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Exploring Lorentz Invariance Violation from Ultrahigh-Energy gamma
Cao, Zhen1,2,3; Aharonian, F.4,5; An, Q.6,7; Axikegu8; Bai, L. X.9; Bai, Y. X.1,3; Bao, Y. W.10; Bastieri, D.11; Bi, X. J.1,2,3; Bi, Y. J.1,3; Cai, H.12; Cai, J. T.11; Cao, Zhe6,7; Chang, J.13; Chang, J. F.1,3,6; Chen, B. M.14; Chen, E. S.1,2,3; Chen, J.9; Chen, Liang1,2,3; Chen, Liang15; Chen, Long8; Chen, M. J.1,3; Chen, M. L.1,3,6; Chen, Q. H.8; Chen, S. H.1,2,3; Chen, S. Z.1,3; Chen, T. L.16; Chen, X. L.1,2,3; Chen, Y.10; Cheng, N.1,3; Cheng, Y. D.1,3; Cui, S. W.14; Cui, X. H.17; Cui, Y. D.18; Piazzoli, B. D’Ettorre19; Dai, B. Z.20; Dai, H. L.1,3,6; Dai, Z. G.7; Danzengluobu16; Volpe, D. della21; Dong, X. J.1,3; Duan, K. K.13; Fan, J. H.11; Fan, Y. Z.13; Fan, Z. X.1,3; Fang, J.20; Fang, K.1,3; Feng, C. F.22; Feng, L.13; Feng, S. H.1,3; Feng, Y. L.13; Gao, B.1,3; Gao, C. D.22; Gao, L. Q.1,2,3; Gao, Q.16; Gao, W.22; Ge, M. M.20; Geng, L. S.1,3; Gong, G. H.23; Gou, Q. B.1,3; Gu, M. H.1,3,6; Guo, F. L.15; Guo, J. G.1,2,3; Guo, X. L.8; Guo, Y. Q.1,3; Guo, Y. Y.1,2,3,13; Han, Y. A.24; He, H. H.1,2,3; He, H. N.13; He, J. C.1,2,3; He, S. L.11; He, X. B.18; He, Y.8; Heller, M.21; Hor, Y. K.18; Hou, C.1,3; Hou X(侯贤)25; Hu, H. B.1,2,3; Hu, S.9; Hu, S. C.1,2,3; Hu, X. J.23; Huang, D. H.8; Huang, Q. L.1,3; Huang, W. H.22; Huang, X. T.22; Huang, X. Y.13; Huang, Z. C.8; Ji, F.1,3; Ji, X. L.1,3,6; Jia, H. Y.8; Jiang, K.6,7; Jiang, Z. J.20; Jin, C.1,2,3; Ke, T.1,3; Kuleshov, D.26; Levochkin, K.26; Li, B. B.14; Li, Cheng6,7; Li, Cong1,3; Li, F.1,3,6; Li, H. B.1,3; Li, H. C.1,3; Li, H. Y.7,13; Li, Jian7; Li, Jie1,3,6; Li, K.1,3; Li, W. L.22; Li, X. R.1,3; Li, Xin6,7; Li, Xin8; Li, Y.9; Li, Y. Z.1,2,3; Li, Zhe1,3; Li, Zhuo27; Liang, E. W.28; Liang, Y. F.28; Lin, S. J.18; Liu, B.7; Liu, C.1,3; Liu, D.22; Liu, H.8; Liu, H. D.24; Liu, J.1,3; Liu, J. L.29; Liu, J. S.18; Liu, J. Y.1,3; Liu, M. Y.16; Liu, R. Y.10; Liu, S. M.8; Liu, W.1,3; Liu, Y.11; Liu, Y. N.23; Liu, Z. X.9; Long, W. J.8; Lu, R.20; Lv, H. K.1,3; Ma, B. Q.27; Ma, L. L.1,3; Ma, X. H.1,3; Mao JR(毛基荣)25; Masood, A.8; Min, Z.1,3; Mitthumsiri, W.30; Montaruli, T.21; Nan, Y. C.22; Pang, B. Y.8; Pattarakijwanich, P.30; Pei, Z. Y.11; Qi, M. Y.1,3; Qi, Y. Q.14; Qiao, B. Q.1,3; Qin, J. J.7; Ruffolo, D.30; Rulev, V.26; Sáiz, A.30; Shao, L.14; Shchegolev, O.26,31; Sheng, X. D.1,3; Shi, J. R.1,3; Song, H. C.27; Stenkin, Yu. V.26,31; Stepanov, V.26; Su, Y.13; Sun, Q. N.8; Sun, X. N.28; Sun, Z. B.32; Tam, P. H. T.18; Tang, Z. B.6,7; Tian, W. W.2,17; Wang, B. D.1,3; Wang, C.32; Wang, H.8; Wang, H. G.11; Wang