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

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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

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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
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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

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

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

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

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

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