Properties of high energy interactions deduced from cosmic rays and their comparison with results from recent accelerator experiments

Details Properties of high energy interactions deduced from cosmic rays and their comparison with results from recent accelerator experiments Properties of high energy interactions deduced from cosmic rays and their comparison with results from recent accelerator experiments

Jul 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982aipc...85..578w&link_type=abstract

AIP Conference Proceedings, Volume 85, pp. 578-584 (1982).

Physics

1

Cosmic-Ray Interactions, Inelastic Scattering: Many-Particle Final States

Scientific paper

The development of ideas about some of the more important characteristics of high energy interactions from cosmic ray studies are considered. Cosmic ray data had suggested that simple Feynman scaling breaks down for energetic secondaries and the authors had previously claimed that accelerator data, up to ISR enegies, also show this feature. The latest pp results seem to confirm this contention, at least insofar as the mean number of secondaries and their mean transverse momentum are still rising.

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