Monte Carlo Simulation for the Propagation of Galactic Cosmic Ray Nuclei

ZHANG Li; ZHANG Ming; MU Jun; YU Chuan-Zan

Chinese Physics C> 1993, Vol. 17> Issue(7) : 589-594

Monte Carlo Simulation for the Propagation of Galactic Cosmic Ray Nuclei

Department of Physics,Yunnan University,Kunming 650091

Abstract
HTML
Reference
Related

PDF

Abstract：
Based on the assumption that galactic cosmic ray(GCR) is produced by the diffusive shock wave acceleration of supernova explosion in the Galaxy,we simulate the propagation of GCR nuclei in the interstellar medium by using the Monte Carlo method.In our simulating calculation,we use the nuclear interaction cross sections and the probabilities of nuclear fragmentation measured in the accelerator experiments;we consider the ionization energy loss of GCR nuclei in the standard leaky box model and the effect of solar modulation on the GCR nuclei by using force-field approximation.Our calculating B/C,V/Fe and the spectra of O and Fe can be compared with experimental data.Finally,we discuss the effects of different compress ratios of shock wave on the calculation results.

References

[1]

Ginzburg, V. L.,andSynovatskii, S. I. 1964, The Origin of Cosmic Rays(New York: Pergamon).[2]Cesarsky, C. J. 20th ICRC Rapporteur, 8(1987),87.[3]Drury, L. O. C. Prog. Phys.,46(1983),973.[4]Ginzburg, V. L.,and Ptuskin, V. S. Rev. Mod. Phys.,48(1976),161.[5]Reams, D. V. 1974, High Energy Particles and Qunta in Astrophysics, edited by Frank B. McDonald and Carl E. Fichtel.[6]Letaw, J. R. Astrophys. J. Suppl.,56(1984),369.[7]Webber, W. R.,et al. Phys. Rev.,C41(1990),533.[8]Silberberg, R.,and Tsao, C. H. Astrophys. J. Suppl.,25(1973),315.[9]Simpson, J. A.,Ann. Reu. Nucl. Part. Sci.,33(1983),323.[10]Ramaty, R.,et al. Solar Phys.,86(1983),395.[11]Gleeson, L. J.,and Axford, W. I.,Astrophys. J.,154(1966),1011.[12]Simon, M.,et al. Astrophys. J.,300(198'6).32.[13]Wiedenback, M. E.,21th ICRC Rapporteur Talk, 11(1990),57.[14]Grunsfeld, J. M.,et al. 21th ICRC, 3(1990),249.[15]Garcia-Muzon, M.,et al, Astrophys. J. Suppl.,64(1987),269.[16]Berezinsky, V. S.,21th ICRC Rapporteur Talk, 11(1990),115.