JC(王建成)25; Wang, J. S.29; Wang, L. P.22; Wang, L. Y.1,3; Wang, R. N.8; Wang, W.18; Wang, W.12; Wang, X. G.28; Wang, X. J.1,3; Wang, X. Y.10; Wang, Y.8; Wang, Y. D.1,3; Wang, Y. J.1,3; Wang, Y. P.1,2,3; Wang, Z. H.9; Wang, Z. X.20; Wang, Zhen29; Wang, Zheng1,3,6; Wei, D. M.13; Wei, J. J.13; Wei, Y. J.1,2,3; Wen, T.20; Wu, C. Y.1,3; Wu, H. R.1,3; Wu, S.1,3; Wu, W. X.8; Wu, X. F.13; Xi, S. Q.1,3; Xia, J.7,13; Xia, J. J.8; Xiang, G. M.2,15; Xiao, D. X.16; Xiao, G.1,3; Xiao, H. B.11; Xin, G. G.12; Xin, Y. L.8; Xing, Y.15; Xu, D. L.29; Xu, R. X.27; Xue, L.22; Yan DH(闫大海)25; Yan, J. Z.13; Yang, C. W.9; Yang, F. F.1,3,6; Yang, J. Y.18; Yang, L. L.18; Yang, M. J.1,3; Yang, R. Z.7; Yang, S. B.20; Yao, Y. H.9; Yao, Z. G.1,3; Ye, Y. M.23; Yin, L. Q.1,3; Yin, N.22; You, X. H.1,3; You, Z. Y.1,2,3; Yu, Y. H.22; Yuan, Q.13; Zeng, H. D.13; Zeng, T. X.1,3,6; Zeng, W.20; Zeng, Z. K.1,2,3; Zha, M.1,3; Zhai, X. X.1,3; Zhang, B. B.10; Zhang, H. M.10; Zhang, H. Y.22; Zhang, J. L.17; Zhang, J. W.9; Zhang, L. X.11; Zhang, Li20; Zhang, Lu14; Zhang, P. F.20; Zhang, P. P.14; Zhang, R.7,13; Zhang, S. R.14; Zhang, S. S.1,3; Zhang, X.10; Zhang, X. P.1,3; Zhang, Y. F.8; Zhang, Y. L.1,3; Zhang, Yi1,13; Zhang, Yong1,3; Zhao, B.8; Zhao, J.1,3; Zhao, L.6,7; Zhao, L. Z.14; Zhao, S. P.13,22; Zheng, F.32; Zheng, Y.8; Zhou, B.1,3; Zhou, H.29; Zhou, J. N.15; Zhou, P.10; Zhou, R.9; Zhou, X. X.8; Zhu, C. G.22; Zhu, F. R.8; Zhu, H.17; Zhu, K. J.1,2,3,6; Zuo, X.1,3
Source PublicationPHYSICAL REVIEW LETTERS
2022-02-03
Volume128Issue:5
DOI10.1103/PhysRevLett.128.051102
Contribution Rank第25完成单位
Indexed BySCI ; EI
Keyword
Abstract

Recently, the LHAASO Collaboration published the detection of 12 ultrahigh-energy gamma-ray sources above 100 TeV, with the highest energy photon reaching 1.4 PeV. The first detection of PeV gamma rays from astrophysical sources may provide a very sensitive probe of the effect of the Lorentz invariance violation (LIV), which results in decay of high-energy gamma rays in the superluminal scenario and hence a sharp cutoff of the energy spectrum. Two highest energy sources are studied in this work. No signature of the existence of the LIV is found in their energy spectra, and the lower limits on the LIV energy scale are derived. Our results show that the first-order LIV energy scale should be higher than about 105 times the Planck scale M-Pl and that the second-order LIV scale is > 10(-3)M(Pl). Both limits improve by at least one order of magnitude the previous results.

