Simulation of Multi-muon Events from EAS at Shallow Depths Underground

Simple item page
dc.creatorBourilkov, Dimitri
dc.date1999-07-06
dc.date.accessioned2026-07-07T02:32:26Z
dc.date.available2026-07-07T02:32:26Z
dc.descriptionThe Monte Carlo program ARROW, based on GEANT and using GHEISHA at energies below 30 GeV, is developed for simulation of the hadron and muon components of extensive air showers with primary energy $10^{12}-10^{17}$ eV. Calculations of the characteristics of multi-muon events as observed underground by the LEP detectors are presented and their dependence on the primary cosmic ray composition and some basic assumptions of the hadronic interaction model is discussed.
dc.description6 pages, 1 figure, 2 tables, presented at the First Arctic Workshop on Cosmic Ray Muons, Sodankyla, Finland, April 24-29, 1999
dc.identifierhttps://arxiv.org/abs/astro-ph/9907078
dc.identifierhttp://arxiv.org/abs/astro-ph/9907078
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/14460
dc.subjectAstrophysics
dc.titleSimulation of Multi-muon Events from EAS at Shallow Depths Underground
dc.typetext

Files

Collections

arXiv