Heavy nucleus collisions between 20 and 60 GeV/nucleon

Details Heavy nucleus collisions between 20 and 60 GeV/nucleon Heavy nucleus collisions between 20 and 60 GeV/nucleon

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....6..156b&link_type=abstract

In NASA. Goddard Space Flight Center 19th Intern. Cosmic Ray Conf., Vol. 6 p 156-159 (SEE N85-35848 24-93)

Physics

Cosmic Rays, Heavy Nuclei, Ion Accelerators, Ionic Collisions, Nuclear Emulsions, Extrapolation, Nuclear Interactions, Particle Production

Scientific paper

Interest in studying relativistic nucleus-nucleus interations arises from the fact that they offer an opportunity to probe nuclear matter at high density and temperature. It is expected that under such extreme conditions a transition from hadronic matter into quark-gluon plasma occurs and that in the interactions of highly relativistic nuclei such conditions are created. Cosmic rays remain a unique source of high energy heavy nuclei. The Japanese-American Cooperative Emulsion Experiment (JACEE-3) was designed to study the collisions of heavy cosmic ray nuclei with different nuclear targets at energies beyond 20 GeV/nucleon. JACEE-3 experiment was carried out using a combined electronic counters and an emulsion chamber detector, which was exposed to the cosmic rays on a balloon at an altitude of 5 g/sq cm.

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