Abstract
We describe charged hadronic energy spectra of the cosmic-ray superfamilies named Ursa Maior and P3'-C1-B90, detected by the Chacaltaya and Pamir Emulsion Chamber Collaborations, respectively, using analytical solutions for the diffusion equations. We obtain a very good description of these events incorporating Feynman scaling breaking in the multiparticle production model of our cascading formalism. Centauro exotic events are also investigated.
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