Stringent Tests of Lorentz Invariance Violation from LHAASO Observations of GRB 221009A
Affiliations
- 1 Key Laboratory of Particle Astrophysics and Experimental Physics Division and Computing Center, Institute of High Energy Physics, Chinese Academy of Sciences, 100049 Beijing, China.
- 2 University of Chinese Academy of Sciences, 100049 Beijing, China.
- 3 Tianfu Cosmic Ray Research Center, 610000 Chengdu, Sichuan, China.
- 4 Dublin Institute for Advanced Studies, 31 Fitzwilliam Place, 2 Dublin, Ireland.
- 5 Max-Planck-Institut for Nuclear Physics, P.O. Box 103980, 69029 Heidelberg, Germany.
- 6 School of Physical Science and Technology and School of Information Science and Technology, Southwest Jiaotong University, 610031 Chengdu, Sichuan, China.
- 7 School of Astronomy and Space Science, Nanjing University, 210023 Nanjing, Jiangsu, China.
- 8 Center for Astrophysics, Guangzhou University, 510006 Guangzhou, Guangdong, China.
- 9 Tsung-Dao Lee Institute and School of Physics and Astronomy, Shanghai Jiao Tong University, 200240 Shanghai, China.
- 10 Institute for Nuclear Research of Russian Academy of Sciences, 117312 Moscow, Russia.
- 11 Hebei Normal University, 050024 Shijiazhuang, Hebei, China.
- 12 University of Science and Technology of China, 230026 Hefei, Anhui, China.
- 13 State Key Laboratory of Particle Detection and Electronics, China.
- 14 Key Laboratory of Dark Matter and Space Astronomy and Key Laboratory of Radio Astronomy, <a href="https://ror.org/02eb4t121">Purple Mountain Observatory</a>, Chinese Academy of Sciences, 210023 Nanjing, Jiangsu, China.
- 15 Research Center for Astronomical Computing, Zhejiang Laboratory, 311121 Hangzhou, Zhejiang, China.
- 16 Key Laboratory for Research in Galaxies and Cosmology, Shanghai Astronomical Observatory, Chinese Academy of Sciences, 200030 Shanghai, China.
- 17 School of Physics and Astronomy, Yunnan University, 650091 Kunming, Yunnan, China.
- 18 Key Laboratory of Cosmic Rays (Tibet University), Ministry of Education, 850000 Lhasa, Tibet, China.
- 19 National Astronomical Observatories, Chinese Academy of Sciences, 100101 Beijing, China.
- 20 School of Physics and Astronomy (Zhuhai) and School of Physics (Guangzhou) and Sino-French Institute of Nuclear Engineering and Technology (Zhuhai), Sun Yat-sen University, 519000 Zhuhai and 510275 Guangzhou, Guangdong, China.
- 21 Institute of Frontier and Interdisciplinary Science, Shandong University, 266237 Qingdao, Shandong, China.
- 22 APC, Université Paris Cité, CNRS/IN2P3, CEA/IRFU, Observatoire de Paris, 119 75205 Paris, France.
- 23 Department of Engineering Physics, Tsinghua University, 100084 Beijing, China.
- 24 School of Physics and Microelectronics, Zhengzhou University, 450001 Zhengzhou, Henan, China.
- 25 Yunnan Observatories, Chinese Academy of Sciences, 650216 Kunming, Yunnan, China.
- 26 China Center of Advanced Science and Technology, Beijing 100190, China.
- 27 College of Physics, Sichuan University, 610065 Chengdu, Sichuan, China.
- 28 School of Physics, Peking University, 100871 Beijing, China.
- 29 Guangxi Key Laboratory for Relativistic Astrophysics, School of Physical Science and Technology, Guangxi University, 530004 Nanning, Guangxi, China.
- 30 Department of Physics, Faculty of Science, Mahidol University, Bangkok 10400, Thailand.
- 31 Moscow Institute of Physics and Technology, 141700 Moscow, Russia.
- 32 Center for Relativistic Astrophysics and High Energy Physics, School of Physics and Materials Science and Institute of Space Science and Technology, Nanchang University, 330031 Nanchang, Jiangxi, China.
- 33 National Space Science Center, Chinese Academy of Sciences, 100190 Beijing, China.
- 34 School of Physics, Huazhong University of Science and Technology, Wuhan 430074, Hubei, China.
- PMID: 39213544
- DOI: 10.1103/PhysRevLett.133.071501
Stringent Tests of Lorentz Invariance Violation from LHAASO Observations of GRB 221009A
Authors
Affiliations
- 1 Key Laboratory of Particle Astrophysics and Experimental Physics Division and Computing Center, Institute of High Energy Physics, Chinese Academy of Sciences, 100049 Beijing, China.
