Calculation of intensity of high energy muon groups observed deep underground

Details Calculation of intensity of high energy muon groups observed deep underground Calculation of intensity of high energy muon groups observed deep underground

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....8..198v&link_type=abstract

In NASA. Goddard Space Flight Center 19th Intern. Cosmic Ray Conf., Vol. 8 p 198-201 (SEE N85-36066 24-93)

Computer Science

Cosmic Ray Showers, Gluons, High Energy Interactions, Muons, Quarks, Bremsstrahlung, Coulomb Collisions, Electron Photon Cascades, Energy Spectra, Models, Nuclear Scattering, Simulation

Scientific paper

The intensity of narrow muon groups observed in Kolar Gold Field (KGF) at the depth of 3375 m.w.e. was calculated in terms of quark-gluon strings model for high energy hadron - air nuclei interactions by the method of direct modeling of nuclear cascade in the air and muon propagation in the ground for normal primary cosmic ray composition. The calculated intensity has been found to be approx. 10 to the 4 times less than one observed experimentally.

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