sibyll: An event generator for simulation of high energy cosmic ray cascades

R. S. Fletcher, T. K. Gaisser, Paolo Lipari, and Todor Stanev
Phys. Rev. D 50, 5710 – Published 1 November 1994
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Abstract

We describe the physical basis and some applications of an efficient event generator designed for Monte Carlo simulations of atmospheric cascades at ultrahigh energies. The event generator (sibyll) incorporates many features of the Lund programs, but emphasizes the fragmentation region and the production of minijets. A consistent treatment of hadron-hadron and hadron-nucleus interactions is emphasized. Examples of applications are the calculation of coincident muons observed in deep underground detectors and the simulation of the longitudinal development of air shower components in the atmosphere.

  • Received 26 January 1994

DOI:https://doi.org/10.1103/PhysRevD.50.5710

©1994 American Physical Society

Authors & Affiliations

R. S. Fletcher, T. K. Gaisser, Paolo Lipari, and Todor Stanev

  • Bartol Research Institute, University of Delaware, Newark, Delaware 19716
  • INFN sezione di Roma, and Dipartimento di Fisica Universitá di Roma I, Piazzale Aldo Moro 2, Rome, Italy
  • Department of Physics, The Johns Hopkins University, Baltimore, Maryland 21218

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Vol. 50, Iss. 9 — 1 November 1994

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