Peta-electron volt gamma-ray emission from the Crab Nebula

Collaboration, Lhaaso; della Volpe, D.; Aharonian, F.; An, Q.; Cao, Zhen; Axikegu, Q. A.; Bai, L.~X X.; Bai, Y.~X X.; Bao, Y.~W W.; Bastieri, D.; Bi, X.~J J.; Bi, Y.~J J.; Cai, H.; Cao, Zhe; Cai, J.~T T.; Chang, J.; Chang, J.~F F.; Chen, B.~M M.; Chen, E.~S S.; Chen, J.; Chen, Liang; Chen, Long; Chen, M. J.; Chen, M.~J L.; Chen, M.~L; Chen, Q. H.; Chen, Q.~H; Chen, S. H.; Chen, S.~H Z.; Chen, S.~Z; Chen, T. L.; Chen, T.~L; Chen, X. L.; Chen, X.~L; Chen, Y.; Cheng, N.; Cheng, Y.~D D.; Cui, S.~W W.; Cui, X.~H H.; Cui, Y.~D D.; D'Ettorre Piazzoli, B.; D’Ettorre Piazzoli, B.; Dai, B.~Z Z.; Dai, H.~L L.; Dai, Z.~G G.; Danzengluobu,; Volpe, Della; Dong, X.~J J.; Duan, K.~K K.; Fan, J.~H H.; Fan, Y.~Z Z.; Fan, Z.~X X.; Fang, J.; Fang, K.; Feng, C.~F F.; Feng, L.; Feng, S.~H H.; Feng, Y.~L L.; Gao, B.; Gao, C.~D D.; Gao, L.~Q Q.; Gao, Q.; Gao, W.; Ge, M.~M M.; Geng, L.~S S.; Gong, G.~H H.; Gou, Q.~B B.; Gu, M.~H H.; Guo, F.~L L.; Guo, J.~G G.; Guo, X.~L L.; Guo, Y.~Q Q.; Guo, Y.~Y Y.; Han, Y.~A A.; He, H.~H H.; He, H.~N N.; He, J.~C C.; He, S.~L L.; He, X.~B B.; He, Y.; Heller, M.; Hor, Y.~K K.; Hou, C.; Hou, X.; Hu, H.~B B.; Hu, S.; Hu, S.~C C.; Hu, X.~J J.; Huang, D.~H H.; Huang, Q.~L L.; Huang, W.~H H.; Huang, X.~T T.; Huang, X.~Y Y.; Huang, Z.~C C.; Ji, F.; Ji, X.~L L.; Jia, H.~Y Y.; Jiang, K.; Jiang, Z.~J J.; Jin, C.; Ke, T.; Kuleshov, D.; Levochkin, K.; Li, B.~B B.; Li, Cheng; Li, Cong; Li, F.; Li, H.~B B.; Li, H.~C C.; Li, H.~Y Y.; Li, Jian; Li, Jie; Li, K.; Li, W.~L L.; Li, X.~R R.; Li, Xin; Li, Xin R.; Li, Y.; Li, Y.~Z Z.; Li, Zhe; Li, Zhuo; Liang, E.~W W.; Liang, Y.~F F.; Lin, S.~J J.; Liu, B.; Liu, C.; Liu, D.; Liu, H.; Liu, H.~D D.; Liu, J.; Liu, J.~L L.; Liu, J.~S S.; Liu, J.~Y Y.; Liu, M.~Y Y.; Liu, R.~Y Y.; Liu, S.~M M.; Liu, W.; Liu, Y.; Liu, Y.~N N.; Liu, Z.~X X.; Long, W.~J J.; Lu, R.; Lv, H.~K K.; Ma, B.~Q Q.; Ma, L.~L L.; Ma, X.~H H.; Mao, J.~R R.; Masood, A.; Min, Z.; Mitthumsiri, W.; Montaruli, T.; Nan, Y.~C C.; Pang, B.~Y Y.; Pattarakijwanich, P.; Pei, Z.~Y Y.; Qi, M.~Y Y.; Qi, Y.~Q Q.; Qiao, B.~Q Q.; Qin, J.~J J.; Ruffolo, D.; Rulev, V.; Saiz, A.; Shao, L.; Shchegolev, O.; Sheng, X.~D D.; Shi, J.~Y Y.; Song, H.~C C.; Stenkin, Yu-U. V.; Stepanov, V.; Su, Y.; Sun, Q.~N N.; Sun, X.~N N.; Sun, Z.~B B.; Tam, P.~H.~T H. T.; Tang, Z.~B B.; Tian, W.~W W.; Wang, B.~D D.; Wang, C.; Wang, H.; Wang, H.~G G.; Wang, J.~C C.; Wang, J.~S S.; Wang, L.~P P.; Wang, L.~Y Y.; Wang, R.~N N.; Wang, Wei; Wang, X. G.; Wang, X.~G J.; Wang, X.~J Y.; Wang, X.~Y; Wang, Y. D.; Wang, Y. J.; Wang, Y.