Alignment in gamma-hadron families of cosmic rays and interaction characteristics at E0 approximately equal to 10 exp 16 eV

Statistics – Computation

Scientific paper

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Cosmic Rays, Elementary Particle Interactions, Gamma Ray Astronomy, Hadrons, Computational Astrophysics, Nuclear Reactions

Scientific paper

Alignment along a straight line of the principal energy fluxes in families of cosmic-ray particles has been observed. The presence of this effect depends on the interaction energy and is evidence of the coplanar character of the dispersion of secondary particles relatively low above the detector instrumentation in an act of nuclear interaction at ultrahigh energies (E0 not less than 10 exp 16 eV).

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