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Measurement of attenuation length of the muon content in extensive air showers from 0.3 to 30 PeV with LHAASO
Cao, Zhen1,2,3; Aharonian, F.4,5; Axikegu6; Bai, Y. X.1,3; Bao, Y. W.7; Bastieri, D.8; Bi, X. J.1,2,3; Bi, Y. J.1,3; Bian, W.9; Bian, W.9; Bukevich, A. V.10; Cao, Q.11; Cao, W. Y.12; Cao, Zhe12,13; Chang, J.14; Chang, J. F.1,3,13; Chen, A. M.9; Chen, E. S.1,2,3; Chen, H. X.15; Chen, Liang16; Chen, Lin6; Chen, Long6; Chen, M. J.1,3; Chen, M. L.1,3,13; Chen, Q. H.6; Chen, S.17; Chen, S. H.1,2,3; Chen, S. Z.1,3; Chen, T. L.18; Chen, Y.7; Cheng, N.1,3; Cheng, Y. D.1,2,3; Chu, M. C.19; Cui, M. Y.14; Cui, S. W.11; Cui, X. H.20; Cui, Y. D.21; Dai, B. Z.17; Dai, H. L.1,3,13; Dai, Z. G.12; Danzengluobu18; Dong, X. Q.1,2,3; Duan, K. K.14; Fan, J. H.8; Fan, Y. Z.14; Fang, J.17; Fang, J. H.15; Fang, K.1,3; Feng, C. F.22; Feng, H.1; Feng, L.14; Feng, S. H.1,3; Feng, X. T.22; Feng, Y.15; Feng, Y. L.18; Gabici, S.23; Gao, B.1,3; Gao, C. D.22; Gao, Q.18; Gao, W.1,3; Gao, W. K.1,2,3; Ge, M. M.17; Ge, T. T.24; Geng, L. S.1,3; Giacinti, G.9; Gong, G. H.25; Gou, Q. B.1,3; Gu, M. H.1,3,13; Guo, F. L.16; Guo, J.25; Guo, X. L.6; Guo, Y. Q.1,3; Guo, Y. Y.14; Han, Y. A.26; Hannuksela, O. A.19; Hasan, M.1,2,3; He, H. H.1,2,3; He, H. N.14; He, J. Y.14; He, Y.6; Hor, Y. K.24; Hou, B. W.1,2,3; Hou, C.1,3; Hou X(侯贤)27; Hu, H. B.1,2,3; Hu, Q.12,14; Hu, S. C.1,3,28; Huang, C.7; Huang, D. H.6; Huang, T. Q.1,3; Huang, W. J.24; Huang, X. T.22; Huang, X. Y.14; Huang, Y.1,2,3; Huang, Y. Y.7; Ji, X. L.1,3,13; Jia, H. Y.6; Jia, K.22; Jiang, H. B.1,3; Jiang, K.12,13; Jiang, X. W.1,3; Jiang, Z. J.17; Jin, M.6; Kang, M. M.29; Karpikov, I.10; Khangulyan, D.1,3; Kuleshov, D.10; Kurinov, K.10; Li, B. B.11; Li, C. M.7; Li, Cheng12,13; Li, Cong1,3; Li, D.1,2,3; Li, F.1,3,13; Li, H. B.1,3; Li, H. C.1,3; Li, Jian12; Li, Jie1,3,13; Li, K.1,3; Li, S. D.2,16; Li, W. L.22; Li, W. L.9; Li, X. R.1,3; Li, Xin12,13; Li, Y. Z.1,2,3; Li, Zhe1,3; Li, Zhuo30; Liang, E. W.31; Liang, Y. F.31; Lin, S. J.24; Liu, B.12; Liu, C.1,3; Liu, D.22; Liu, D. B.9; Liu, H.6; Liu, H. D.26; Liu, J.1,3; Liu, J. L.1,3; Liu, M. Y.18; Liu, R. Y.7; Liu, S. M.6; Liu, W.1,3; Liu, Y.8; Liu, Y. N.25; Luo, Q.24; Luo, Y.9; Lv, H. K.1,3; Ma, B. Q.30; Ma, L. L.1,3; Ma, X. H.1,3; Mao JR(毛基荣)27; Min, Z.1,3; Mitthumsiri, W.32; Mu, H. J.26; Nan, Y. C.1,3; Neronov, A.23; Ng, K. C. Y.19; Ou, L. J.8; Pattarakijwanich, P.32; Pei, Z. Y.8; Qi, J. C.1,2,3; Qi, M. Y.1,3; Qiao, B. Q.1,3; Qin, J. J.12; Raza, A.1,2,3; Ruffolo, D.32; Sáiz, A.32; Saeed, M.1,2,3; Semikoz, D.23; Shao, L.11; Shchegolev, O.10,33; Sheng, X. D.1,3; Shu, F. W.34; Song, H. C.30; Stenkin, Yu. V.10,33; Stepanov, V.10; Su, Y.14; Sun, D. X.12,14; Sun, Q. N.6; Sun, X. N.31; Sun, Z. B.35; Takata, J.36; Tam, P. H. T.24; Tang, Q. W.34; Tang, R.9; Tang, Z. B.12,13; Tian, W. W.2,20; Wan, L. H.24; Wang, C.35; Wang, C. B.6; Wang, G. W.12; Wang, H. G.8; Wang, H. H.24; Wang