~D P.; Wang, Y.~J; Wang, Z. H.; Wang, Y.~P; Wang, Zhen H.; Wang, Z. X.; Wang, Zheng X.; Wang, Zheng; Wei, D.~M M.; Wei, J.~J J.; Wei, Y.~J J.; Wen, T.; Wu, C.~Y Y.; Wu, H.~R R.; Wu, S.; Wu, W.~X X.; Wu, X.~F F.; Xi, S.~Q Q.; Xia, J.; Xia, J.~J J.; Xiang, G.~M M.; Xiao, D.~X X.; Xiao, G.; Xiao, H.~B B.; Xin, G.~G G.; Xin, Y.~L L.; Xing, Y.; Xu, D.~L L.; Xu, R.~X X.; Xue, L.; Yan, D.~H H.; Yan, J.~Z Z.; Yang, C.~W W.; Yang, F.~F F.; Yang, J.~Y Y.; Yang, L.~L L.; Yang, M.~J J.; Yang, R.~Z Z.; Yang, S.~B B.; Yao, Y.~H H.; Yao, Z.~G G.; Ye, Y.~M M.; Yin, L.~Q Q.; Yin, N.; You, X.~H H.; You, Z.~Y Y.; Yu, Y.~H H.; Yuan, Q.; Zeng, H.~D D.; Zeng, T.~X X.; Zeng, W.; Zeng, Z.~K K.; Zha, M.; Zhai, X.~X X.; Zhang, B.~B B.; Zhang, H.~M M.; Zhang, H.~Y Y.; Zhang, J.~L L.; Zhang, J.~W W.; Zhang, L.~X X.; Zhang, Li; Zhang, Lu; Zhang, P.~F F.; Zhang, P.~P P.; Zhang, R.; Zhang, S.~R R.; Zhang, S.~S S.; Zhang, X.; Zhang, X.~P P.; Zhang, Y.~F F.; Zhang, Yi F.; Zhang, Y.~L L.; Zhang, Yong L.; Zhao, B.; Zhao, J.; Zhao, L.; Zhao, L.~Z Z.; Zhao, S.~P P.; Zheng, F.; Zheng, Y.; Zhou, B.; Zhou, H.; Zhou, J.~N N.; Zhou, P.; Zhou, R.; Zhou, X.~X X.; Zhu, C.~G G.; Zhu, F.~R R.; Zhu, H.; Zhu, K.~J J.; Zuo, X.

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American Association for the Advancement of Science, Science, 6553(373), p. 425-430, 2021

DOI: 10.1126/science.abg5137

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Peta-electron volt gamma-ray emission from the Crab Nebula

Journal article published in 2021 by Lhaaso Collaboration, D. della Volpe, F. Aharonian

, Q. An, Zhen Cao, Q. A. Axikegu, L.~X X. Bai, Y.~X X. Bai, Y.~W W. Bao, D. Bastieri, X.~J J. Bi, Y.~J J. Bi, H. Cai, Zhe Cao, J.~T T. Cai and other authors.

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Abstract

High-energy photons from the Crab Nebula The Crab Nebula contains a pulsar that excites the surrounding gas to emit high-energy radiation. The combination of the pulsar's youth and nearby location makes the nebula the brightest gamma-ray source in the sky. The LHAASO Collaboration report observations of this source at energies of tera– to peta–electron volts, extending the spectrum of this prototypical object. They combine these data with observations at lower energies to model the physics of the emission process. The multiwave-length data can be explained by a combination of synchrotron radiation and inverse Compton scattering. Science , abg5137, this issue p. 425

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Peta-electron volt gamma-ray emission from the Crab Nebula

Abstract