A tera–electron volt afterglow from a narrow jet in an extremely bright gamma-ray burst

作者：Z. Cao, F. Aharonian, Qier An, Axikegu, Lixin Bai, Y. X. Bai, Y. W. Bao, D. Bastieri, Xiao-Jun Bi, Y. J. Bi, J. T. Cai, Qing Ping Cao, Weiwei Cao, Zhe Cao, Jin Chang, Jin Chang, E. S. Chen, Liang Chen, Lin Chen, Long Chen, M. J. Chen, Mingliang Chen, Q. H. Chen, Shaw Horng Chen, S. Z. Chen, T. L. Chen, Ye Chen, H. L. Cheng, Na Cheng, Yaodong Cheng, S. W. Cui, X. H. Cui, Y. D. Cui, B. Z. Dai, H. L. Dai, Zi-Gao Dai, Danzengluobu Danzengluobu, D. della Volpe, X. Q. Dong, K. K. Duan, J. H. Fan, Y. Z. Fan, J. Fang, Kun Fang, Chunsheng Feng, Li Feng, S. H. Feng, X. T. Feng, Y. L. Feng, B. S. Gao, C. D. Gao, L. Q. Gao, Qinhe Gao, Wei Gao, Wei Gao, M. M. Ge, Li‐Sheng Geng, G. Gong, Q. B. Gou, M. H. Gu, Fulai Guo, X. L. Guo, Yi-Qing Guo, Y. Y. Guo, Y. A. Han, H. H. He, Hao-Ning He, Jiawei He, X. B. He, Y. He, Matthieu Heller, Y. K. Hor, B. W. Hou, Changming Hou, X. T. Hou, H. B. Hu, Qi Hu, S. C. Hu, D. Huang, T. Q. Huang, W. J. Huang, X. T. Huang, X. Y. Huang, Y. Huang, Zhongjie Huang, X. L. Ji, H. Y. Jia, Kaixuan Jia, K. Jiang, X. W. Jiang, Z. J. Jiang, Ming Liang Jin, M. M. Kang, Tengfei Ke, Denis Kuleshov, K. Kurinov, Bing Li, Cheng Li, Cong Li, Di Li, Fenfang Li, Hao Li, H. C. Li, H. Y. Li, Jian Li, Jian Li, Jie Li, K. Li, Wenwen Li, Wenwen Li, X. R. Li, Xin Li, Yanqi Li, Zhe Li, Zhuo Li, E. W. Liang, Yun-Feng Liang, S. J. Lin, B. Liu, Chunhong Liu, Desheng Liu, Huamei Liu, H. D. Liu, Jian Liu, J. L. Liu, J. L. Liu, J. S. Liu, J. Y. Liu, M. Y. Liu, Ruo-Yu Liu, S. M. Liu, Wan-cheng Liu, Yueliang Liu, Y. N. Liu, W. J. Long, R. Lu, Q. Luo, H. K. Lv, B. Q., L. L., X. H. Ma, J.R Mao, Z. Min, W. Mitthumsiri, Y. C. Nan, Z. W. Ou, B. Y. Pang, P. Pattarakijwanich, Z. Y. Pei, M. Qi, Y. Q. Qi, Bing-Qiang Qiao, Jiajun Qin, D. Ruffolo, A. Sáiz, C. Y. Shao, L. Shao, OLeg B. Shchegolev, X. D. Sheng, H. C. Song, Yu. V. Stenkin, V. Stepanov, Yang Su, Q. N. Sun, X. N. Sun, Zhenyu Sun, P. H. T. Tam, Z. Tang, Wei Tian, Chun Wang, Chuxuan Wang, Guangwei Wang, H. G. Wang, H. H. Wang, J. C. Wang, J. S. Wang, Kang Wang, L. P. Wang, L. Y. Wang, P. H. Wang, Rong Wang, Wei Wang, Xiang-Gao Wang, Xiang‐Yu Wang, Yuwen Wang, Y. D. Wang, Yingjie Wang, Zining Wang, Z. X. Wang, Zhen Wang, Zheng Wang, D. M. Wei, J. J. Wei, Yifan Wei, T. Wen, C. Y. Wu, H. R. Wu, Sha Sha Wu, Xue-Feng Wu, Yuping Wu, Shao-Qiang Xi, J. Xia, J. Xia, G. M. Xiang, D. X. Xiao, Guang-Cheng Xiao, G. G. Xin, Y. Xin, Yi Xing, Zhenyang Xiong, D. L. Xu, R. F. Xu, Rong Xu, L. Xue, Dahai Yan, Jun Yan, T Yan, C. W. Yang, Fan Yang, Fei Yang, H. W. Yang, J. Y. Yang, Lili Yang, Min Jae Yang, Ruizhi Yang, S. B. Yang, Yuhua Yao, Z. G. Yao, Y. M. Ye, L. Q. Yin, N. Yin, X. H. You, Zhanping You, Yonglin Yu, Qiang Yuan, H. Yue, Houdun Zeng, T. X. Zeng, W. Zeng, Z. K. Zeng, Min Zha, Bing Zhang, Bin‐Bin Zhang, F. Zhang, Hai-Ming Zhang, H. Y. Zhang, Jiajia Zhang, Lixia Zhang, L. Zhang, P. F. Zhang, P. P. Zhang, Rui Zhang, Songbo Zhang, S. R. Zhang, S. S. Zhang, Xiao Zhang, X. P. Zhang, Y. F. Zhang, Yong Zhang, Yong Zhang, Bowen Zhao, Jinmiao Zhao, Lei Zhao, L. Z. Zhao, Shunsheng Zhao, F. Zheng, Jian-He Zheng, Bin Zhou, Hao Zhou, Jingzhi Zhou, Ping Zhou, Rong Zhou, X. X. Zhou, C. G. Zhu, F. R. Zhu, Hui Zhu, Kai Zhu, X. Zuo · 发表于：Science · 年份：2023 · DOI：10.1126/science.adg9328 · 被引用次数：220 · 研究领域：Gamma-ray bursts and supernovae、Astrophysics and Cosmic Phenomena、Pulsars and Gravitational Waves Research

Some gamma-ray bursts (GRBs) have a tera-electron volt (TeV) afterglow, but the early onset of this has not been observed. We report observations with the Large High Altitude Air Shower Observatory (LHAASO) of the bright GRB 221009A, which serendipitously occurred within the instrument's field of view. More than 64,000 photons >0.2 TeV were detected within the first 3000 seconds. The TeV flux began several minutes after the GRB trigger and then rose to a peak ~10 seconds later. This was followed by a decay phase, which became more rapid ~650 seconds after the peak. We interpret the emission using a model of a relativistic jet with half-opening angle of ~0.8°. This is consistent with the core of a structured jet and could explain the high isotropic energy of this GRB.