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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 :
Cao Z
Aharonian F
Axikegu
Bai YX
Bao YW
Bastieri D
Bi XJ
Bi YJ
Bian W
Bukevich AV
Cao Q
Cao WY
Cao Z
Chang J
Chang JF
Chen AM
Chen ES
Chen HX
Chen L
Chen L
Chen L
Chen MJ
Chen ML
Chen QH
Chen S
Chen SH
Chen SZ
Chen TL
Chen Y
Cheng N
Cheng YD
Cui MY
Cui SW
Cui XH
Cui YD
Dai BZ
Dai HL
Dai ZG
Danzengluobu
Dong XQ
Duan KK
Fan JH
Fan YZ
Fang J
Fang JH
Fang K
Feng CF
Feng H
Feng L
Feng SH
Feng XT
Feng Y
Feng YL
Gabici S
Gao B
Gao CD
Gao Q
Gao W
Gao WK
Ge MM
Geng LS
Giacinti G
Gong GH
Gou QB
Gu MH
Guo FL
Guo XL
Guo YQ
Guo YY
Han YA
Hasan M
He HH
He HN
He JY
He Y
Hor YK
Hou BW
Hou C
Hou X
Hu HB
Hu Q
Hu SC
Huang DH
Huang TQ
Huang WJ
Huang XT
Huang XY
Huang Y
Ji XL
Jia HY
Jia K
Jiang K
Jiang XW
Jiang ZJ
Jin M
Kang MM
Karpikov I
Kuleshov D
Kurinov K
Li BB
Li CM
Li C
Li C
Li D
Li F
Li HB
Li HC
Li J
Li J
Li K
Li SD
Li WL
Li WL
Li XR
Li X
Li YZ
Li Z
Li Z
Liang EW
Liang YF
Lin SJ
Liu B
Liu C
Liu D
Liu DB
Liu H
Liu HD
Liu J
Liu JL
Liu MY
Liu RY
Liu SM
Liu W
Liu Y
Liu YN
Luo Q
Luo Y
Lv HK
Ma BQ
Ma LL
Ma XH
Mao JR
Min Z
Mitthumsiri W
Mu HJ
Nan YC
Neronov A
Ou LJ
Pattarakijwanich P
Pei ZY
Qi JC
Qi MY
Qiao BQ
Qin JJ
Raza A
Ruffolo D
Sáiz A
Saeed M
Semikoz D
Shao L
Shchegolev O
Sheng XD
Shu FW
Song HC
Stenkin YV
Stepanov V
Su Y
Sun DX
Sun QN
Sun XN
Sun ZB
Takata J
Tam PHT
Tang QW
Tang R
Tang ZB
Tian WW
Wang C
Wang CB
Wang GW
Wang HG
Wang HH
Wang JC
Wang K
Wang K
Wang LP
Wang LY
Wang PH
Wang R
Wang W
Wang XG
Wang XY
Wang Y
Wang YD
Wang YJ
Wang ZH
Wang ZX
Wang Z
Wang Z
Wei DM
Wei JJ
Wei YJ
Wen T
Wu CY
Wu HR
Wu QW
Wu S
Wu XF
Wu YS
Xi SQ
Xia J
Xiang GM
Xiao DX
Xiao G
Xin YL
Xing Y
Xiong DR
Xiong Z
Xu DL
Xu RF
Xu RX
Xu WL
Xue L
Yan DH
Yan JZ
Yan T
Yang CW
Yang CY
Yang F
Yang FF
Yang LL
Yang MJ
Yang RZ
Yang WX
Yao YH
Yao ZG
Yin LQ
Yin N
You XH
You ZY
Yu YH
Yuan Q
Yue H
Zeng HD
Zeng TX
Zeng W
Zha M
Zhang BB
Zhang F
Zhang H
Zhang HM
Zhang HY
Zhang JL
Zhang L
Zhang PF
Zhang PP
Zhang R
Zhang SB
Zhang SR
Zhang SS
Zhang X
Zhang XP
Zhang YF
Zhang Y
Zhang Y
Zhao B
Zhao J
Zhao L
Zhao LZ
Zhao SP
Zhao XH
Zheng F
Zhong WJ
Zhou B
Zhou H
Zhou JN
Zhou M
Zhou P
Zhou R
Zhou XX
Zhou XX
Zhu BY
Zhu CG
Zhu FR
Zhu H
Zhu KJ
Zou YC
Zuo X
Source :
Physical review letters [Phys Rev Lett] 2024 Mar 29; Vol. 132 (13), pp. 131002.
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±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.

Details

Language :
English
ISSN :
1079-7114
Volume :
132
Issue :
13
Database :
MEDLINE
Journal :
Physical review letters
Publication Type :
Academic Journal
Accession number :
38613275
Full Text :
https://doi.org/10.1103/PhysRevLett.132.131002