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Inelastic cross section for<i>p</i>-air collisions from air shower experiments and total cross section for<i>p</i>-<i>p</i>collisions up to √<i>s</i>=24 TeV

M. HondaInstitute for Cosmic Ray Research, University of Tokyo, Tanashi, Tokyo, JapanM. NaganoYuge National College of Maritime Technology, Yuge, Ehlme, JapanS. C. TonwarYuge National College of Maritime Technology, Yuge, Ehlme, JapanK. KasaharaYuge National College of Maritime Technology, Yuge, Ehlme, JapanT. HaraYuge National College of Maritime Technology, Yuge, Ehlme, JapanN. HayashidaYuge National College of Maritime Technology, Yuge, Ehlme, JapanY. MatsubaraFaculty of Engineering, Kanagawa University, Kanagawa, JapanM. TeshimaTata Institute of Fundamental Research, Homi Bhabha Marg. Colaba, Bombay, IndiaS. YoshidaInstitute for Cosmic Ray Research, University of Tokyo, Tanashi, Tokyo, Japan
1993en
ABI

Аннотация

Based on an analysis of the extensive air shower data accumulated over the last ten years at Akeno Cosmic Ray Observatory, the value of the proton-air nuclei inelastic cross section (${\mathrm{\ensuremath{\sigma}}}_{\mathrm{in}}^{\mathit{p}\mathrm{\ensuremath{-}}\mathrm{air}}$) has been determined assuming the validity of quasi-Feynman scaling of particle production in the fragmentation region. The energy dependence of ${\mathrm{\ensuremath{\sigma}}}_{\mathrm{in}}^{\mathit{p}\mathrm{\ensuremath{-}}\mathrm{air}}$ can be represented as 290(E/1 TeV${)}^{0.052}$ mb in the energy interval ${10}^{16.2}$--${10}^{17.6}$ eV, where E is the incident proton energy. The total p-p cross section (${\mathrm{\ensuremath{\sigma}}}_{\mathrm{tot}}^{\mathit{p}\mathrm{\ensuremath{-}}\mathit{p}}$), derived using the nuclear distribution function obtained from the shell model, increases with energy as 38.5+1.37 ${\mathrm{ln}}^{2}$(\ensuremath{\surd}s /10 GeV) mb.

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