A cosmic-ray ultra high-energy multijet family event

Details A cosmic-ray ultra high-energy multijet family event A cosmic-ray ultra high-energy multijet family event

Mar 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987pefpn..10..393z&link_type=abstract

(Physica Energiae Fortis et Physica Nuclearis, vol. 10, July 1986, p. 393-399) Chinese Physics (ISSN 0273-429X), vol. 7, Jan.-Ma

Physics

Cosmic Ray Showers, High Energy Interactions, Particle Production, Energy Spectra, Gluons, Hadrons, Jets, Particle Accelerators, Quantum Chromodynamics, Quarks

Scientific paper

A cosmic-ray ultrahigh-energy multijet family event with visible energy of about 1500 TeV and five large cores is reported. This event was found in the 1980-1981 exposure of the Mt. Kambala emulsion-chamber experiment. The family characteristics are analyzed and compared with other cosmic ray events in the same energy range. The production and fragmentation characteristics of the five jets are studied and compared with the experimental results of accelerators and emulsion chamber C-jets, as well as with QCD predictions above the TeV range. Some features on hadronic interactions in the TeV range are discussed.

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