- 2 University of Chinese Academy of Sciences, 100049 Beijing, China.
- 3 Tianfu Cosmic Ray Research Center, 610000 Chengdu, Sichuan, China.
- 4 Dublin Institute for Advanced Studies, 31 Fitzwilliam Place, 2 Dublin, Ireland.
- 5 Max-Planck-Institut for Nuclear Physics, P.O. Box 103980, 69029 Heidelberg, Germany.
- 6 School of Physical Science and Technology and School of Information Science and Technology, Southwest Jiaotong University, 610031 Chengdu, Sichuan, China.
- 7 School of Astronomy and Space Science, Nanjing University, 210023 Nanjing, Jiangsu, China.
- 8 Center for Astrophysics, Guangzhou University, 510006 Guangzhou, Guangdong, China.
- 9 Tsung-Dao Lee Institute and School of Physics and Astronomy, Shanghai Jiao Tong University, 200240 Shanghai, China.
- 10 Institute for Nuclear Research of Russian Academy of Sciences, 117312 Moscow, Russia.
- 11 Hebei Normal University, 050024 Shijiazhuang, Hebei, China.
- 12 University of Science and Technology of China, 230026 Hefei, Anhui, China.
- 13 State Key Laboratory of Particle Detection and Electronics, China.
- 14 Key Laboratory of Dark Matter and Space Astronomy and Key Laboratory of Radio Astronomy, <a href="https://ror.org/02eb4t121">Purple Mountain Observatory</a>, Chinese Academy of Sciences, 210023 Nanjing, Jiangsu, China.
- 15 Research Center for Astronomical Computing, Zhejiang Laboratory, 311121 Hangzhou, Zhejiang, China.
- 16 Key Laboratory for Research in Galaxies and Cosmology, Shanghai Astronomical Observatory, Chinese Academy of Sciences, 200030 Shanghai, China.
- 17 School of Physics and Astronomy, Yunnan University, 650091 Kunming, Yunnan, China.
- 18 Key Laboratory of Cosmic Rays (Tibet University), Ministry of Education, 850000 Lhasa, Tibet, China.
- 19 National Astronomical Observatories, Chinese Academy of Sciences, 100101 Beijing, China.
- 20 School of Physics and Astronomy (Zhuhai) and School of Physics (Guangzhou) and Sino-French Institute of Nuclear Engineering and Technology (Zhuhai), Sun Yat-sen University, 519000 Zhuhai and 510275 Guangzhou, Guangdong, China.
- 21 Institute of Frontier and Interdisciplinary Science, Shandong University, 266237 Qingdao, Shandong, China.
- 22 APC, Université Paris Cité, CNRS/IN2P3, CEA/IRFU, Observatoire de Paris, 119 75205 Paris, France.
- 23 Department of Engineering Physics, Tsinghua University, 100084 Beijing, China.
- 24 School of Physics and Microelectronics, Zhengzhou University, 450001 Zhengzhou, Henan, China.
- 25 Yunnan Observatories, Chinese Academy of Sciences, 650216 Kunming, Yunnan, China.
- 26 China Center of Advanced Science and Technology, Beijing 100190, China.
- 27 College of Physics, Sichuan University, 610065 Chengdu, Sichuan, China.
- 28 School of Physics, Peking University, 100871 Beijing, China.
- 29 Guangxi Key Laboratory for Relativistic Astrophysics, School of Physical Science and Technology, Guangxi University, 530004 Nanning, Guangxi, China.
- 30 Department of Physics, Faculty of Science, Mahidol University, Bangkok 10400, Thailand.
- 31 Moscow Institute of Physics and Technology, 141700 Moscow, Russia.
- 32 Center for Relativistic Astrophysics and High Energy Physics, School of Physics and Materials Science and Institute of Space Science and Technology, Nanchang University, 330031 Nanchang, Jiangxi, China.
- 33 National Space Science Center, Chinese Academy of Sciences, 100190 Beijing, China.
- 34 School of Physics, Huazhong University of Science and Technology, Wuhan 430074, Hubei, China.
- PMID: 39213544
- DOI: 10.1103/PhysRevLett.133.071501
Abstract
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 E_{QG,1}>10 times the Planck energy E_{Pl} for the linear LIV effect, and E_{QG,2}>6×10^{-8}E_{Pl} for the quadratic LIV effect. Our limits on the quadratic LIV case improve previous best bounds by factors of 5-7.
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