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Precision Measurement of the (e+ + e-) Flux in Primary Cosmic Rays from 0.5 GeV to 1 TeV with the Alpha Magnetic Spectrometer on the International Space Station

ContributorsAMS Collaboration
Published inPhysical Review Letters, vol. 113, no. 22, 221102
Publication date2014
Abstract

We present a measurement of the cosmic ray (e+ + e−) flux in the range 0.5 GeV to 1 TeV based on the analysis of 10.6 million (e+ + e−) events collected by AMS. The statistics and the resolution of AMS provide a precision measurement of the flux. The flux is smooth and reveals new and distinct information. Above 30.2 GeV, the flux can be described by a single power law with a spectral index gamma= -3.170 +- 0.008(stat + sys) +- 0.008(energy scale).

Keywords
  • Cosmic rays
  • Positrons
  • Electrons
  • AMS
  • Space mission
Citation (ISO format)
AMS Collaboration. Precision Measurement of the (e+ + e-) Flux in Primary Cosmic Rays from 0.5 GeV to 1 TeV with the Alpha Magnetic Spectrometer on the International Space Station. In: Physical Review Letters, 2014, vol. 113, n° 22, p. 221102. doi: 10.1103/PhysRevLett.113.221102
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Journal ISSN0031-9007
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