Time distribution of muon pairs detected at 40 m.w.e

Details Time distribution of muon pairs detected at 40 m.w.e Time distribution of muon pairs detected at 40 m.w.e

Aug 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982nciml..34..529b&link_type=abstract

Nuovo Cimento, Lettere, Serie 2, vol. 34, Aug. 21, 1982, p. 529-532.

Computer Science

Performance

Energetic Particles, Muons, Particle Interactions, Primary Cosmic Rays, Temporal Distribution, Performance Prediction, Statistical Distributions, Stochastic Processes

Scientific paper

Experimental results are reported on the distribution of arrival time intervals between pairs of atmospheric muons detected at 40 m.w.e. underground and generated in interactions of primary nuclei with average energy about 600 GeV. A total number of 72,220 single muons was recorded with a total frequency of 7.1 muons per second, in good agreement with previous measurements at the same depth; 2 x 10 to the -6th random coincidences per second were obtained, a negligible value. The temporal analysis showed very good agreement between data and stochastic predictions. It is concluded that the overabundance of short-delayed cosmic ray particles, if real at higher energies, is not present either at the lower energies of single muons or at the intermediate energies of muon pairs detected in the experiment.

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