Statistic Model for Galactic Cosmic Rays

Xu Chunxian; Dai Hongyue

Chinese Physics C> 1997, Vol. 21> Issue(S2) : 25-32

Statistic Model for Galactic Cosmic Rays

Xu Chunxian ¹ ,
Dai Hongyue ²

1. Institute of High Energy Physics, the Chinese Academy of Sciences, Beijing, China;
2. Department of Physics, University of Utah, Salt Lake City, UT 84112 U. S. A

Abstract
HTML
Reference
Related

PDF

Abstract：
This paper supposes that all cosmic ray (CR) particles of energy below 3×10¹⁸eV mainly originate and accelerate in an individual explosion of the supernova (SN) in the Galaxy; with the use of an isotropic diffusion propagation model, the non-steady state density distribution of Iron nuclei is investigated. Considering the effect of extragalactic CRs and the variety of the galactic CR nuclei, the statistic model of galactic CRs with a reasonable distribution of the galactic SNs in space and time can account for the spectrum of CRs in the energy range of 10¹²-10²⁰eV quite well.
- primary cosmic rays ,
- cosmic ray composition ,
- cosmic ray spectra ,
- cosmic ray propagation

[1]	Ran Ding , Zhi-Long Han , Li Huang , Yi Liao . Phenomenology of colored radiative neutrino mass model and its implications on cosmic-ray observations. Chinese Physics C, 2018, 42(10): 103101. doi: 10.1088/1674-1137/42/10/103101
[2]	Tian-Lu Chen , Wei Liu , Qi Gao , Mao-Yuan Liu , Hai-Jin Li , Danzengluobu , Ying Shi . Cosmic ray electron spectrum due to the dispersion ofinjection spectrum. Chinese Physics C, 2018, 42(7): 075001. doi: 10.1088/1674-1137/42/7/075001
[3]	Chao Jin , Yi-Qing Guo , Hong-Bo Hu . Spatial dependent diffusion of cosmic rays and the excess of primary electrons derived from high precision measurements by AMS-02. Chinese Physics C, 2016, 40(1): 015101. doi: 10.1088/1674-1137/40/1/015101
[4]	Yong-ji Xie , Zhong-hua Qin , Xiao-yan Ma , Jian Zhang , Ling-hui Wu , Wan Xie , Ming-yi Dong , Jing Dong , Xiao-lu Ji , Xiao-shan Jiang , Qun Ou-yang , Ke-jun Zhu , Yuan-bo Chen . Construction and cosmic-ray test of the new inner drift chamber for BESIII. Chinese Physics C, 2016, 40(9): 096003. doi: 10.1088/1674-1137/40/9/096003
[5]	CHEN Tian-Xiang , LI Cheng , SUN Yong-Jie , CHEN Hong-Fang , SHAO Ming , TANG Ze-Bo , YANG Rong-Xing , ZHOU Yi , ZHANG Yi-Fei . A cosmic ray test platform based on high time resolution MRPC technology. Chinese Physics C, 2015, 39(5): 056003. doi: 10.1088/1674-1137/39/5/056003
[6]	ZHANG Fei , FAN Rui-Rui , PENG Wen-Xi , DONG Yi-Fan , GONG Ke , LIANG Xiao-Hua , LIU Ya-Qing , WANG Huan-Yu . A prototype silicon detector system for space cosmic-ray charge measurement. Chinese Physics C, 2014, 38(6): 066101. doi: 10.1088/1674-1137/38/6/066101
[7]	WU Yu-Cheng , HAO Xi-Qing , YUE Qian , LI Yuan-Jing , CHENG Jian-Ping , KANG Ke-Jun , CHEN Yun-Hua , LI Jin , LI Jian-Min , LI Yu-Lan , LIU Shu-Kui , MA Hao , REN Jin-Bao , SHEN Man-Bin , WANG Ji-Min , WU Shi-Yong , XUE Tao , YI Nan , ZENG Xiong-Hui , ZENG Zhi , ZHU Zhong-Hua . Measurement of cosmic ray flux in the China JinPing underground laboratory. Chinese Physics C, 2013, 37(8): 086001. doi: 10.1088/1674-1137/37/8/086001
[8]	GE Yong-Shuai , WANG Zhi-Gang , YU Bo-Xiang , XIE Yu-Guang , ZHANG Ai-Wu , XUE Zhen , LIU Ying-Biao , GAO Long , NIU Shun-Li , CAI Xiao , FANG Jian , SUN Xi-Lei , NING Fei-Peng , ZHOU Li , HU Tao , , . A novel 2-dimensional cosmic ray position detector based on a CsI(Na) pixel array and an ICCD camera. Chinese Physics C, 2012, 36(11): 1101-1105. doi: 10.1088/1674-1137/36/11/011
