Giant mini-clusters as possible origin of halo phenomena observed in super-families

Details Giant mini-clusters as possible origin of halo phenomena observed in super-families Giant mini-clusters as possible origin of halo phenomena observed in super-families

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....6..360.&link_type=abstract

In NASA. Goddard Space Flight Center 19th Intern. Cosmic Ray Conf., Vol. 6 p 360-363 (SEE N85-35848 24-93)

Mathematics

Logic

Cosmic Rays, Gamma Rays, Hadrons, Halos, Protons, Detection, Energy Distribution, Energy Spectra, High Energy Interactions, Nuclear Emulsions, Radiation Detectors

Scientific paper

Among 91 mini-clusters from 30 high energy Chiron-type families in Chacaltaya emulsion chambers, there were observed several extremely large multiplicity clusters in the highest energy range, far beyond the average of ordinary type clusters. Some details of microscopic observation of those giant mini-clusters in nuclear emulsion plates and some phenomenological regularity found in common among them are described. Such giant mini-clusters are possible candidates for the origin of narrow symmetric single halo phenomena in X-ray films which are frequently observed in super-families of visible energy greater than 1,000 TeV.

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