Energy estimates of cosmic ray events

Details Energy estimates of cosmic ray events Energy estimates of cosmic ray events

Oct 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980icrc....6..187d&link_type=abstract

In: International Cosmic Ray Conference, 16th, Kyoto, Japan, August 6-18, 1979, Conference Papers. Volume 6. (A81-12386 02-93) T

Physics

Nuclear Physics

Cosmic Rays, High Energy Interactions, Particle Energy, Particle Interactions, Incident Radiation, Nuclear Emulsions, Nuclei (Nuclear Physics), Particle Production

Scientific paper

Modified methods for estimating the energy of the incident particles in high energy cosmic ray collisions are proposed and their validity is demonstrated in accelerator experiments with known beam energies. The Castagnoli method (Castagnoli et al., 1953) is modified and the PT method is modified, wherein a constant value of the average transverse momentum (equal to .35 GeV) of the produced charged particles is assumed. It is shown that both the Collective Tube models (Berlad, Dar, and Eilam, 1976) and the Independent Particle Fragmentation model (Dar, and Vary, 1972) lead to the same energy estimate for particle-nucleus collisions as well as the same energy estimate for nucleus-nucleus collisions.

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