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.
Rastegarzadeh,G and Nemati,M . (2019). Dependence of Xmax and multiplicity of electron and muon on different high energy interaction models. Iranian Journal of Physics Research, 10(1), 47-53.
MLA
Rastegarzadeh,G , and Nemati,M . "Dependence of Xmax and multiplicity of electron and muon on different high energy interaction models", Iranian Journal of Physics Research, 10, 1, 2019, 47-53.
HARVARD
Rastegarzadeh G, Nemati M. (2019). 'Dependence of Xmax and multiplicity of electron and muon on different high energy interaction models', Iranian Journal of Physics Research, 10(1), pp. 47-53.
CHICAGO
G Rastegarzadeh and M Nemati, "Dependence of Xmax and multiplicity of electron and muon on different high energy interaction models," Iranian Journal of Physics Research, 10 1 (2019): 47-53,
VANCOUVER
Rastegarzadeh G, Nemati M. Dependence of Xmax and multiplicity of electron and muon on different high energy interaction models. Iranian Journal of Physics Research. 2019;10(1):47-53 (In Persian).
