Your browser doesn't support javascript.
loading
Measurements of All-Particle Energy Spectrum and Mean Logarithmic Mass of Cosmic Rays from 0.3 to 30 PeV with LHAASO-KM2A.
Cao, Zhen; Aharonian, F; Bai, Y X; Bao, Y W; Bastieri, D; Bi, X J; Bi, Y J; Bian, W; Bukevich, A V; Cao, Q; Cao, W Y; Cao, Zhe; Chang, J; Chang, J F; Chen, A M; Chen, E S; Chen, H X; Chen, Liang; Chen, Lin; Chen, Long; Chen, M J; Chen, M L; Chen, Q H; Chen, S; 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; Dong, X Q; Duan, K K; Fan, J H; Fan, Y Z; Fang, J; Fang, J H; Fang, K; Feng, C F; Feng, H; Feng, L; Feng, S H; Feng, X T; Feng, Y.
Afiliação
  • Cao Z; Key Laboratory of Particle Astrophysics and Experimental Physics Division and Computing Center, Institute of High Energy Physics, Chinese Academy of Sciences, 100049 Beijing, China.
  • Aharonian F; University of Chinese Academy of Sciences, 100049 Beijing, China.
  • Axikegu; Tianfu Cosmic Ray Research Center, 610000 Chengdu, Sichuan, China.
  • Bai YX; Dublin Institute for Advanced Studies, 31 Fitzwilliam Place, 2 Dublin, Ireland.
  • Bao YW; Max-Planck-Institut for Nuclear Physics, P.O. Box 103980, 69029 Heidelberg, Germany.
  • Bastieri D; School of Physical Science and Technology and School of Information Science and Technology, Southwest Jiaotong University, 610031 Chengdu, Sichuan, China.
  • Bi XJ; Key Laboratory of Particle Astrophysics and Experimental Physics Division and Computing Center, Institute of High Energy Physics, Chinese Academy of Sciences, 100049 Beijing, China.
  • Bi YJ; Tianfu Cosmic Ray Research Center, 610000 Chengdu, Sichuan, China.
  • Bian W; School of Astronomy and Space Science, Nanjing University, 210023 Nanjing, Jiangsu, China.
  • Bukevich AV; Center for Astrophysics, Guangzhou University, 510006 Guangzhou, Guangdong, China.
  • Cao Q; Key Laboratory of Particle Astrophysics and Experimental Physics Division and Computing Center, Institute of High Energy Physics, Chinese Academy of Sciences, 100049 Beijing, China.
  • Cao WY; University of Chinese Academy of Sciences, 100049 Beijing, China.
  • Cao Z; Tianfu Cosmic Ray Research Center, 610000 Chengdu, Sichuan, China.
  • Chang J; Key Laboratory of Particle Astrophysics and Experimental Physics Division and Computing Center, Institute of High Energy Physics, Chinese Academy of Sciences, 100049 Beijing, China.
  • Chang JF; Tianfu Cosmic Ray Research Center, 610000 Chengdu, Sichuan, China.
  • Chen AM; Tsung-Dao Lee Institute and School of Physics and Astronomy, Shanghai Jiao Tong University, 200240 Shanghai, China.
  • Chen ES; Institute for Nuclear Research of Russian Academy of Sciences, 117312 Moscow, Russia.
  • Chen HX; Hebei Normal University, 050024 Shijiazhuang, Hebei, China.
  • Chen L; University of Science and Technology of China, 230026 Hefei, Anhui, China.
  • Chen L; University of Science and Technology of China, 230026 Hefei, Anhui, China.
  • Chen L; State Key Laboratory of Particle Detection and Electronics, China.
  • Chen MJ; 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.
  • Chen ML; Key Laboratory of Particle Astrophysics and Experimental Physics Division and Computing Center, Institute of High Energy Physics, Chinese Academy of Sciences, 100049 Beijing, China.
  • Chen QH; Tianfu Cosmic Ray Research Center, 610000 Chengdu, Sichuan, China.
  • Chen S; State Key Laboratory of Particle Detection and Electronics, China.
  • Chen SH; Tsung-Dao Lee Institute and School of Physics and Astronomy, Shanghai Jiao Tong University, 200240 Shanghai, China.
