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Sulla componente della radiazione penetrante generatrice di stelle

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Il Nuovo Cimento (1943-1954)

Riassunto

Si propone un modello che può servire a studiare fenomenologicamente la componente della radiazione penetrante generatrice di stelle. Si discute in particolare quella parte di tale componente responsabile del maggior numero delle evaporazioni e delle minori esplosioni, di energia inferiore al BeV. Si confrontano i risultati ottenuti con i fatti sperimentali fino ad ora noti in proposito.

Summary

A model for the starproducing component of cosmic radiation is discussed. The behavior of nucleons of not too high an energy is studied in some detail. Some consequences of the proposed model are compared with the experimental facts.

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Authors and Affiliations

  1. Centro di Fisica Nucleare del C.N.R., Roma

    B. Ferretti

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  1. B. Ferretti
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Ferretti, B. Sulla componente della radiazione penetrante generatrice di stelle. Nuovo Cim 6, 379–389 (1949). https://doi.org/10.1007/BF02781030

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  • DOI: https://doi.org/10.1007/BF02781030

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