[9]	FU Zai-Wei , QIAN Sen , NING Zhe , LIU Shu-Dong , CHEN Xiao-Hui , HENG Yue-Kun , WANG Yi-Fang , QI Ming , YANG Shuai , SUN Yong-Jie , SHAO Ming , LI Cheng , ZHENG Yang-Heng . Cosmic ray test for a T0 detector. Chinese Physics C, 2011, 35(10): 946-951. doi: 10.1088/1674-1137/35/10/011
[10]	YUE Ke , YU Yu-Hong , XU Hu-Shan , SUN Zhi-Yu , WANG Jian-Song , XIAO Zhi-Gang , HU Zheng-Guo , CHEN Ruo-Fu , ZHANG Xue-Ying , TU Xiao-Lin , CHEN Jun-Ling , ZHAN Wen-Long . Characteristics of the sampling paddle modules of neutron wall from the cosmic ray test. Chinese Physics C, 2010, 34(8): 1111-1115. doi: 10.1088/1674-1137/34/8/014
[11]	WU Zhi , LIU Jian-Bei , QIN Zhong-Hua , WU Ling-Hui , CHEN Chang , CHEN Yuan-Bo , CHEN Ma-Li , CHEN Xi-Hui , DONG Ming-Yi , GUAN Bei-Ju , HUANG Jie , JIANG Xiao-Shan , JIN Yan , LI Fei , LI Ren-Ying , LI Xiao-Nan , LEI Guang-Kun , LIU Rong-Guang , LUO Xiao-Lan , MA Xiao-Yan , SHENG Hua-Yi , SUN Han-Sheng , TANG Xiao , WANG Lan , WANG Liang , XU Mei-Hang , ZHANG Jian , ZHANG Hong-Yu , ZHANG Yin-Hong , ZHAO Yu-Bin , ZHAO Ping-Ping , ZHU Ke-Jun , ZHU Qi-Ming , ZHUANG Bao-An . Tuning of the cosmic-ray test system of the BESⅢ drift chamber. Chinese Physics C, 2010, 34(7): 983-987. doi: 10.1088/1674-1137/34/7/010
[12]	YAN Jie , SUN Sheng-Sen , LI Cheng , HE Kang-Lin . BESⅢ barrel time-of-flight (TOF) calibration using cosmic ray data. Chinese Physics C, 2010, 34(3): 368-373. doi: 10.1088/1674-1137/34/3/012
[13]	LIANG Yu-Tie , MAO Ya-Jun , YOU Zheng-Yun . Study of BESⅢ MUC offline software with cosmic-ray data. Chinese Physics C, 2009, 33(7): 562-566. doi: 10.1088/1674-1137/33/7/011
[14]	XU Mei-Hang , CHEN Chang , CHEN Yuan-Bo , WU Zhi , QIN Zhong-Hua , WU Ling-Hui , LIU Jian-Bei , WANG Lan , JIN Yan , LIU Rong-Guang , ZHU Qi-Ming , ZHANG Jian , HUANG Jie . Installation and cosmic ray test of the high voltage system of the BESⅢ drift chamber. Chinese Physics C, 2008, 32(12): 992-994. doi: 10.1088/1674-1137/32/12/010
[15]	CHEN Xi-Hui , XIE Xiao-Xi , LI Xiao-Nan , GAO Cui-Shan , ZHANG Yin-Hong , NIE Zhen-Dong , MIN Jian , XIE Yi-GANG . Design and implementation of the detector control system for the BESⅢ drift chamber cosmic ray test. Chinese Physics C, 2008, 32(8): 649-652. doi: 10.1088/1674-1137/32/8/012
[16]	Liu Shaomin , Ding Linkai , Shi Ce , Zhaxiciren , Zhaxisanzhu , Mu Jun , Wnag Hui , Lu Hong , Feng Zhenyong , Ren Jingru , Yu Guangce , Zhou Wende , Labaciren , Meng Xianru , Meng Lie , Zhang Jilong , Zhang Chunsheng , Zhang Huimin , Shi Zhizheng , Jia Huanyiu , Mei Dongming , Huang Qing , Tan Youheng , Huo Anxiang , Dai Benzhong . Correlation Between Sun Shadows of 10 TeV Cosmic Ray and the Solar Activity. Chinese Physics C, 1997, 21(S4): 11-18.
[17]	Luo Guangxuan , Tan Youheng , Zhang Chunsheng , Dong Yuju , Yuan Peng , Zhang Huimin , Wang Hui , Yuang Yukui , Li Jing . Energy Spectrum of Primary Cosmic Rays at the “Knee” Region Observed with the Huairou Air Shower Array. Chinese Physics C, 1995, 19(S4): 325-331.
[18]	Jiang Yinlin . Atmospheric Cherenkov Images of Cosmic Ray Muons. Chinese Physics C, 1995, 19(S1): 5-11.
[19]	Cao Zhen , Ding Linkai . Generator of QCD Parton Model for the Cosmic Ray Ultrahigh Energy Interaction. Chinese Physics C, 1994, 18(S4): 321-332.
[20]	Lu Suiling , Ren Jingru , Su Shi , Wang Chengrui , He Mao . Variation of the Intensity of High Energy Cosmic Ray Hadrons with Altitude. Chinese Physics C, 1992, 16(S2): 123-125.

