Z
Zi-Gao Dai
Researcher at Nanjing University
Publications - 439
Citations - 13461
Zi-Gao Dai is an academic researcher from Nanjing University. The author has contributed to research in topics: Gamma-ray burst & Neutron star. The author has an hindex of 60, co-authored 412 publications receiving 12069 citations. Previous affiliations of Zi-Gao Dai include Wuhan University & Chinese Ministry of Education.
Papers
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Journal ArticleDOI
Repeating Fast Radio Bursts from Pulsar-Asteroid Belt Collisions: Frequency Drifting and Polarization
TL;DR: In this article, the authors focus on the prediction of time-frequency drifting and polarization of fast radio bursts (FRBs) and find that a broad frequency band of the FRBs would be expected, due to the mass difference of the incident asteroids.
Journal ArticleDOI
Neutrino emission from a GRB afterglow shock during an inner supernova shock breakout
TL;DR: In this article, neutrino emission for early afterglows of GRB 060218-like GRBs was studied, where neutrinos are expected to be produced from photopion interactions in a GRB blast wave that propagates into a dense wind.
Insight-HXMT and GECAM-C observations of the brightest-of-all-time GRB 221009A
Z. H. An,S. Antier,Xingzi Bi,Qingcui Bu,C. Cai,X. L. Cao,A. Camisasca,Zhi Chang,Gang Chen,Li Sheng Chen,Tian-Xiang Chen,Wen Chen,Yibao Chen,Yong Chen,Yu-Peng Chen,Michael W. Coughlin,Weinan Cui,Zi-Gao Dai,T. Hussenot-Desenonges,Yanqi Du,Yuanyuan Du,Yunping Du,Chengwei Fan,F. Frontera,He Gao,Min Gao,Ming-Yu Ge,Ke Gong,Yu-Dong Gu,Ju Guan,Dong Ya Guo,Zhibi Guo,C. Guidorzi,Da-Wei Han,JianJian He,Jun He,Dongjie Hou,Yue Huang,Jiabin Huo,Zhenyu Ji,Shu-Mei Jia,D. A. Kann,A. Klotz,L. D. Kong,Lin Lan,Andi Li,Chaoyang Li,Cheng-Kui Li,Gang Li,Mao-Shun Li,Ti-Pei Li,Wei Li,Xiaobo Li,Xinqiao Li,Xufang Li,Yanguo Li,Zheng-Wei Li,Jing Yue Liang,Xiaoxing Liang,Jin-Yuan Liao,Lin Lin,Congzhan Liu,Hengbo Liu,Hong-wei Liu,Jiacong Liu,Xiao-jing Liu,Yaling Liu,Yu-Rong Liu,Fang Lu,Hong Lu,Xuefeng Lu,Qiumin Luo,Tao Luo,Bin Ma,Fusheng Ma,R. Ma,R.R. Maccary,Jinbin Mao,Bin Meng,Jianyin Nie,Mauro Orlandini,Ge Ou,J. Peng,Wenxi Peng,Rui Qiao,Jinglian Qu,Xiaochen Ren,Jingyuan Shi,Qiannan Shi,Li-Ming Song,Xinying Song,J. Su,G. X. Sun,Liang Sun,Xilei Sun,Wenqing Tan,Ying Tan,L. Tao,Y. L. Tuo,D. Turpin,Jin-zhou Wang,Chen Wang,Chenwei Wang,Hong-jun Wang,Hui Wang,Jin Wang,Lingjue Wang,Pengjie Wang,Ping Wang,Wenshuai Wang,Xiangyou Wang,Xilai Wang,Yu-Sa Wang,Yue Wang,XiangYang Wen,Bo Wu,B. Y. Wu,Hong-jie Wu,Shengbing Xiao,S. Xiao,Yunlong Xiao,Shengrong Xie,Shaolin Xiong,Senlin Xiong,Dong Xu,Yanqing Xu,Ying Xu,Yuqing Xu,W. C. Xue,Sheng Yang,Yanjuan Yang,Zihao Yang,Wentao Ye,Q. B. Yi,Shuyu Yi,Q. Q. Yin,Yuan You,Yunwei Yu,Wei Yu,Wenzhong Yu,Ming Zeng,Ning Zhang,Bing Zhang,Dali Zhang,Fan Zhang,HongMei Zhang,Juan Zhang,Liang Zhang,Feng Zhang,Shu Zhang,Shuang-Nan Zhang,Wan-Chang Zhang,Xiaofei Zhang,Xiaolong Zhang,Yanqiu Zhang,Yan-ting Zhang,Yifei Zhang,Yuanyang Zhang,Zhen Yi Zhang,Guoyan Zhao,Hai-Sheng Zhao,Hong-Yu Zhao,Qingyu Zhao,Shuping Zhao,Xiaohong Zhao,Xiao-Yan Zhao,Yi Zhao,Chao Zheng,Shi-Jie Zheng,D. K. Zhou,Xing Zhou,Xiaoli Zhu +171 more
TL;DR: In this paper , the authors measured the isotropic equivalent energy of the gamma-ray burst of GRB 221009A, including its precursor, main emission (ME), flaring emission and early afterglow, in the hard X-ray to soft gamma ray band from 10 keV to 6 MeV.
Journal ArticleDOI
Emission from a Pulsar Wind Nebula: Application to the Persistent Radio Counterpart of FRB 121102
Yu-Han Yang,Zi-Gao Dai +1 more
TL;DR: In this article, a pulsar wind nebula powered by a magnetar without surrounding supernova ejecta was proposed as a radio counterpart of fast radio bursts (FRBs) and the model parameters were constrained by the spectrum of the counterpart emission, the size of the nebula, and the large but decreasing rotation measure (RM) of the repeating bursts.
Journal ArticleDOI
GRB 211211A: A Neutron Star–White Dwarf Merger?
TL;DR: In this paper , the gamma-ray burst of GRB 211211A and its associated kilonova-like emission were reported, and it was shown that this association event may arise from a neutron star-white dwarf (NS-WD) merger if the central engine leaves a magnetar behind.