Peculiarities of gamma-quanta distribution at 20 TeV energy

Details Peculiarities of gamma-quanta distribution at 20 TeV energy Peculiarities of gamma-quanta distribution at 20 TeV energy

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....6..451e&link_type=abstract

In NASA. Goddard Space Flight Center 19th Intern. Cosmic Ray Conf., Vol. 6 p 451-454 (SEE N85-35848 24-93)

Computer Science

Angular Distribution, Calorimeters, Cascade Flow, Cosmic Ray Showers, Electromagnetic Radiation, Fragmentation, Gamma Ray Bursts, Gluons, Ionization Chambers, Particle Density (Concentration), Particle Motion, Protons, Secondary Cosmic Rays, Simulation, Three Dimensional Motion, Charged Particles, Galactic Cosmic Rays, Particle Interactions

Scientific paper

The angular distribution of protons from the fragmentational region is analyzed. The gamma-quanta families are generated in a dense target by cosmic ray particles at 20 Tev energy. Families were found which had dense groups (spikes) of gamma-quanta where the rapidity/density is 3 times more than the average value determined for all registered families. The experimental data is compared with the results of artificial families simulation.

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