  • Chen SZ; Key Laboratory of Particle Astrophysics and Experimental Physics Division and Computing Center, Institute of High Energy Physics, Chinese Academy of Sciences, 100049 Beijing, China.
  • Chen TL; University of Chinese Academy of Sciences, 100049 Beijing, China.
  • Chen Y; Tianfu Cosmic Ray Research Center, 610000 Chengdu, Sichuan, China.
  • Cheng N; Research Center for Astronomical Computing, Zhejiang Laboratory, 311121 Hangzhou, Zhejiang, China.
  • Cheng YD; Key Laboratory for Research in Galaxies and Cosmology, Shanghai Astronomical Observatory, Chinese Academy of Sciences, 200030 Shanghai, China.
  • Cui MY; School of Physical Science and Technology and School of Information Science and Technology, Southwest Jiaotong University, 610031 Chengdu, Sichuan, China.
  • Cui SW; School of Physical Science and Technology and School of Information Science and Technology, Southwest Jiaotong University, 610031 Chengdu, Sichuan, China.
  • Cui XH; Key Laboratory of Particle Astrophysics and Experimental Physics Division and Computing Center, Institute of High Energy Physics, Chinese Academy of Sciences, 100049 Beijing, China.
  • Cui YD; Tianfu Cosmic Ray Research Center, 610000 Chengdu, Sichuan, China.
  • Dai BZ; Key Laboratory of Particle Astrophysics and Experimental Physics Division and Computing Center, Institute of High Energy Physics, Chinese Academy of Sciences, 100049 Beijing, China.
  • Dai HL; Tianfu Cosmic Ray Research Center, 610000 Chengdu, Sichuan, China.
  • Dai ZG; State Key Laboratory of Particle Detection and Electronics, China.
  • Danzengluobu; School of Physical Science and Technology and School of Information Science and Technology, Southwest Jiaotong University, 610031 Chengdu, Sichuan, China.
  • Dong XQ; School of Physics and Astronomy, Yunnan University, 650091 Kunming, Yunnan, China.
  • Duan KK; Key Laboratory of Particle Astrophysics and Experimental Physics Division and Computing Center, Institute of High Energy Physics, Chinese Academy of Sciences, 100049 Beijing, China.
  • Fan JH; University of Chinese Academy of Sciences, 100049 Beijing, China.
  • Fan YZ; Tianfu Cosmic Ray Research Center, 610000 Chengdu, Sichuan, China.
  • Fang J; Key Laboratory of Particle Astrophysics and Experimental Physics Division and Computing Center, Institute of High Energy Physics, Chinese Academy of Sciences, 100049 Beijing, China.
  • Fang JH; Tianfu Cosmic Ray Research Center, 610000 Chengdu, Sichuan, China.
  • Fang K; Key Laboratory of Cosmic Rays (Tibet University), Ministry of Education, 850000 Lhasa, Tibet, China.
  • Feng CF; School of Astronomy and Space Science, Nanjing University, 210023 Nanjing, Jiangsu, China.
  • Feng H; Key Laboratory of Particle Astrophysics and Experimental Physics Division and Computing Center, Institute of High Energy Physics, Chinese Academy of Sciences, 100049 Beijing, China.
  • Feng L; Tianfu Cosmic Ray Research Center, 610000 Chengdu, Sichuan, China.
  • Feng SH; Key Laboratory of Particle Astrophysics and Experimental Physics Division and Computing Center, Institute of High Energy Physics, Chinese Academy of Sciences, 100049 Beijing, China.
Phys Rev Lett ; 132(13): 131002, 2024 Mar 29.
Article em En | MEDLINE | ID: mdl-38613275
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±0.05±0.15 PeV. Below the knee, the spectral index is found to be -2.7413±0.0004±0.0050, while above the knee, it is -3.128±0.005±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±0.0003±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.

Texto completo: 1 Coleções: 01-internacional Base de dados: MEDLINE Idioma: En Ano de publicação: 2024 Tipo de documento: Article

Texto completo: 1 Coleções: 01-internacional Base de dados: MEDLINE Idioma: En Ano de publicação: 2024 Tipo de documento: Article