Inelastic cross section forp-air collisions from air shower experiments and total cross section forp-pcollisions up to √s=24 TeV
- 1 February 1993
- journal article
- research article
- Published by American Physical Society (APS) in Physical Review Letters
- Vol. 70 (5) , 525-528
- https://doi.org/10.1103/physrevlett.70.525
Abstract
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 () has been determined assuming the validity of quasi-Feynman scaling of particle production in the fragmentation region. The energy dependence of can be represented as 290(E/1 TeV mb in the energy interval – eV, where E is the incident proton energy. The total p-p cross section (), derived using the nuclear distribution function obtained from the shell model, increases with energy as 38.5+1.37 (√s /10 GeV) mb.
Keywords
This publication has 12 references indexed in Scilit:
- Measurements of cosmic-ray air shower development at energies above 10 to the 17th eVThe Astrophysical Journal, 1990
- High-energy nucleon-nucleus scattering and cosmic-ray cross sectionsPhysical Review D, 1988
- Measurement of the proton-antiproton total and elastic cross sections at the CERN SPS colliderPhysics Letters B, 1984
- Energy spectrum of primary cosmic rays between 1014.5and 1018eVJournal of Physics G: Nuclear Physics, 1984
- Inelastic-Air Cross Section at Energies betweenandeV Estimated from Air-Shower ExperimentsPhysical Review Letters, 1983
- Hadronic interactions at energies around103TeV inferred from the large-scale emulsion-chamber experiment at Mt. FujiPhysical Review D, 1981
- Tests of geometrical scaling and generalizationsNuclear Physics B, 1975
- Evidence for Rapidly RisingTotal Cross Section from Cosmic-Ray DataPhysical Review Letters, 1972
- High-energy scattering of protons by nucleiNuclear Physics B, 1970
- End to the Cosmic-Ray Spectrum?Physical Review Letters, 1966