Primary proton spectrum between 200 TeV and 1000 TeV observed with the Tibet burst detector and air shower array

被引:57
作者
Amenomori, M [1 ]
Ayabe, S
Caidong
Danzengluobu
Ding, LK
Feng, ZY
Fu, Y
Guo, HW
He, M
Hibino, K
Hotta, N
Huang, Q
Huo, AX
Izu, K
Jia, HY
Kajino, F
Kasahara, K
Katayose, Y
Labaciren
Li, JY
Lu, H
Lu, SL
Luo, GX
Meng, XR
Mizutani, K
Mu, J
Nanjo, H
Nishizawa, M
Ohnishi, M
Ohta, I
Ouchi, T
Peng, ZR
Ren, JR
Saito, T
Sakata, M
Sasaki, T
Shi, ZZ
Shibata, M
Shiomi, A
Shirai, T
Sugimoto, H
Taira, K
Tan, YH
Tateyama, N
Torii, S
Utsugi, T
Wang, CR
Wang, H
Xu, XW
Yamamoto, Y
机构
[1] Hirosaki Univ, Dept Phys, Hirosaki, Aomori 0368561, Japan
[2] Saitama Univ, Dept Phys, Urawa, Saitama 3388570, Japan
[3] Tibet Univ, Dept Math & Phys, Lhasa 850000, Peoples R China
[4] Acad Sinica, Inst High Energy Phys, Lab Cosm Ray & High Energy Astrophys, Beijing 100039, Peoples R China
[5] South West Jiaotong Univ, Dept Phys, Chengdu 610031, Peoples R China
[6] Kanagawa Univ, Fac Engn, Yokohama, Kanagawa 2218686, Japan
[7] Utsunomiya Univ, Fac Educ, Utsunomiya, Tochigi 3218505, Japan
[8] Univ Tokyo, Inst Cosm Ray Res, Kashiwa, Chiba 2778582, Japan
[9] Konan Univ, Dept Phys, Kobe, Hyogo 6588501, Japan
[10] Shibaura Inst Technol, Fac Syst Engn, Omiya, Saitama 3308570, Japan
[11] Yokohama Natl Univ, Fac Engn, Yokohama, Kanagawa 2400067, Japan
[12] Yunnan Univ, Dept Phys, Kunming 650091, Peoples R China
[13] Natl Inst Informat, Tokyo 1018430, Japan
[14] Tokyo Metropolitan Coll Aeronaut Engn, Tokyo 1160003, Japan
[15] Shonan Inst Technol, Fujisawa, Kanagawa 2518511, Japan
[16] Nagoya Univ, Solar Terr Environm Lab, Nagoya, Aichi 4648601, Japan
[17] Shandong Univ, Dept Phys, Jinan 250100, Peoples R China
关键词
D O I
10.1103/PhysRevD.62.112002
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Since 1996, a hybrid experiment consisting of the emulsion chamber and burst detector array and the Tibet-II air-shower array has been operated at Yangbajing (4300 m above sea level, 606 g/cm(2)) in Tibet. This experiment can detect air-shower cores, called bunt events. accompanied by air showers in excess of about 100 TeV. We observed about 4300 burst events accompanied by air showers during 690 days of operation and selected 820 proton-induced events with its primary energy above 200 TeV using a neural network method. Using this data set, we obtained the energy spectrum of primary protons in the energy range from 200 to 1000 TeV. The differential energy spectrum obtained in this energy region can be fitted by a power law with the index of - 2.97 +/- 0.06, which is steeper than that obtained by direct measurements at lower energies. We also obtained the energy spectrum of helium nuclei at particle energies around 1000 TeV.
引用
收藏
页码:1 / 13
页数:13
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