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      Cosmic Ray Air Shower Characteristics in the Framework of the Parton-Based Gribov-Regge Model NEXUS

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          Abstract

          The purpose of this paper is twofold: first we want to introduce a new type of hadronic interaction model (NEXUS), which has a much more solid theoretical basis as, for example, presently used models like QGSJET and VENUS, and ensures therefore a much more reliable extrapolation towards high energies. Secondly, we want to promote an extensive air shower (EAS) calculation scheme, based on cascade equations rather than explicit Monte Carlo simulations, which is very accurate in calculations of main EAS characteristics and extremely fast concerning computing time. We employ the NEXUS model to provide the necessary data on particle production in hadron-air collisions and present the average EAS characteristics for energies 10^14 - 10^17 eV. The experimental data of the casa-blanka group are analyzed in the framework of the new model.

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          Author and article information

          Journal
          11 September 2000
          Article
          10.1103/PhysRevD.63.054030
          hep-ph/0009119
          f95aa930-c9f4-4010-8c4b-5cc2db1c7354
          History
          Custom metadata
          SUBATECH 00-13
          Phys.Rev. D63 (2001) 054030
          15 pages, 8 figures
          hep-ph astro-ph nucl-th

          General astrophysics,High energy & Particle physics,Nuclear physics
          General astrophysics, High energy & Particle physics, Nuclear physics

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