A complanar emission of particles in nuclear interaction for E sub 0 >10 sup 1 sup 6 eV detected in the stratosphere

A gamma-hadron superfamily of cosmic rays with total energy >10 sup 1 sup 6 eV was detected by an emulsion chamber aboard a stratospheric balloon, the event being the unique example of so high energy nuclear interaction in the world statistics. Applying the experience accumulated by the Pamir Col...

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Detalles Bibliográficos
Autores principales: Managadze, A K, Galkin, V I, Goncharova, L A, Kopenkin, V V, Kotelnikov, K A, Osedlo, V I, Polukhina, N G, Rakobolskaya, I V, Roganova, T M, Sveshnikova, L G
Lenguaje:rus
Publicado: Joint Inst. Nucl. Res. 2002
Materias:
Acceso en línea:http://cds.cern.ch/record/748263
Descripción
Sumario:A gamma-hadron superfamily of cosmic rays with total energy >10 sup 1 sup 6 eV was detected by an emulsion chamber aboard a stratospheric balloon, the event being the unique example of so high energy nuclear interaction in the world statistics. Applying the experience accumulated by the Pamir Collaboration (a mountain emulsion experiment) for superfamily analysis, in this family the phenomenon of coplanar emission of most energetic particles and significant lateral asymmetry of other particles in the central area of the event were found. The superfamily belongs to the energy range unattainable for modern accelerators