Monte Carlo studies on electromagnetic cascades in extensive air showers

1968 ◽  
Vol 46 (10) ◽  
pp. S189-S196 ◽  
Author(s):  
K. O. Thielheim ◽  
E. K. Schlegel ◽  
R. Beiersdorf
Keyword(s):  
Monte Carlo ◽  
Electron Density ◽  
Three Dimensional ◽  
High Energy ◽  
Extensive Air Showers ◽  
Air Showers ◽  
Energy Distributions ◽  
The Core ◽  
Fragmentation Mechanisms ◽  
Monte Carlo Studies

Three-dimensional Monte Carlo calculations have been performed on the trajectories of high-energy hadrons in extensive air showers. The central electron density and gradient of distribution are obtained for individual electromagnetic cascades together with coordinates at the level of observation. Various assumptions concerning primary mass number and energy, distributions of strong interaction parameters, and fragmentation mechanisms are discussed with respect to the production of steep maxima of electron density by single electromagnetic cascades in the core region of extensive air showers.

ENERGY ESTIMATION OF ULTRA-HIGH ENERGY COSMIC RAY PHOTONS BY MONTE CARLO SIMULATIONS OF EXTENSIVE AIR SHOWERS

2010 ◽  
Vol 25 (20) ◽  
pp. 3953-3964
Author(s):  
A. GERANIOS ◽  
D. KOUTSOKOSTA ◽  
O. MALANDRAKI ◽  
H. ROSAKI-MAVROULI
Keyword(s):  
Monte Carlo ◽  
Gamma Ray ◽  
Cosmic Ray ◽  
High Energy ◽  
Extensive Air Showers ◽  
Ultra High Energy ◽  
Air Showers ◽  
Simulation Code ◽  
Energy Estimation ◽  
High Energy Cosmic Rays

Ultra-High Energy Cosmic Rays (UHECR) (E ≥ 5 × 1019 eV ) are detected through Extensive Air Showers that are created when a primary cosmic ray particle interacts with the atmosphere of the Earth. The energy of the primary particle can be estimated experimentally based on simulations. In this paper, we attempt to estimate the energy of UHECR gamma ray photons by applying a Monte Carlo simulation code and we compare the results with the ones derived in our previous papers for hadron initiated showers. The scenario of simulations is adapted to the P. Auger Observatory site.

Note on multiple-core structure of the hadronic component of extensive air showers

1968 ◽  
Vol 46 (10) ◽  
pp. S37-S40 ◽  
Author(s):  
K. O. Thielheim ◽  
E. K. Schlegel ◽  
R. Beieesdorf
Keyword(s):  
Monte Carlo ◽  
Primary Particle ◽  
High Energy ◽  
Core Structure ◽  
Extensive Air Showers ◽  
Mass Composition ◽  
Air Showers ◽  
Hadronic Interaction ◽  
Monte Carlo Calculations ◽  
Hadronic Component

Monte Carlo calculations on high-energy hadrons in extensive air showers have been performed, using various models of hadronic interaction and fragmentation. Frequencies of showers the hadronic component of which shows multiple-core structure are discussed in terms of primary particle and hadronic interaction parameters. The existence of a correlation between the primary mass composition and the frequencies of specified types of showers is demonstrated.

ENERGY ESTIMATION OF ULTRA-HIGH ENERGY COSMIC RAY HADRONS BY MONTE CARLO SIMULATIONS OF EXTENSIVE AIR SHOWERS

2010 ◽  
Vol 25 (12) ◽  
pp. 2561-2571 ◽  
Author(s):  
A. GERANIOS ◽  
D. KOUTSOKOSTA ◽  
A. MASTICHIADIS ◽  
O. MALANDRAKI ◽  
H. ROSAKI-MAVROULI ◽  
...  
Keyword(s):  
Monte Carlo ◽  
Cosmic Ray ◽  
High Energy ◽  
Extensive Air Showers ◽  
Ultra High Energy ◽  
Air Showers ◽  
Simulation Code ◽  
Energy Estimation ◽  
High Energy Cosmic Rays ◽  
The Earth

Ultra-High Energy Cosmic Rays (E ≥ 5 ×1019 eV ) are detected through Extensive Air Showers that are created when a primary cosmic ray particle interacts with the atmosphere of the Earth. The energy of the primary particle can be estimated experimentally based on simulations. In this paper we attempt to estimate the energy of UHECR hadrons ( He, Li, C, Fe ) by applying a Monte Carlo simulation code and we compare the results with the ones derived in our previous paper for proton initiated showers. The scenario of simulations is adapted to the P. Auger Observatory site.

Three-dimensional simulation of air showers. Core structures

1968 ◽  
Vol 46 (10) ◽  
pp. S164-S174 ◽  
Author(s):  
N. Ogita ◽  
M. Rathgeber ◽  
S. Takagi ◽  
A. Ueda
Keyword(s):  
Monte Carlo ◽  
Monte Carlo Simulations ◽  
Three Dimensional ◽  
Nuclear Interaction ◽  
High Energy ◽  
Primary Energy ◽  
Air Showers ◽  
Density Peaks ◽  
Shower Development ◽  
Fireball Model

Three-dimensional Monte Carlo simulations of extensive air showers were made with a model of nuclear interaction based essentially on the two-fireball model. Monte Carlo simulations were tried with primary protons of energy 106 and 2.5 × 105 GeV. Various quantities related to electrons, nuclear-active particles, and muons were obtained which enable us to get detailed information on the development of individual showers.Among various features so far simulated, those of core structures, in particular, are presented in great detail and discussed in connection with shower development. Within the framework of the fireball model the following main features were noted for the formation of multiple electron cores. The fraction of multicored events is strongly dependent on the primary energy, and decreases considerably with increasing height. These events were all initiated at high altitudes and none of them had high-density peaks with a separation of a few or more meters. High-energy nuclear particles play an important role in producing multicored events, but none of the peaks in multi-cored events were produced by a single γ ray.These features, in comparison with the experimental results, require the introduction of a large mean transverse momentum for nucleons, particularly at high energies [Formula: see text]. It seems likely that it increases with energy.

Three-Dimensional Monte Carlo Simulation of Extensive Air Showers

1967 ◽  
Vol 164 (5) ◽  
pp. 1567-1583 ◽  
Author(s):  
Hale V. Bradt ◽  
Saul A. Rappaport
Keyword(s):  
Monte Carlo Simulation ◽  
Monte Carlo ◽  
Three Dimensional ◽  
Extensive Air Showers ◽  
Air Showers
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