High energy particles coplanar emission and spatial characteristics of gamma-families with energies sum Egamma = 100-2000 TeV.

Details High energy particles coplanar emission and spatial characteristics of gamma-families with energies sum Egamma = 100-2000 TeV. High energy particles coplanar emission and spatial characteristics of gamma-families with energies sum Egamma = 100-2000 TeV.

Aug 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001icrc....4.1415y&link_type=abstract

Proceedings of the 27th International Cosmic Ray Conference. 07-15 August, 2001. Hamburg, Germany. Under the auspices of the Int

Physics

Scientific paper

The paper presents the experimental data obtained by large-scale X-ray emulsion chambers of "Pamir" experiment. Azimuthal effects and alignment of the most energetic particles in γ-families with energies E γ = 100-2000 TeV are considered. Experimental dependences of the azimuthal and alignment parameters on family spatial characteristics are compared with MCO Quark-Gluon String Model.

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