ANALYSIS ON COSMIC RAY MULTI-μ PHENOMENA IN ENERGY REGION 10<SUP>14</SUP>—10<SUP>16</SUP>eV

JING Cai-Liu; JING Gui-Ru; DING Lin-Kai; ZHU Qing-Qi

Chinese Physics C> 1985, Vol. 9> Issue(2) : 134-141

ANALYSIS ON COSMIC RAY MULTI-μ PHENOMENA IN ENERGY REGION 10¹⁴—10¹⁶eV

Abstract
HTML
Reference
Related

PDF

Abstract：
Under the condition of the primary cosmic ray incidence with different composition, the multi-μ phenomena are simulated by the scaling model of the hadronic interactions included by the mechanism of jet production with large transverse momentum The results show that the primary heavy heavy nuclei contribute significantly to the large μ-multiplicity events observed at deep underground. But even the heavy nucleus dominant primary model is used, the multi-μ event rate simulated is still lower than the experimental data and it suggests the existence of other multi-μ sources. The lateral distribution of multi-μ events is in accordance with experiments.

References

[1]

S. Miyake et al.. Journal of Phys. Soc. of Japan. 18(1963), 464.[2] Y. Muraki, 17th ICRC, Paris, 7(1981), MN 3-8.[3] M. R. Krishnaswamy et al., 16th ICRC, Kyoto, 13(1979), 378.[4] J. W. Elbert et al., 17th ICRC, Paris, 7(1981), 42.[5] Y. N. Vavilov et al., 17th ICRC, Paris, 7(1951), 38.[6] J. W. Elbert et al., Phys. Rev., D27(1983), 1448.[7] T. Aoki et al., 18th ICRC, Bangalore, 7(1983), 58.P. K. F. Grieder, 18th ICRC, Bangalore, 7(1983), 59.T. L. Asatiani et al.. 18th ICRC, Bangalore, 7f 1983), 60.[8] M. R. Krishnaswamy et al., 18th ICRC, BangaIore, 7(1983), 52.T. K. Gaisser et aI., 18th ICRC, Bangalore, 7(1983), 5 3Y. Muraki et aI., 18th ICRC, Bangalore, 7(1983), 54.[9] J. G. Rushbroke, CERN/EP 82-157, (1982).[10] 丁林恺、朱清棋、郭可尊, 高能物理与核物理, 6(1982) 657, Ding Lin-Kai et al.,ICR-Repo rt-107-83-8-1(1983).[11] 丁林恺、荆贵茹, 高能物理与核物理, 7(1983), 129,[12] M. R. Krishnaswamy et al., 15th ICRC, Plovdiv,6(1977), 161.

[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]	YANG Hong-Tao , LIU Jun , GENG Qing-Xi , LIU Chang-Qin , ZHANG Pin , GAO Xiao-Yu , ZHA Min , JING Gui-Ru , JING Cai-Liu , ZHU Qing-Qi , Cheung T , Leung K , NG L . The Study of Primary Cosmic Ray Mass Composition Around the. Chinese Physics C, 2006, 30(6): 497-500.
[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]	LIU Zhen-An . Z⁰ Data Analysis in L3 Cosmic-Ray Experiment. Chinese Physics C, 2003, 27(5): 395-398.
[5]	FENG CunFeng , ZHANG XueYao , KONG FanMin , HE Mao , FU Yu , DAI ZhiQiang , ZHANG NaiJian . Relation between Interactive Models and Identification of Primary Cosmic Ray Components at the “Knee”. Chinese Physics C, 2000, 24(6): 467-472.
[6]	XUE Liang , DAI ZhiQiang , LI Jinyu , ZHANG Xueyao , FENG CunFeng , FU Yu , ZHANG NaiJian , REN JingRu , LU SuiLing . Phenomenon of Alignment in Cosmic Ray High Energy Family Events. Chinese Physics C, 2000, 24(11): 979-984.
[7]	Ding Linkal , Zhu Qingqi , Shen Changquan , Yao Zhiguo , Cheung Tsang , Matti Vallinkoski . An Approach to Study the Cosmic Ray ‘Knee’Composition From Underground Multimuon Events at a Shallower Depth. Chinese Physics C, 1999, 23(6): 584-588.
[8]	Xu Chunxian , Dai Hongyue . A Statistic Model for Galactic Cosmic Rays. Chinese Physics C, 1997, 21(6): 486-493.
[9]	Luo Guangxuan , Tan Youheng , Zhang Chunsheng , Dong Yuju , Yuan Peng , Zhang Huimin , Wang Hui , Yuan Yukui , Li Jing . Primary Energy Spectrum of Cosmic Ray at the. Chinese Physics C, 1995, 19(9): 769-774.
[10]	Jia Huanyu , Cao Zhen , Zhang Huimin . The Study of Meteorological Effects on TeV Cosmic Ray Flux. Chinese Physics C, 1994, 18(9): 788-793.
[11]	ZHU Yong-Sheng , ZHANG Liang-Sheng , GAO Wen-Xiu , ZHANG Ying-Ping , ZHAO Ping-De , ZHANG Jia-Wen , LI Fang , CHEN Le-Jun , XU Zhi-Qing . THE COSMIC RAY DATA ANALYSIS OF μ-COUNTER ARRAY IN BES. Chinese Physics C, 1990, 14(2): 102-109.
[12]	XU Ke-Zun , ZHANG Zhen-Hua , TANG Zi-Zhou , WANG Ming-Qian . MEASUREMENT OF THE ENERGY SPECTRUM OF PRIMARY COSMIC PAYS. Chinese Physics C, 1987, 11(1): 1-5.
[13]	HE Yu-Dong , ZHOU Wen-De , HE Ren-Dao , MU Jun , DING Lin-Kai , ZHU Qing-Qi , JING Cai-Liu , JING Gui-Ru . AN ANALYSIS OF PRIMARY COSMIC RAY COMPOSITION AT ENERGIES AROUND 10¹⁴eV USING SINGLE-SHOWER EVENTS OBSERVED BY MOUNTAIN EMULSION CHAMBER. Chinese Physics C, 1986, 10(6): 641-646.
[14]	JING Cai-Liu , DING Lin-Kai , ZHU QiNG-Qi , JING Gui-Ru . A DEDUCTION ON PRIMARY COSMIC PAY COMPOSITION AND SPECTRA ABOVE 10¹⁴eV. Chinese Physics C, 1986, 10(5): 636-640.
[15]	XU Chun-Xian . THE ANISOTROPY OF COSMIC RAY PARTICLES IN THE ENERGY RANGE 10¹¹—10¹⁹eV. Chinese Physics C, 1985, 9(4): 385-390.
[16]	CHEN Ying-Xuan , HE Chang-Xiao , XIAO Qian-Yi , WANG Li-Xiang . THE TIME DISTRIBUTION OF EAS WITH E>10¹⁴eV. Chinese Physics C, 1985, 9(4): 391-396.
[17]	SUN Luo-Rui . A SYUDY OF ENERGY SPECTRUM OF COSMIC RAYS RANGING FROM 6×10¹⁴ TO 5×10¹⁶eV. Chinese Physics C, 1984, 8(4): 502-507.
[18]	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.
[19]	DING LIN-KAI , ZHU QING-QI , GUO KE-ZHUN . CLUSTER PHENOMENA OBSERVED IN EMULSION CHAMBER EXPERIMENTS IN ENERGY REGION OF 10¹⁵—10¹⁶ eV AND HADRON JETS WITH LARGE TRANSVERSE MOMENTA. Chinese Physics C, 1982, 6(6): 657-664.
[20]	CHANG KONG-LIANG . DIMENSIONAL METHOD TO SOLVE THE DIFFUSION CONVECTION EQUATION OF SOLAR COSMIC RAYS. Chinese Physics C, 1978, 2(3): 200-210.

