The photonuclear energy loss of cosmic-ray muons and its relation with photon-nucleon cross-section

Details The photonuclear energy loss of cosmic-ray muons and its relation with photon-nucleon cross-section The photonuclear energy loss of cosmic-ray muons and its relation with photon-nucleon cross-section

Aug 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981ncimc...4..471m&link_type=abstract

Nuovo Cimento C, Serie 1, vol. 4C, July-Aug. 1981, p. 471-485.

Other

8

Cosmic Rays, Energy Dissipation, High Energy Interactions, Muons, Photonuclear Reactions, Energy Spectra, Nucleons, Particle Intensity, Photons, Scattering Cross Sections

Scientific paper

The nuclear interaction coefficient of the photonuclear energy loss for high-energy muons is calculated by the generalized vector-dominance model with the different energy dependences in real photon-nucleon cross-sections, and by the parton model with a modified scaling variable. The intensities of cosmic-ray muons at great depths are converted into the energy spectrum by taking range fluctuation into account. By comparing the exponents of the spectrum with those from other experiments, it is concluded that the real photon-nucleon cross-section has a ln-squared nu dependence at higher energies than TeV regions.

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