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Measurements of All-Particle Energy Spectrum and Mean Logarithmic Mass of Cosmic Rays from 0.3 to 30 PeV with LHAASO-KM2A

Authors :
The LHAASO Collaboration
Cao, Zhen
Aharonian, F.
An, Q.
Axikegu, A.
Bai, Y. X.
Bao, Y. W.
Bastieri, D.
Bi, X. J.
Bi, Y. J.
Cai, J. T.
Cao, Q.
Cao, W. Y.
Cao, Zhe
Chang, J.
Chang, J. F.
Chen, A. M.
Chen, E. S.
Chen, Liang
Chen, Lin
Chen, Long
Chen, M. J.
Chen, M. L.
Chen, Q. H.
Chen, S. H.
Chen, S. Z.
Chen, T. L.
Chen, Y.
Cheng, N.
Cheng, Y. D.
Cui, M. Y.
Cui, S. W.
Cui, X. H.
Cui, Y. D.
Dai, B. Z.
Dai, H. L.
Dai, Z. G.
Danzengluobu
della Volpe, D.
Dong, X. Q.
Duan, K. K.
Fan, J. H.
Fan, Y. Z.
Fang, J.
Fang, K.
Feng, C. F.
Feng, L.
Feng, S. H.
Feng, X. T.
Feng, Y. L.
Gabici, S.
Gao, B.
Gao, C. D.
Gao, L. Q.
Gao, Q.
Gao, W.
Gao, W. K.
Ge, M. M.
Geng, L. S.
Giacinti, G.
Gong, G. H.
Gou, Q. B.
Gu, M. H.
Guo, F. L.
Guo, X. L.
Guo, Y. Q.
Guo, Y. Y.
Han, Y. A.
He, H. H.
He, H. N.
He, J. Y.
He, X. B.
He, Y.
Heller, M.
Hor, Y. K.
Hou, B. W.
Hou, C.
Hou, X.
Hu, H. B.
Hu, Q.
Hu, S. C.
Huang, D. H.
Huang, T. Q.
Huang, W. J.
Huang, X. T.
Huang, X. Y.
Huang, Y.
Huang, Z. C.
Ji, X. L.
Jia, H. Y.
Jia, K.
Jiang, K.
Jiang, X. W.
Jiang, Z. J.
Jin, M.
Kang, M. M.
Ke, T.
Kuleshov, D.
Kurinov, K.
Li, B. B.
Li, Cheng
Li, Cong
Li, D.
Li, F.
Li, H. B.
Li, H. C.
Li, H. Y.
Li, J.
Li, Jian
Li, Jie
Li, K.
Li, W. L.
Li, X. R.
Li, Xin
Li, Y. Z.
Li, Zhe
Li, Zhuo
Liang, E. W.
Liang, Y. F.
Lin, S. J.
Liu, B.
Liu, C.
Liu, D.
Liu, H.
Liu, H. D.
Liu, J.
Liu, J. L.
Liu, J. Y.
Liu, M. Y.
Liu, R. Y.
Liu, S. M.
Liu, W.
Liu, Y.
Liu, Y. N.
Lu, R.
Luo, Q.
Lv, H. K.
Ma, B. Q.
Ma, L. L.
Ma, X. H.
Mao, J. R.
Min, Z.
Mitthumsiri, W.
Mu, H. J.
Nan, Y. C.
Neronov, A.
Ou, Z. W.
Pang, B. Y.
Pattarakijwanich, P.
Pei, Z. Y.
Qi, M. Y.
Qi, Y. Q.
Qiao, B. Q.
Qin, J. J.
Ruffolo, D.
Sáiz, A.
Semikoz, D.
Shao, C. Y.
Shao, L.
Shchegolev, O.
Sheng, X. D.
Shu, F. W.
Song, H. C.
Stenkin, Yu. V.
Stepanov, V.
Su, Y.
Sun, Q. N.
Sun, X. N.
Sun, Z. B.
Tam, P. H. T.
Tang, Q. W.
Tang, Z. B.
Tian, W. W.
Wang, C.
Wang, C. B.
Wang, G. W.
Wang, H. G.
Wang, H. H.
Wang, J. C.
Wang, K.
Wang, L. P.
Wang, L. Y.
Wang, P. H.
Wang, R.
Wang, W.
Wang, X. G.
Wang, X. Y.
Wang, Y.
Wang, Y. D.
Wang, Y. J.
Wang, Z. H.
Wang, Z. X.
Wang, Zhen
Wang, Zheng
Wei, D. M.
Wei, J. J.
Wei, Y. J.
Wen, T.
Wu, C. Y.
Wu, H. R.
Wu, S.
Wu, X. F.
Wu, Y. S.
Xi, S. Q.
Xia, J.
Xia, J. J.
Xiang, G. M.
Xiao, D. X.
Xiao, G.
Xin, G. G.
Xin, Y. L.
Xing, Y.
Xiong, Z.
Xu, D. L.
Xu, R. F.
Xu, R. X.
Xu, W. L.
Xue, L.
Yan, D. H.
Yan, J. Z.
Yan, T.
Yang, C. W.
Yang, F.
Yang, F. F.
Yang, H. W.
Yang, J. Y.
Yang, L. L.
Yang, M. J.
Yang, R. Z.
Yang, S. B.
Yao, Y. H.
Yao, Z. G.
Ye, Y. M.
Yin, L. Q.
Yin, N.
You, X. H.
You, Z. Y.
Yu, Y. H.
Yuan, Q.
Yue, H.
Zeng, H. D.
Zeng, T. X.
Zeng, W.
Zha, M.
Zhang, B. B.
Zhang, F.
Zhang, H. M.
Zhang, H. Y.
Zhang, J. L.
Zhang, L. X.
Zhang, Li
Zhang, P. F.
Zhang, P. P.
Zhang, R.
Zhang, S. B.
Zhang, S. R.
Zhang, S. S.
Zhang, X.
Zhang, X. P.
Zhang, Y. F.
Zhang, Yi
Zhang, Yong
Zhao, B.
Zhao, J.
Zhao, L.
Zhao, L. Z.
Zhao, S. P.
Zheng, F.
Zhou, B.
Zhou, H.
Zhou, J. N.
Zhou, M.
Zhou, P.
Zhou, R.
Zhou, X. X.
Zhu, C. G.
Zhu, F. R.
Zhu, H.
Zhu, K. J.
Zuo, X.
Source :
Physical Review Letters 132, 131002 (2024)
Publication Year :
2024

