A COSMIC RAY SUPER HIGH ENERGY MULTIJET FAMILY EVENT

ZOU Bao-Tang; WANG Cheng-Rui; REN Jing-Ru

Chinese Physics C> 1986, Vol. 10> Issue(4) : 393-399

A COSMIC RAY SUPER HIGH ENERGY MULTIJET FAMILY EVENT

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Abstract：
A cosmic ray super high energy family event with visible energy of about 1500TeV and five big cores is reported. This event was found in the 1980—1981 exposure of Mt. Kambala(5500M a.s.l.) emulsion chamber experiment. The family characteristics are analized and compared with the other cosmic ray events in the same energy range. The production and fragmentation characteristics of the five jets are studied and compared with the experimntal results of accelerators and C-jets as well as with QCD predictions up to TeV. Some features on hadronic interactions at TeV range are disccused.

References

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ZOU Bao-Tang, WANG Cheng-Rui and REN Jing-Ru. A COSMIC RAY SUPER HIGH ENERGY MULTIJET FAMILY EVENT[J]. Chinese Physics C, 1986, 10(4): 393-399.

ZOU Bao-Tang, WANG Cheng-Rui and REN Jing-Ru. A COSMIC RAY SUPER HIGH ENERGY MULTIJET FAMILY EVENT[J]. Chinese Physics C, 1986, 10(4): 393-399. shu

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Received: 1900-01-01
Revised: 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

A COSMIC RAY SUPER HIGH ENERGY MULTIJET FAMILY EVENT

Corresponding author: ZOU Bao-Tang,

Received Date: 1900-01-01

Accepted Date: 1900-01-01

Available Online: 1986-08-05

Abstract: A cosmic ray super high energy family event with visible energy of about 1500TeV and five big cores is reported. This event was found in the 1980—1981 exposure of Mt. Kambala(5500M a.s.l.) emulsion chamber experiment. The family characteristics are analized and compared with the other cosmic ray events in the same energy range. The production and fragmentation characteristics of the five jets are studied and compared with the experimntal results of accelerators and C-jets as well as with QCD predictions up to TeV. Some features on hadronic interactions at TeV range are disccused.

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