عوامل موثر در عمق بيشينه بهمن هاي گسترده هوايي (EAS) شبيه سازي شده به وسيله مدل هاي اندركنش هادروني و بررسي فراواني ذرات توليد شده به وسيله هر مدل در سطح زمين

Dependence of Xmax and multiplicity of electron and muon on different high energy interaction models

Different high energy interaction models are the applied in CORSIKA code to simulate Extensive Air Showers (EAS) generated by Cosmic Rays (CR). In this work the effects of QGSJET01, QGSJETII, DPMJET, SIBYLL models on Xmax and multiplicity of secondary electrons and muons at observation level are studied.