Theoretical Study of Extensive Air Shower Effects in Atmosphere by Simulating the Lateral structure of Several Cosmic Radiations. (arXiv:2007.16004v1 [astro-ph.HE])
<a href="http://arxiv.org/find/astro-ph/1/au:+Jassim_H/0/1/0/all/0/1">Hassanen Abdulhussaen Jassim</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Al_Rubaiee_A/0/1/0/all/0/1">A. A. Al-Rubaiee</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Al_Alawy_I/0/1/0/all/0/1">Iman Tarik Al-Alawy</a>
Extensive air showers (EAS) are a cascade of electromagnetic radiation and
ionized particles that produced in the atmosphere through the interaction of a
primary cosmic ray with the atom of nucleus in the air producing a huge amount
of secondary particles such as X-ray, electrons, neutrons, muons, alpha
particles, etc. In this work, EAS effects were demonstrated by estimating the
lateral distribution function (LDF) at ultrahigh energies of the various cosmic
ray particles. The LDF of charged particles such as electron and positron pair
production, gamma and muons particles was simulated at ultrahigh energies
10^16, 10^18 and 10^19 eV. The simulation was carried out using an air shower
simulator called AIRES system version 2.6.0. The effect of the primary
particles, energies and zenith angle on the LDF of charged particles produced
in the EAS was taken into account. Comparison of LDF for charged particles and
experimental results gave good agreement for electron and positron pair
production and muons particles at 10^19 eV for 0 and 10 zenith angles
Extensive air showers (EAS) are a cascade of electromagnetic radiation and
ionized particles that produced in the atmosphere through the interaction of a
primary cosmic ray with the atom of nucleus in the air producing a huge amount
of secondary particles such as X-ray, electrons, neutrons, muons, alpha
particles, etc. In this work, EAS effects were demonstrated by estimating the
lateral distribution function (LDF) at ultrahigh energies of the various cosmic
ray particles. The LDF of charged particles such as electron and positron pair
production, gamma and muons particles was simulated at ultrahigh energies
10^16, 10^18 and 10^19 eV. The simulation was carried out using an air shower
simulator called AIRES system version 2.6.0. The effect of the primary
particles, energies and zenith angle on the LDF of charged particles produced
in the EAS was taken into account. Comparison of LDF for charged particles and
experimental results gave good agreement for electron and positron pair
production and muons particles at 10^19 eV for 0 and 10 zenith angles
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