1965
DOI: 10.1007/bf02734821
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Production of knock-on electrons by cosmic-ray muons underground (148 m w.e.)

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Cited by 14 publications
(4 citation statements)
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“…In the 60s, experiments at CERN and Brookhaven measured this scattering cross section using accelerator-produced muons [1][2][3][4]. At the same time, µe collisions were measured by cosmic-ray experiments [5][6][7][8]. The scattering of muons off polarized electrons was then proposed as a polarimeter for high-energy muon beams in the late 80s [9] and measured by the SMC collaboration at CERN a few years later [10].…”
Section: Introductionmentioning
confidence: 99%
“…In the 60s, experiments at CERN and Brookhaven measured this scattering cross section using accelerator-produced muons [1][2][3][4]. At the same time, µe collisions were measured by cosmic-ray experiments [5][6][7][8]. The scattering of muons off polarized electrons was then proposed as a polarimeter for high-energy muon beams in the late 80s [9] and measured by the SMC collaboration at CERN a few years later [10].…”
Section: Introductionmentioning
confidence: 99%
“…The correction factors for zenith angles of 78" and 60" are 1. 75 energy at the detector The discussed corrections have been applied to the experimental results shown in fig. 56.…”
Section: Muons Frotn Neutrino Interactionsmentioning
confidence: 99%
“…Other mechanisms responsible for such dileptons production, although more suppressed, are the production of dimuon through a virtual photon (Trident process) or through highly energetic knock-on electrons (see e.g. [57][58][59][60]). The dimuon yield, suppressed by a factor of (m e /m µ ) 5 compared to electron bremsstrahlung, is estimated through MC simulations to be ∼ 10 −7 per MOT.…”
Section: Introductionmentioning
confidence: 99%