JC(王建成)27; Wang, Kai7; Wang, Kai36; Wang, L. P.1,2,3; Wang, L. Y.1,3; Wang, P. H.6; Wang, R.22; Wang, W.24; Wang, X. G.31; Wang, X. Y.7; Wang, Y.6; Wang, Y. D.1,3; Wang, Y. J.1,3; Wang, Z. H.29; Wang, Z. X.17; Wang, Zhen9; Wang, Zheng1,3,13; Wei, D. M.14; Wei, J. J.14; Wei, Y. J.1,2,3; Wen, T.17; Wu, C. Y.1,3; Wu, H. R.1,3; Wu, Q. W.36; Wu, S.1,3; Wu, X. F.14; Wu, Y. S.12; Xi, S. Q.1,3; Xia, J.12,14; Xiang, G. M.2,16; Xiao, D. X.11; Xiao, G.1,3; Xin, Y. L.6; Xing, Y.16; Xiong DR(熊定荣)27; Xiong, Z.1,2,3; Xu, D. L.9; Xu, R. F.1,2,3; Xu, R. X.30; Xu, W. L.29; Xue, L.22; Yan, D. H.17; Yan, J. Z.14; Yan, T.1,3; Yang, C. W.29; Yang CY(杨初源)27; Yang, F.11; Yang, F. F.1,3,13; Yang, L. L.24; Yang, M. J.1,3; Yang, R. Z.12; Yang, W. X.8; Yao, Y. H.1,3; Yao, Z. G.1,3; Yin, L. Q.1,3; Yin, N.22; You, X. H.1,3; You, Z. Y.1,3; Yu, Y. H.12; Yuan, Q.14; Yue, H.1,2,3; Zeng, H. D.14; Zeng, T. X.1,3,13; Zeng, W.17; Zha, M.1,3; Zhang, B. B.7; Zhang, F.6; Zhang, H.9; Zhang, H. M.7; Zhang, H. Y.17; Zhang, J. L.20; Zhang, Li17; Zhang, P. F.17; Zhang, P. P.12,14; Zhang, R.14; Zhang, S. B.2,20; Zhang, S. R.11; Zhang, S. S.1,3; Zhang, X.7; Zhang, X. P.1,3; Zhang, Y. F.6; Zhang, Yi1,14; Zhang, Yong1,3; Zhao, B.6; Zhao, J.1,3; Zhao, L.12,13; Zhao, L. Z.11; Zhao, S. P.14; Zhao XH(赵晓红)27; Zheng, F.35; Zhong, W. J.7; Zhou, B.1,3; Zhou, H.9; Zhou, J. N.16; Zhou, M.34; Zhou, P.7; Zhou, R.29; Zhou, X. X.1,2,3; Zhou, X. X.6; Zhu, B. Y.12,14; Zhu, C. G.22; Zhu, F. R.6; Zhu, H.20; Zhu, K. J.1,2,3,13; Zou, Y. C.36; Zuo, X.1,3
发表期刊PHYSICAL REVIEW D
2024-11-14
卷号110期号:10
DOI10.1103/PhysRevD.110.103017
产权排序第27完成单位
收录类别SCI
摘要The attenuation length of the muon content in extensive air showers provides important information regarding the generation and development of air showers. This information can be used not only to improve the description of such showers but also to test fundamental models of hadronic interactions. Using data from the LHAASO-KM2A experiment, the development of the muon content in high-energy air showers was studied. The attenuation length of muon content in the air showers was measured from experimental data in the energy range from 0.3 to 30 PeV using the constant intensity cut method. By comparing the attenuation length of the muon content with predictions from high-energy hadronic interaction models (QGSJET-II-04, SIBYLL 2.3d, and EPOS-LHC), it is evident that LHAASO results are significantly shorter than those predicted by the first two models (QGSJET-II-04 and SIBYLL 2.3d) but relatively close to those predicted by the third model (EPOS-LHC). Thus, the LHAASO data favor the EPOS-LHC model over the other two models. The three interaction models confirmed an increasing trend in the attenuation length as the cosmic-ray energy increases.
