Measurement of Cosmic-Ray Muon Charge Ratio at Sea Level Between Energies of 10 and 1500 GeV

T. H. Burnett, L. J. LaMay, G. E. Masek, T. Maung, E. S. Miller, H. Ruderman, and W. Vernon
Phys. Rev. Lett. 30, 937 – Published 7 May 1973
PDFExport Citation

Abstract

We have measured the cosmic-ray muon charge ratio, μ+μ, from 10 GeV to 1.5 TeV with a sea-level magnetic spectrometer at eight different zenith angles between 0° and 90°. The data are consistent with a constant charge ratio between 50 GeV and 1.5 TeV, in agreement with the predictions of the scaling hypothesis. Assuming the charge ratio to be constant, we obtain its value as 1.261 ± 0.009.

  • Received 12 March 1973

DOI:https://doi.org/10.1103/PhysRevLett.30.937

©1973 American Physical Society

Authors & Affiliations

T. H. Burnett, L. J. LaMay, G. E. Masek, T. Maung, E. S. Miller, H. Ruderman, and W. Vernon

  • Department of Physics, University of California, San Diego, La Jolla, California 92037

References (Subscription Required)

Click to Expand
Issue

Vol. 30, Iss. 19 — 7 May 1973

Reuse & Permissions
Access Options
Author publication services for translation and copyediting assistance advertisement

Authorization Required


×
×

Images

×

Sign up to receive regular email alerts from Physical Review Letters

Log In

Cancel
×

Search


Article Lookup

Paste a citation or DOI

Enter a citation
×