Funding ProjectNational Key R&D program of China[2018YFA0404202] ; National Key R&D program of China[2018YFA0404201] ; National Key R&D program of China[2018YFA0404203] ; National Key R&D program of China[2018YFA0404204] ; National Natural Science Foundation of ChinaNational Natural Science Foundation of China (NSFC)[12175248] ; National Natural Science Foundation of ChinaNational Natural Science Foundation of China (NSFC)[11635011] ; National Natural Science Foundation of ChinaNational Natural Science Foundation of China (NSFC)[11775233] ; National Natural Science Foundation of ChinaNational Natural Science Foundation of China (NSFC)[12022502] ; National Natural Science Foundation of ChinaNational Natural Science Foundation of China (NSFC)[U2031201] ; Chinese Academy of SciencesChinese Academy of Sciences ; Program for Innovative Talents and Entrepreneur in Jiangsu ; Chengdu Management Committee of Tianfu New Area
Funding OrganizationNational Key R&D program of China[2018YFA0404202, 2018YFA0404201, 2018YFA0404203, 2018YFA0404204] ; National Natural Science Foundation of ChinaNational Natural Science Foundation of China (NSFC)[12175248, 11635011, 11775233, 12022502, U2031201] ; Chinese Academy of SciencesChinese Academy of Sciences ; Program for Innovative Talents and Entrepreneur in Jiangsu ; Chengdu Management Committee of Tianfu New Area
Language英语
Subject Area天文学 ; 天体物理学 ; 高能天体物理学
MOST Discipline Catalogue理学 ; 理学::天文学
SubtypeArticle
PublisherAMER PHYSICAL SOC
Publication PlaceONE PHYSICS ELLIPSE, COLLEGE PK, MD 20740-3844 USA
ISSN0031-9007
URL查看原文
WOS IDWOS:000759200500008
WOS Research AreaPhysics
WOS SubjectPhysics, Multidisciplinary
WOS KeywordQUANTUM-GRAVITY ; SPACE-TIME ; TESTS ; CONSTRAINTS
EI Accession Number20221111771144
EI KeywordsSpectroscopy
EI Classification Number931.3 Atomic and Molecular Physics - 932.1 High Energy Physics
Citation statistics
Document Type期刊论文
Version出版稿
Identifierhttp://ir.ynao.ac.cn/handle/114a53/24957
Collection高能天体物理研究组
星系类星体研究组
Corresponding AuthorCao, Zhen
Affiliation1.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, Chengdu, 610000 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.State Key Laboratory of Particle Detection and Electronics, 100049 Beijing, China;
7.University of Science and Technology of China, 230026 Hefei, Anhui, China;
8.School of Physical Science and Technology and School of Information Science and Technology, Southwest Jiaotong University, 610031 Chengdu, Sichuan, China;
9.College of Physics, Sichuan University, 610065 Chengdu, Sichuan, China;
10.School of Astronomy and Space Science, Nanjing University, 210023 Nanjing, Jiangsu, China;
11.Center for Astrophysics, Guangzhou University, 510006 Guangzhou, Guangdong, China;
12.School of Physics and Technology, Wuhan University, 430072 Wuhan, Hubei, China;
13.Key Laboratory of Dark Matter and Space Astronomy, Purple Mountain Observatory, Chinese Academy of Sciences, 210023 Nanjing, Jiangsu, China;
14.Hebei Normal University, 050024 Shijiazhuang, Hebei, China;
15.Key Laboratory for Research in Galaxies and Cosmology, Shanghai Astronomical Observatory, Chinese Academy of Sciences, 200030 Shanghai, China;
16.Key Laboratory of Cosmic Rays (Tibet University), Ministry of Education, 850000 Lhasa, Tibet, China;
17.National Astronomical Observatories, Chinese Academy of Sciences, 100101 Beijing, China;
18.School of Physics and Astronomy and School of Physics (Guangzhou), Sun Yat-sen University, 519000 Zhuhai, Guangdong, China;
19.Dipartimento di Fisica dell’Università di Napoli “Federico II,” Complesso Universitario di Monte Sant’Angelo, via Cinthia, 80126 Napoli, Italy;
20.School of Physics and Astronomy, Yunnan University, 650091 Kunming, Yunnan, China;
21.Département de Physique Nucléaire et Corpusculaire, Faculté de Sciences, Université de Genève, 24 Quai Ernest Ansermet, 1211 Geneva, Switzerland;
22.Institute of Frontier and Interdisciplinary Science, Shandong University, 266237 Qingdao, Shandong, China;
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.Institute for Nuclear Research of Russian Academy of Sciences, 117312 Moscow, Russia;
27.School of Physics, Peking University, 100871 Beijing, China;
28.School of Physical Science and Technology, Guangxi University, 530004 Nanning, Guangxi, China;
29.Tsung-Dao Lee Institute and School of Physics and Astronomy, Shanghai Jiao Tong University, 200240 Shanghai, China;
30.Department of Physics, Faculty of Science, Mahidol University, 10400 Bangkok, Thailand;
31.Moscow Institute of Physics and Technology, 141700 Moscow, Russia;
32.National Space Science Center, Chinese Academy of Sciences, 100190 Beijing, China
Recommended Citation
GB/T 7714
Cao, Zhen,Aharonian, F.,An, Q.,et al. Exploring Lorentz Invariance Violation from Ultrahigh-Energy gamma[J]. PHYSICAL REVIEW LETTERS,2022,128(5).
APA Cao, Zhen.,Aharonian, F..,An, Q..,Axikegu.,Bai, L. X..,...&Zuo, X..(2022).Exploring Lorentz Invariance Violation from Ultrahigh-Energy gamma.PHYSICAL REVIEW LETTERS,128(5).
MLA Cao, Zhen,et al."Exploring Lorentz Invariance Violation from Ultrahigh-Energy gamma".PHYSICAL REVIEW LETTERS 128.5(2022).
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