资助项目Chengdu Management Committee of Tianfu New Area; National Natural Science Foundation of China[12175121]; National Natural Science Foundation of China[12275280]; National Natural Science Foundation of China[12393851]; National Natural Science Foundation of China[12393852]; National Natural Science Foundation of China[12393853]; National Natural Science Foundation of China[12393854]; National Natural Science Foundation of China[12205314]; National Natural Science Foundation of China[12105301]; National Natural Science Foundation of China[12305120]; National Natural Science Foundation of China[12261160362]; National Natural Science Foundation of China[12105294]; National Natural Science Foundation of China[U1931201]; National Natural Science Foundation of China[12375107]; National Science and Technology Development Agency (NSTDA); National Research Council of Thailand (NRCT) under the High-Potential Research Team Grant Program[N42A650868]
项目资助者Chengdu Management Committee of Tianfu New Area ; National Natural Science Foundation of China[12175121, 12275280, 12393851, 12393852, 12393853, 12393854, 12205314, 12105301, 12305120, 12261160362, 12105294, U1931201, 12375107] ; National Science and Technology Development Agency (NSTDA) ; National Research Council of Thailand (NRCT) under the High-Potential Research Team Grant Program[N42A650868]
语种英语
学科领域天文学 ; 天体物理学 ; 高能天体物理学 ; 星系与宇宙学
文章类型Article
出版者AMER PHYSICAL SOC
出版地ONE PHYSICS ELLIPSE, COLLEGE PK, MD 20740-3844 USA
ISSN2470-0010
URL查看原文
WOS记录号WOS:001381876900001
WOS研究方向Astronomy & Astrophysics ; Physics
WOS类目Astronomy & Astrophysics ; Physics, Particles & Fields
关键词[WOS]ENERGY-SPECTRUM
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文献类型期刊论文
版本出版稿
条目标识符http://ir.ynao.ac.cn/handle/114a53/27982
专题星系类星体研究组
高能天体物理研究组
南方基地
作者单位1.Key Laboratory of Particle Astrophysics and Experimental Physics Division and Computing Center, Institute of High Energy Physics, Chinese Academy of Sciences, 100049 Beijing, China;
2.University of Chinese Academy of Sciences, 100049 Beijing, China;
3.TIANFU Cosmic Ray Research Center, Chengdu, Sichuan, China;
4.Dublin Institute for Advanced Studies, 31 Fitzwilliam Place, 2 Dublin, Ireland;
5.Max-Planck-Institut for Nuclear Physics, P.O. Box 103980, 69029 Heidelberg, Germany;
6.School of Physical Science and Technology and School of Information Science and Technology, Southwest Jiaotong University, 610031 Chengdu, Sichuan, China;
7.School of Astronomy and Space Science, Nanjing University, 210023 Nanjing, Jiangsu, China;
8.Center for Astrophysics, Guangzhou University, 510006 Guangzhou, Guangdong, China;
9.Tsung-Dao Lee Institute and School of Physics and Astronomy, Shanghai Jiao Tong University, 200240 Shanghai, China;
10.Institute for Nuclear Research of Russian Academy of Sciences, 117312 Moscow, Russia;
11.Hebei Normal University, 050024 Shijiazhuang, Hebei, China;
12.University of Science and Technology of China, 230026 Hefei, Anhui, China;
13.State Key Laboratory of Particle Detection and Electronics, China;
14.Key Laboratory of Dark Matter and Space Astronomy and Key Laboratory of Radio Astronomy, Purple Mountain Observatory, Chinese Academy of Sciences, 210023 Nanjing, Jiangsu, China;