Access

Get Citation

JING Cai-Liu, JING Gui-Ru, DING Lin-Kai and ZHU Qing-Qi. ANALYSIS ON COSMIC RAY MULTI-μ PHENOMENA IN ENERGY REGION 10¹⁴—10¹⁶eV[J]. Chinese Physics C, 1985, 9(2): 134-141.

JING Cai-Liu, JING Gui-Ru, DING Lin-Kai and ZHU Qing-Qi. ANALYSIS ON COSMIC RAY MULTI-μ PHENOMENA IN ENERGY REGION 10¹⁴—10¹⁶eV[J]. Chinese Physics C, 1985, 9(2): 134-141. shu

RIS(for EndNote,Reference Manager,ProCite)

BibTex

Txt

Milestone

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

Article Metric

Article Views(2475)
PDF Downloads(464)
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

ANALYSIS ON COSMIC RAY MULTI-μ PHENOMENA IN ENERGY REGION 10¹⁴—10¹⁶eV

Corresponding author: JING Cai-Liu,

Received Date: 1900-01-01

Accepted Date: 1900-01-01

Available Online: 1985-04-05

Abstract: Under the condition of the primary cosmic ray incidence with different composition, the multi-μ phenomena are simulated by the scaling model of the hadronic interactions included by the mechanism of jet production with large transverse momentum The results show that the primary heavy heavy nuclei contribute significantly to the large μ-multiplicity events observed at deep underground. But even the heavy nucleus dominant primary model is used, the multi-μ event rate simulated is still lower than the experimental data and it suggests the existence of other multi-μ sources. The lateral distribution of multi-μ events is in accordance with experiments.

HTML

Reference (1)

ANALYSIS ON COSMIC RAY MULTI-μ PHENOMENA IN ENERGY REGION 10¹⁴—10¹⁶eV

Abstract：

References

Access

Article Metrics

Metrics

通讯作者: 陈斌, bchen63@163.com

Email This Article

ANALYSIS ON COSMIC RAY MULTI-μ PHENOMENA IN ENERGY REGION 10¹⁴—10¹⁶eV

Corresponding author: JING Cai-Liu,

HTML

目录

ANALYSIS ON COSMIC RAY MULTI-μ PHENOMENA IN ENERGY REGION 1014—1016eV

Abstract：

References

Access

Article Metrics

Metrics

通讯作者: 陈斌, bchen63@163.com

Email This Article

ANALYSIS ON COSMIC RAY MULTI-μ PHENOMENA IN ENERGY REGION 1014—1016eV

Corresponding author: JING Cai-Liu,

HTML

目录

ANALYSIS ON COSMIC RAY MULTI-μ PHENOMENA IN ENERGY REGION 10¹⁴—10¹⁶eV

ANALYSIS ON COSMIC RAY MULTI-μ PHENOMENA IN ENERGY REGION 10¹⁴—10¹⁶eV