Author:
Goyal D. P.,Kumar Animesh,Singh K. Yugindro,Singh S.
Abstract
The phenomenon of cluster production in nucleon–nucleus interactions at ultrahigh energies [Formula: see text] has been investigated using the available cosmic-ray data. The rapidity gap distributions of charged particles in a nondiffractive region of the cross section are found to support the Snider two-channel model as opposed to the model of Quigg, Pirilla, and Thomas. The variation of cluster density and cluster size with the primary energy, multiplicity of shower particles, and nature of the target mass has also been studied.
Publisher
Canadian Science Publishing
Subject
General Physics and Astronomy
Cited by
2 articles.
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