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Stringent Tests of Lorentz Invariance Violation from LHAASO Observations of GRB 221009A
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; 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; Cui, M. Y.14; Cui, S. W.11; Cui, X. H.19; Cui, Y. D.20; 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.21; Feng, H.1; Feng, L.14; Feng, S. H.1,3; Feng, X. T.21; Feng, Y.15; Feng, Y. L.18; Gabici, S.22; Gao, B.1,3; Gao, C. D.21; Gao, Q.18; Gao, W.1,3; Gao, W. K.1,2,3; Ge, M. M.17; Geng, L. S.1,3; Giacinti, G.9; Gong, G. H.23; Gou, Q. B.1,3; Gu, M. H.1,3,13; Guo, F. L.16; Guo, X. L.6; Guo, Y. Q.1,3; Guo, Y. Y.14; Han, Y. A.24; 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.20; Hou, B. W.1,2,3; Hou, C.1,3; Hou X(侯贤)25; Hu, H. B.1,2,3; Hu, Q.12,14; Hu, S. C.1,3,26; Huang, D. H.6; Huang, T. Q.1,3; Huang, W. J.20; Huang, X. T.21; Huang, X. Y.14; Huang, Y.1,2,3; Ji, X. L.1,3,13; Jia, H. Y.6; Jia, K.21; Jiang, K.12,13; Jiang, X. W.1,3; Jiang, Z. J.17; Jin, M.6; Kang, M. M.27; Karpikov, I.10; 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.21; Li, W. L.9; Li, X. R.1,3; Li, Xin12,13; Li, Y. Z.1,2,3; Li, Zhe1,3; Li, Zhuo28; Liang, E. W.29; Liang, Y. F.29; Lin, S. J.20,35; Liu, B.12; Liu, C.1,3; Liu, D.21; Liu, D. B.9; Liu, H.6; Liu, H. D.24; 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.23; Luo, Q.20,35; Luo, Y.9; Lv, H. K.1,3; Ma, B. Q.28; Ma, L. L.1,3; Ma, X. H.1,3; Mao JR(毛基荣)25; Min, Z.1,3; Mitthumsiri, W.30; Mu, H. J.24; Nan, Y. C.1,3; Neronov, A.22; Ou, L. J.8; Pattarakijwanich, P.30; 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.30; Sáiz, A.30; Saeed, M.1,2,3; Semikoz, D.22; Shao, L.11; Shchegolev, O.10,31; Sheng, X. D.1,3; Shu, F. W.32; Song, H. C.28; Stenkin, Yu. V.10,31; Stepanov, V.10; Su, Y.14; Sun, D. X.12,14; Sun, Q. N.6; Sun, X. N.29; Sun, Z. B.33; Takata, J.34; Tam, P. H.20
发表期刊Physical Review Letters
2024-08-16
卷号133期号:7
DOI10.1103/PhysRevLett.133.071501
产权排序第25完成单位
收录类别SCI ; EI
摘要On 9 October 2022, the Large High Altitude Air Shower Observatory (LHAASO) reported the observation of the very early TeV afterglow of the brightest-of-all-time gamma-ray burst 221009A, recording the highest photon statistics in the TeV band ever obtained from a gamma-ray burst. We use this unique observation to place stringent constraints on the energy dependence of the speed of light in vacuum, a manifestation of Lorentz invariance violation (LIV) predicted by some quantum gravity (QG) theories. Our results show that the 95% confidence level lower limits on the QG energy scales are EQG,1>10 times the Planck energy EPl for the linear LIV effect, and EQG,2>6×10-8EPl for the quadratic LIV effect. Our limits on the quadratic LIV case improve previous best bounds by factors of 5-7. © 2024 American Physical Society.
