Abstract
Starting from the exact expression for a transition probability in the relativistic angular momentum representation and using some approximations following from the assumed peripherality of collisions we have obtained an expression for the angular distribution of secondary particles. The differential and integral angular distributions calculated for the energies 10 3 GeV, 10 4 GeV, 10 5 GeV, lead to a natural explanation of the appearance of two maxima in the angular distributions.
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