Wenger, Edward Allen Wyslouch, Boleslaw Yilmaz, Yetkin Yoon, A. S. Zanetti, Marco Roland, Christof E Sumorok, Konstanty C Xie, Si Alver, Burak Han Bauer, Gerry P Harris, Philip Coleman Lee, Yen-Jie Loizides, Constantinos Luckey Jr, P David Massachusetts Institute of Technology. Department of Physics Massachusetts Institute of Technology. Laboratory for Nuclear Science Massachusetts Institute of Technology. School of Science Alver, B. Bauer, Gerry P. Bendavid, Joshua L. Busza, Wit Butz, Erik M. Cali, Ivan Amos Chan, M. D'Enterria, David Everaerts, Pieter Bruno Bart Gomez-Ceballos, Guillelmo Goncharov, Maxim Hahn, Kristian Allan Harris, P. Kim, Y. Klute, Markus Lee, Y.-J. Li, W. Loizides, C. Luckey, P. David, Jr. Ma, Teng Nahn, Steven Paus, Christoph M. E. Roland, Christof E. Rudolph, Matthew Scott Stephans, George S. F. Sumorok, Konstanty C. Wenger, Edward Allen Wyslouch, Boleslaw Xie, S. Yilmaz, Yetkin Yoon, A. S. Zanetti, Marco 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. United States. Dept. of Energy National Science Foundation (U.S.) Alfred P. Sloan Foundation 2015-03-17T18:35:02Z 2015-03-17T18:35:02Z 2010-07 2010-07 Article http://purl.org/eprint/type/JournalArticle 03702693 http://hdl.handle.net/1721.1/96052 Khachatryan, V., A.M. Sirunyan, A. Tumasyan, W. Adam, T. Bergauer, M. Dragicevic, J. Erö, et al. “Measurement of the Charge Ratio of Atmospheric Muons with the CMS Detector.” Physics Letters B 692, no. 2 (August 2010): 83–104. https://orcid.org/0000-0002-3831-9071 https://orcid.org/0000-0003-3106-4894 https://orcid.org/0000-0002-6047-4211 https://orcid.org/0000-0003-3681-0649 https://orcid.org/0000-0003-2593-7767 https://orcid.org/0000-0002-0869-5631 en_US http://dx.doi.org/10.1016/j.physletb.2010.07.033 Physics Letters B Creative Commons Attribution http://creativecommons.org/licenses/by-nc-nd/3.0/ application/pdf Elsevier Elsevier
spellingShingle Bendavid, Joshua L.
Busza, Wit
Butz, Erik M.
Cali, Ivan Amos
Chan, M.
D'Enterria, David
Everaerts, Pieter Bruno Bart
Gomez-Ceballos, Guillelmo
Goncharov, Maxim
Hahn, Kristian Allan
Kim, Y.
Klute, Markus
Li, W.
Ma, Teng
Nahn, Steven
Paus, Christoph M. E.
Rudolph, Matthew Scott
Stephans, George S. F.
Wenger, Edward Allen
Wyslouch, Boleslaw
Yilmaz, Yetkin
Yoon, A. S.
Zanetti, Marco
Roland, Christof E
Sumorok, Konstanty C
Xie, Si
Alver, Burak Han
Bauer, Gerry P
Harris, Philip Coleman
Lee, Yen-Jie
Loizides, Constantinos
Luckey Jr, P David
Measurement of the charge ratio of atmospheric muons with the CMS detector
title Measurement of the charge ratio of atmospheric muons with the CMS detector
title_full Measurement of the charge ratio of atmospheric muons with the CMS detector
title_fullStr Measurement of the charge ratio of atmospheric muons with the CMS detector
title_full_unstemmed Measurement of the charge ratio of atmospheric muons with the CMS detector
title_short Measurement of the charge ratio of atmospheric muons with the CMS detector
title_sort measurement of the charge ratio of atmospheric muons with the cms detector
url http://hdl.handle.net/1721.1/96052
https://orcid.org/0000-0002-3831-9071
https://orcid.org/0000-0003-3106-4894
https://orcid.org/0000-0002-6047-4211
https://orcid.org/0000-0003-3681-0649
https://orcid.org/0000-0003-2593-7767
https://orcid.org/0000-0002-0869-5631
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