Institutional Repository System Of Yunnan Observatories, CAS
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 |
DOI | 10.1103/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) |
ISSN | 0031-9007 |
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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