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

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

  • 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.
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    [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.

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

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