Access

Get Citation

Xu Chunxian and Dai Hongyue. Statistic Model for Galactic Cosmic Rays[J]. Chinese Physics C, 1997, 21(S2): 25-32.

Xu Chunxian and Dai Hongyue. Statistic Model for Galactic Cosmic Rays[J]. Chinese Physics C, 1997, 21(S2): 25-32. shu

RIS(for EndNote,Reference Manager,ProCite)

BibTex

Txt

Milestone

Received: 1996-07-03

Article Metric

Article Views(529)
PDF Downloads(2)
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

Statistic Model for Galactic Cosmic Rays

1. Institute of High Energy Physics, the Chinese Academy of Sciences, Beijing, China;

2. Department of Physics, University of Utah, Salt Lake City, UT 84112 U. S. A

Received Date: 1996-07-03

Abstract: This paper supposes that all cosmic ray (CR) particles of energy below 3×10¹⁸eV mainly originate and accelerate in an individual explosion of the supernova (SN) in the Galaxy; with the use of an isotropic diffusion propagation model, the non-steady state density distribution of Iron nuclei is investigated. Considering the effect of extragalactic CRs and the variety of the galactic CR nuclei, the statistic model of galactic CRs with a reasonable distribution of the galactic SNs in space and time can account for the spectrum of CRs in the energy range of 10¹²-10²⁰eV quite well.

Statistic Model for Galactic Cosmic Rays

Abstract：

Access

Article Metrics

Metrics

通讯作者: 陈斌, bchen63@163.com

Email This Article

Statistic Model for Galactic Cosmic Rays

HTML

目录