[1]	LIU Qian , ZHANG Jia-Wen , CHEN Jin , LI Ru-Bai , ZHAO Jian-Bing , HAN Ji-Feng , XIE Yu-Guang , YAO Ning , QI Na-Ding . Cosmic Ray Test Station for BESⅢ RPC. Chinese Physics C, 2006, 30(4): 327-330.
[2]	ZENG Gang , YU Zong-Qiang , YAN Yong-Lian . Beam Hardening Correction Base on Monte Carlo Simulation Method. Chinese Physics C, 2006, 30(2): 178-182.
[3]	YUE Qian , LI Yuan-Jing , CHENG Jian-Ping , WANG Yi , LI Jin , LAI Yong-Fang , LI Qing-Hua , TANG Le . Cosmic-Ray Test and Temperature Effects of MRPC. Chinese Physics C, 2004, 28(11): 1180-1183.
[4]	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. Chinese Physics C, 2004, 28(3): 232-238.
[5]	REN Shao-Jun , SANG Wen-Bin , JIN Wei , LI Wan-Wan , ZHANG Qi , MIN Jia-Hua . Primary Study of Monte Carlo Simulation on CdZnTe Nuclear Detector. Chinese Physics C, 2004, 28(2): 191-195.
[6]	QIU You-Heng , DENG Li , YING Yang-Jun , XIAO Gang . Monte Carlo Simulation of Boron Neutron Capture Therapy. Chinese Physics C, 2003, 27(10): 936-942.
[7]	WANG Yong-Gang , XUE Liang , FENG Cun-Feng , FU Yu , LI Jie , ZHANG Xue-Yao , LI Jin-Yu , ZHANG Nai-Jian , HE Mao , WANG Cheng-Rui , REN Jing-Ru , LU Sui-Ling . Adjustment of Parameters of Primary Cosmic Ray Energy Spectrum with Recent Direct Measurments. Chinese Physics C, 2002, 26(2): 108-115.
[8]	PENG Qiu-He . Where Do the Extra High Energy Cosmic Rays Come From A Model of Active Galactic Nuclei With Magnetic Monopoles. Chinese Physics C, 2002, 26(S1): 104-111.
[9]	Huang Yinzhi , Cheng Baosen , Liu Huaimin , Ma Aimin , Xiong Weijun , Fan Xiaoling , Qi Nading , Zhang Dahua , Chen Shaomin , Xie Yuehong , Li Haibo , Hu Jingliang , Zhang Jinlong . Development and Application of Fast Monte Carlo Simulation Method for Beijing τ-Charm Factory (BTCF). Chinese Physics C, 1997, 21(8): 686-696.
[10]	Xu Chunxian , Dai Hongyue . A Statistic Model for Galactic Cosmic Rays. Chinese Physics C, 1997, 21(6): 486-493.
[11]	CAO Pei-Yuan , WANG Cheng-Rui , HE Mao , ZHANG Nai-Jian , LI Jin-Yu , LI Jie , REN Jing-Ru , LU Sui-Ling . High Energy Gamma Rays and Hadrons in Atmospheric Cosmic Rays. Chinese Physics C, 1992, 16(10): 886-890.
[12]	ZHANG Li , ZHANG Ming , MU Jun , YU Chuan-Zan . Propagation of Cosmic-Ray Nuclei with Reacceleration. Chinese Physics C, 1992, 16(5): 392-397.
[13]	SA Ben-Hao , YANG Xia-Zhou , BAI Xi-Xiang . TRANSPORT THEORY APPROACH TO THE PARTON MULTIPLE SCATTERING IN NUCLEI——MONTE CARLO SIMULATION. Chinese Physics C, 1988, 12(2): 203-207.
[14]	WANG Tai-Jie , WANG Shu-Qin , YAN Wu-Guang , HUANG Yin-Zhi , HUANG De-Qiang , LANG Peng-Fei . SIMPLIFIED MONTE CARLO SIMULATION FOR BEIJING SPECTROMETER. Chinese Physics C, 1986, 10(4): 385-392.
[15]	ZHU Qing-Qi , WU Shi-Pei . SIMULATION CALCULATION FOR DETECTION EFFICIENCY IN THE MEASUREMENT OF COSMIC RAY HADRON SPECTRA. Chinese Physics C, 1985, 9(3): 263-267.
[16]	DING Lin-Kai , JING Gui-Ru . NUCLEAR COMPONENTS OF PRIMARYS COSMIC RAYS AND CLUSTER PHENOMENA IN EMULSION CHAMBER EXPERIMENTS. Chinese Physics C, 1983, 7(2): 129-134.
[17]	ZHANG HE-QI . PROPAGATION OF COSMIC RAY ELECTRONS IN THE GALAXY. Chinese Physics C, 1981, 5(4): 477-483.
[18]	Kuang Hao-huai , Hu Wen-jun , Zhou Yin-zao , Tan You-HENG , Shen Chang-quan , Jang Yin-lin , Zhu Qing-qi , Qin Ke-yu , Li Yan-guo , Wang Li-an . IDENTIFICATION OF THE HORIZONTAL COSIMC RAY PENETRATING PARTICLES. Chinese Physics C, 1980, 4(4): 413-416.
[19]	Ding Lin-kai , Zhu Qing-qi . MONTE-CARLO SIMULATION OF COSMIC RAY ANTIPROTON INTENSITY. Chinese Physics C, 1980, 4(6): 735-740.
[20]	CHANG KONG-LIANG . PROPAGATION EFFECTS OF SOLAR COSMIC RAYS. Chinese Physics C, 1978, 2(5): 385-393.

Access

Get Citation

ZHANG Li, ZHANG Ming, MU Jun and YU Chuan-Zan. Monte Carlo Simulation for the Propagation of Galactic Cosmic Ray Nuclei[J]. Chinese Physics C, 1993, 17(7): 589-594.

ZHANG Li, ZHANG Ming, MU Jun and YU Chuan-Zan. Monte Carlo Simulation for the Propagation of Galactic Cosmic Ray Nuclei[J]. Chinese Physics C, 1993, 17(7): 589-594. shu

RIS(for EndNote,Reference Manager,ProCite)

BibTex

Txt

Milestone

Received: 1900-01-01
Revised: 1900-01-01

Article Metric

Article Views(3879)
PDF Downloads(476)
Cited by(0)

Policy on re-use

To reuse of subscription content published by CPC, the users need to request permission from CPC, unless the content was published under an Open Access license which automatically permits that type of reuse.

通讯作者: 陈斌, bchen63@163.com

1.
沈阳化工大学材料科学与工程学院沈阳 110142

Monte Carlo Simulation for the Propagation of Galactic Cosmic Ray Nuclei

Corresponding author: ZHANG Li,

Department of Physics,Yunnan University,Kunming 650091

Received Date: 1900-01-01

Accepted Date: 1900-01-01

Available Online: 1993-07-05

Abstract: Based on the assumption that galactic cosmic ray(GCR) is produced by the diffusive shock wave acceleration of supernova explosion in the Galaxy,we simulate the propagation of GCR nuclei in the interstellar medium by using the Monte Carlo method.In our simulating calculation,we use the nuclear interaction cross sections and the probabilities of nuclear fragmentation measured in the accelerator experiments;we consider the ionization energy loss of GCR nuclei in the standard leaky box model and the effect of solar modulation on the GCR nuclei by using force-field approximation.Our calculating B/C,V/Fe and the spectra of O and Fe can be compared with experimental data.Finally,we discuss the effects of different compress ratios of shock wave on the calculation results.

HTML

Reference (1)

Monte Carlo Simulation for the Propagation of Galactic Cosmic Ray Nuclei

Abstract：

References

Access

Article Metrics

Metrics

通讯作者: 陈斌, bchen63@163.com

Email This Article