资助项目N/A
项目资助者N/A
语种英语
学科领域物理学 ; 高能天体物理学 ; 天文学 ; 星系与宇宙学 ; 天文学 ; 天体物理学 ; 高能天体物理学
文章类型Journal article (JA)
ISSN0031-9007
URL查看原文
EI入藏号20243416924506
EI分类号1301.1.3
引用统计
文献类型期刊论文
条目标识符http://ir.ynao.ac.cn/handle/114a53/27562
专题星系类星体研究组
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, Beijing, 100049, China;
2.University of Chinese Academy of Sciences, Beijing, 100049, China;
3.Tianfu Cosmic Ray Research Center, Sichuan, Chengdu, 610000, China;
4.Dublin Institute for Advanced Studies, 31 Fitzwilliam Place, Dublin, 02, Ireland;
5.Max-Planck-Institut for Nuclear Physics, P.O. Box 103980, Heidelberg, 69029, Germany;
6.School of Physical Science and Technology, School of Information Science and Technology, Southwest Jiaotong University, Sichuan, Chengdu, 610031, China;
7.School of Astronomy and Space Science, Nanjing University, Jiangsu, Nanjing, 210023, China;
8.Center for Astrophysics, Guangzhou University, Guangdong, Guangzhou, 510006, China;
9.Tsung-Dao Lee Institute, School of Physics and Astronomy, Shanghai Jiao Tong University, Shanghai, 200240, China;
10.Institute for Nuclear Research of Russian Academy of Sciences, Moscow, 117312, Russia;
11.Hebei Normal University, Hebei, Shijiazhuang, 050024, China;
12.University of Science and Technology of China, Anhui, Hefei, 230026, China;
13.State Key Laboratory of Particle Detection and Electronics, China;
14.Key Laboratory of Dark Matter and Space Astronomy, Key Laboratory of Radio Astronomy, Purple Mountain Observatory, Chinese Academy of Sciences, Jiangsu, Nanjing, 210023, China;
15.Research Center for Astronomical Computing, Zhejiang Laboratory, Zhejiang, Hangzhou, 311121, China;
16.Key Laboratory for Research in Galaxies and Cosmology, Shanghai Astronomical Observatory, Chinese Academy of Sciences, Shanghai, 200030, China;
17.School of Physics and Astronomy, Yunnan University, Yunnan, Kunming, 650091, China;
18.Key Laboratory of Cosmic Rays (Tibet University), Ministry of Education, Tibet, Lhasa, 850000, China;
19.National Astronomical Observatories, Chinese Academy of Sciences, Beijing, 100101, China;
20.School of Physics and Astronomy (Zhuhai), School of Physics (Guangzhou), Sino-French Institute of Nuclear Engineering and Technology (Zhuhai), Sun Yat-sen University, Zhuhai, 519000, China;
21.Institute of Frontier and Interdisciplinary Science, Shandong University, Shandong, Qingdao, 266237, China;
22.APC, Université Paris Cité, CNRS/IN2P3, CEA/IRFU, Observatoire de Paris, 119, Paris, 75205, France;
23.Department of Engineering Physics, Tsinghua University, Beijing, 100084, China;
24.School of Physics and Microelectronics, Zhengzhou University, Henan, Zhengzhou, 450001, China;
25.Yunnan Observatories, Chinese Academy of Sciences, Yunnan, Kunming, 650216, China;
26.China Center of Advanced Science and Technology, Beijing, 100190, China;
27.College of Physics, Sichuan University, Sichuan, Chengdu, 610065, China;
28.School of Physics, Peking University, Beijing, 100871, China;
29.Guangxi Key Laboratory for Relativistic Astrophysics, School of Physical Science and Technology, Guangxi University, Guangxi, Nanning, 530004, China;
30.Department of Physics, Faculty of Science, Mahidol University, Bangkok, 10400, Thailand;
31.Moscow Institute of Physics and Technology, Moscow, 141700, Russia;
32.Center for Relativistic Astrophysics and High Energy Physics, School of Physics and Materials Science, Institute of Space Science and Technology, Nanchang University, Jiangxi, Nanchang, 330031, China;
33.National Space Science Center, Chinese Academy of Sciences, Beijing, 100190, China;
34.School of Physics, Huazhong University of Science and Technology, Hubei, Wuhan, 430074, China;
35.School of Physics and Astronomy (Zhuhai), School of Physics (Guangzhou), Sino-French Institute of Nuclear Engineering and Technology (Zhuhai), Sun Yat-sen University, Guangdong, Guangzhou, 510275, China
推荐引用方式
GB/T 7714
Cao, Zhen,Aharonian, F.,Axikegu,et al. Stringent Tests of Lorentz Invariance Violation from LHAASO Observations of GRB 221009A[J]. Physical Review Letters,2024,133(7).
APA Cao, Zhen.,Aharonian, F..,Axikegu.,Bai, Y. X..,Bao, Y. W..,...&Tam, P. H..(2024).Stringent Tests of Lorentz Invariance Violation from LHAASO Observations of GRB 221009A.Physical Review Letters,133(7).
MLA Cao, Zhen,et al."Stringent Tests of Lorentz Invariance Violation from LHAASO Observations of GRB 221009A".Physical Review Letters 133.7(2024).
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