Abstract

We present the measurements of all-particle energy spectrum and mean logarithmic mass of cosmic rays in the energy range of 0.3-30 PeV using data collected from LHAASO-KM2A between September 2021 and December 2022, which is based on a nearly composition-independent energy reconstruction method, achieving unprecedented accuracy. Our analysis reveals the position of the knee at $3.67 \pm 0.05 \pm 0.15$ PeV. Below the knee, the spectral index is found to be -$2.7413 \pm 0.0004 \pm 0.0050$, while above the knee, it is -$3.128 \pm 0.005 \pm 0.027$, with the sharpness of the transition measured with a statistical error of 2%. The mean logarithmic mass of cosmic rays is almost heavier than helium in the whole measured energy range. It decreases from 1.7 at 0.3 PeV to 1.3 at 3 PeV, representing a 24% decline following a power law with an index of -$0.1200 \pm 0.0003 \pm 0.0341$. This is equivalent to an increase in abundance of light components. Above the knee, the mean logarithmic mass exhibits a power law trend towards heavier components, which is reversal to the behavior observed in the all-particle energy spectrum. Additionally, the knee position and the change in power-law index are approximately the same. These findings suggest that the knee observed in the all-particle spectrum corresponds to the knee of the light component, rather than the medium-heavy components.<br />Comment: 8 pages, 3 figures

Details

Database :
arXiv
Journal :
Physical Review Letters 132, 131002 (2024)
Publication Type :
Report
Accession number :
edsarx.2403.10010
Document Type :
Working Paper
Full Text :
https://doi.org/10.1103/PhysRevLett.132.131002