Study on the Production Characteristics of Cosmic Ray High Energy Family Events with Simulation and Experiment

WANG Kong-Sen; WANG He; HUANG Xing-Tao; MA Lian-Liang; MA Li-Na; WANG Yong-Gang; XUE Liang; FENG Cun-Feng; ZHANG Xue-Yao; LI Jin-Yu; ZHANG Nai-Jian; HE Mao; WANG Cheng-

Chinese Physics C> 2004, Vol. 28> Issue(3) : 232-238

Study on the Production Characteristics of Cosmic Ray High Energy Family Events with Simulation and Experiment

Department of Physics,Shandong University,Ji'nan 250100,China2 Institute of High Energy Physics,CAS,Beijing 100039,China

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Abstract：
A Monte Carlo simulation on production characteristics of high energy family events observed with Mt. Kanbala emulsion chambers is made based on hadronic interaction models QGSJET and DPMJET with program CORSIKA which is commonly used in the simulations of EAS experiments. The production efficiency of family events for different primary particles and its relationship with primary energies are given. The distributions of lateral spreads, numbers of showers, total visible energies of the family events and their corresponding average values got from simulations are systematically compared with those of the experiment. It shows that their results are consistent basically. Additionally, family events from both simulations and experiment have the similar tendency of energy concentration.

References

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WANG Kong-Sen, WANG He, HUANG Xing-Tao, MA Lian-Liang, MA Li-Na, WANG Yong-Gang, XUE Liang, FENG Cun-Feng, ZHANG Xue-Yao, LI Jin-Yu, ZHANG Nai-Jian, HE Mao, WANG Cheng-, Study on the Production Characteristics of Cosmic Ray High Energy Family Events with Simulation and Experiment[J]. Chinese Physics C, 2004, 28(3): 232-238.

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Received: 2003-06-16
Revised: 1900-01-01

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通讯作者: 陈斌, bchen63@163.com

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沈阳化工大学材料科学与工程学院沈阳 110142

Study on the Production Characteristics of Cosmic Ray High Energy Family Events with Simulation and Experiment

Corresponding author: WANG Kong-Sen,

Department of Physics,Shandong University,Ji'nan 250100,China2 Institute of High Energy Physics,CAS,Beijing 100039,China

Received Date: 2003-06-16

Accepted Date: 1900-01-01

Available Online: 2004-03-05

Abstract: A Monte Carlo simulation on production characteristics of high energy family events observed with Mt. Kanbala emulsion chambers is made based on hadronic interaction models QGSJET and DPMJET with program CORSIKA which is commonly used in the simulations of EAS experiments. The production efficiency of family events for different primary particles and its relationship with primary energies are given. The distributions of lateral spreads, numbers of showers, total visible energies of the family events and their corresponding average values got from simulations are systematically compared with those of the experiment. It shows that their results are consistent basically. Additionally, family events from both simulations and experiment have the similar tendency of energy concentration.

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Study on the Production Characteristics of Cosmic Ray High Energy Family Events with Simulation and Experiment

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