15.Research Center for Astronomical Computing, Zhejiang Laboratory, 311121 Hangzhou, Zhejiang, China;
16.Key Laboratory for Research in Galaxies and Cosmology, Shanghai Astronomical Observatory, Chinese Academy of Sciences, 200030 Shanghai, China;
17.School of Physics and Astronomy, Yunnan University, 650091 Kunming, Yunnan, China;
18.Key Laboratory of Cosmic Rays (Tibet University), Ministry of Education, 850000 Lhasa, Tibet, China;
19.Department of Physics, The Chinese University of Hong Kong, Shatin, New Territories, Hong Kong, China;
20.Key Laboratory of Radio Astronomy and Technology, National Astronomical Observatories, Chinese Academy of Sciences, 100101 Beijing, China;
21.School of Physics and Astronomy (Zhuhai) and School of Physics (Guangzhou) and Sino-French Institute of Nuclear Engineering and Technology (Zhuhai), Sun Yat-sen University, 519000 Zhuhai 510275 Guangzhou, Guangdong, China;
22.Institute of Frontier and Interdisciplinary Science,;
23.APC, Université Paris Cité, CNRS/IN2P3, CEA/IRFU, Observatoire de Paris, 119 75205 Paris, France;
24.School of Physics and Astronomy (Zhuhai) and School of Physics (Guangzhou) and Sino-French Institute of Nuclear Engineering and Technology (Zhuhai), Sun Yat-sen University, 519000 Zhuhai and 510275 Guangzhou, Guangdong, China;
25.Department of Engineering Physics and Department of Astronomy, Tsinghua University, 100084 Beijing, China;
26.School of Physics and Microelectronics, Zhengzhou University, 450001 Zhengzhou, Henan, China;
27.Yunnan Observatories, Chinese Academy of Sciences, 650216 Kunming, Yunnan, China;
28.China Center of Advanced Science and Technology, Beijing 100190, China;
29.College of Physics, Sichuan University, 610065 Chengdu, Sichuan, China;
30.School of Physics, Peking University, 100871 Beijing, China;
31.Guangxi Key Laboratory for Relativistic Astrophysics, School of Physical Science and Technology, Guangxi University, 530004 Nanning, Guangxi, China;
32.Department of Physics, Faculty of Science, Mahidol University, Bangkok 10400, Thailand;
33.Moscow Institute of Physics and Technology, 141700 Moscow, Russia;
34.Center for Relativistic Astrophysics and High Energy Physics, School of Physics and Materials Science and Institute of Space Science and Technology, Nanchang University, 330031 Nanchang, Jiangxi, China;
35.National Space Science Center, Chinese Academy of Sciences, 100190 Beijing, China;
36.School of Physics, Huazhong University of Science and Technology, Wuhan 430074, Hubei, China
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GB/T 7714		 Cao, Zhen,Aharonian, F.,Axikegu,et al. Measurement of attenuation length of the muon content in extensive air showers from 0.3 to 30 PeV with LHAASO[J]. PHYSICAL REVIEW D,2024,110(10).
APA Cao, Zhen.,Aharonian, F..,Axikegu.,Bai, Y. X..,Bao, Y. W..,...&Zuo, X..(2024).Measurement of attenuation length of the muon content in extensive air showers from 0.3 to 30 PeV with LHAASO.PHYSICAL REVIEW D,110(10).
MLA Cao, Zhen,et al."Measurement of attenuation length of the muon content in extensive air showers from 0.3 to 30 PeV with LHAASO".PHYSICAL REVIEW D 110.10(2024).
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