李军_西藏大学机构知识库

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李军

职称：教授
研究方向：中国语言文学
学科领域：教育，汉语，中国文学，中国史，音乐
所属二级机构：文学院
成果数量：57条 ,属于文学院数量为:20条

检索结果：返回 57 结果。

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期刊

唐朝初期中原与吐蕃佛教交融依存语境解读中文核心期刊(北大)

作者：李军，周志琴（西藏大学文学院）
出处：西藏大学学报(社会科学版) 2024 第39卷第1期 P95-100
关键词：唐朝吐蕃佛教交融依存
摘要：吐蕃与唐朝因中原佛教结缘，而双方的交融依存发端于唐朝重启了儒家孟子性善论仁道思想，摒弃了过去天赋神权论的儒家思想。儒学扬弃之后在唐朝初期强调“仁”道，唐朝因“仁”和合吐蕃，佛教的中国化也在唐朝初期有了新的面目：“提倡众生平等”。儒学的“仁”转化为佛学的“众生平等”理念，形成了吐蕃与中原的基本交往范式

期刊

Optimization of performance of the KM2A full array using the Crab Nebula Scopus文摘索引数据库(荷)

作者： Zhen Cao ，F. Aharonian，Q. An ，Axikegu ，Y.X. Bai ，Y.W. Bao ，D. Bastieri，X.J. Bi ，Y.J. Bi ，J.T. Cai ，Q. Cao ，W.Y. Cao ，Zhe Cao ，J. Chang ，J.F. Chang ，A.M. Chen ，E.S. Chen ，Liang Chen ，Lin Chen ，Long Chen ，M.J. Chen ，M.L. Chen ，Q.H. Chen ，S.H. Chen ，T.L. Chen ，Y. Chen ，N. Cheng ，Y.D. Cheng ，M.Y. Cui ，S.W. Cui ，X.H. Cui ，Y.D. Cui ，B.Z. Dai ，H.L. Dai ，Z.G. Dai ，Danzengluobu ，D. della Volpe，X.Q. Dong ，K.K. Duan ，J.H. Fan ，Y.Z. Fan ，J. Fang ，K. Fang ，C.F. Feng ，L. Feng ，S.H. Feng ，X.T. Feng ，Y.L. Feng ，S. Gabici，B. Gao ，C.D. Gao ，L.Q. Gao ，Q. Gao ，W. Gao ，W.K. Gao ，M.M. Ge ，L.S. Geng ，G. Giacinti，G.H. Gong ，Q.B. Gou ，M.H. Gu ，F.L. Guo ，X.L. Guo ，Y.Q. Guo ，Y.Y. Guo ，Y.A. Han ，H.H. He ，H.N. He ，J.Y. He ，X.B. He ，Y. He ，M. Heller，Y.K. Hor ，B.W. Hou ，C. Hou ，X. Hou ，H.B. Hu ，Q. Hu ，S.C. Hu ，D.H. Huang ，T.Q. Huang ，W.J. Huang ，X.T. Huang ，X.Y. Huang ，Y. Huang ，Z.C. Huang ，X.L. Ji ，H.Y. Jia ，K. Jia ，K. Jiang ，X.W. Jiang ，Z.J. Jiang ，M. Jin ，M.M. Kang ，T. Ke ，D. Kuleshov，K. Kurinov，B.B. Li ，Cheng Li ，Cong Li ，D. Li ，F. Li ，H.B. Li ，H.C. Li ，H.Y. Li ，J. Li ，Jian Li ，Jie Li ，K. Li ，W.L. Li ，W.L. Li ，X.R. Li ，Xin Li ，Y.Z. Li ，Zhe Li ，Zhuo Li ，E.W. Liang ，Y.F. Liang ，S.J. Lin ，B. Liu ，C. Liu ，D. Liu ，H. Liu ，H.D. Liu ，J. Liu ，J.L. Liu ，J.Y. Liu ，M.Y. Liu ，R.Y. Liu ，S.M. Liu ，W. Liu ，Y. Liu ，Y.N. Liu ，R. Lu ，Q. Luo ，H.K. Lv ，B.Q. Ma ，L.L. Ma ，X.H. Ma ，J.R. Mao ，Z. Min ，W. Mitthumsiri，H.J. Mu ，Y.C. Nan ，A. Neronov，Z.W. Ou ，B.Y. Pang ，P. Pattarakijwanich，Z.Y. Pei ，M.Y. Qi ，Y.Q. Qi ，B.Q. Qiao ，J.J. Qin ，D. Ruffolo，A. Sáiz，D. Semikoz，C.Y. Shao ，L. Shao ，O. Shchegolev，X.D. Sheng ，F.W. Shu ，H.C. Song ，Yu.V. Stenkin，V. Stepanov，Y. Su ，Q.N. Sun ，X.N. Sun ，Z.B. Sun ，P.H.T. Tam ，Q.W. Tang ，Z.B. Tang ，W.W. Tian ，C. Wang ，C.B. Wang ，G.W. Wang ，H.G. Wang ，H.H. Wang ，J.C. Wang ，K. Wang ，L.P. Wang ，L.Y. Wang ，P.H. Wang ，R. Wang ，W. Wang ，X.G. Wang ，X.Y. Wang ，Y. Wang ，Y.D. Wang ，Y.J. Wang ，Z.H. Wang ，Z.X. Wang ，Zhen Wang ，Zheng Wang ，D.M. Wei ，J.J. Wei ，Y.J. Wei ，T. Wen ，C.Y. Wu ，H.R. Wu ，S. Wu ，X.F. Wu ，Y.S. Wu ，S.Q. Xi ，J. Xia ，J.J. Xia ，G.M. Xiang ，D.X. Xiao ，G. Xiao ，G.G. Xin ，Y.L. Xin ，Y. Xing ，Z. Xiong ，D.L. Xu ，R.F. Xu ，R.X. Xu ，W.L. Xu ，L. Xue ，D.H. Yan ，J.Z. Yan ，T. Yan ，C.W. Yang ，F. Yang ，F.F. Yang ，H.W. Yang ，J.Y. Yang ，L.L. Yang ，M.J. Yang ，R.Z. Yang ，S.B. Yang ，Y.H. Yao ，Z.G. Yao ，Y.M. Ye ，L.Q. Yin ，N. Yin ，X.H. You ，Z.Y. You ，Y.H. Yu ，Q. Yuan ，H. Yue ，H.D. Zeng ，T.X. Zeng ，W. Zeng ，M. Zha ，B.B. Zhang ，F. Zhang ，H.M. Zhang ，H.Y. Zhang ，J.L. Zhang ，L.X. Zhang ，Li Zhang ，P.F. Zhang ，P.P. Zhang ，R. Zhang ，S.B. Zhang ，S.R. Zhang ，S.S. Zhang ，X. Zhang ，X.P. Zhang ，Y.F. Zhang ，Yi Zhang ，Yong Zhang ，B. Zhao ，J. Zhao ，L. Zhao ，L.Z. Zhao ，S.P. Zhao ，F. Zheng ，B. Zhou ，H. Zhou ，J.N. Zhou ，M. Zhou ，P. Zhou ，R. Zhou ，X.X. Zhou ，C.G. Zhu ，F.R. Zhu ，H. Zhu ，K.J. Zhu ，X. Zuo ，（ ¹Key Laboratory of Particle Astrophyics &Experimental Physics Division &Computing Center, Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, China;²University of Chinese Academy of Sciences, Beijing 100049, China;³Tianfu Cosmic Ray Research Center, Chengdu 610000, China;⁴Dublin Institute for Advanced Studies, 31 Fitzwilliam Place, 2 Dublin, Ireland;⁵Max-Planck-Institut for Nuclear Physics, P.O. Box 103980, 69029 Heidelberg, Germany;⁶State Key Laboratory of Particle Detection and Electronics, China;⁷University of Science and Technology of China, Hefei 230026, China;⁸School of Physical Science and Technology &School of Information Science and Technology, Southwest Jiaotong University, Chengdu 610031, China;⁹School of Astronomy and Space Science, Nanjing University, Nanjing 210023, China;¹⁰Center for Astrophysics, Guangzhou University, Guangzhou 510006, China;¹¹Hebei Normal University, Shijiazhuang 050024, China;¹²Key Laboratory of Dark Matter and Space Astronomy &Key Laboratory of Radio Astronomy, Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing 210023, China;¹³Tsung-Dao Lee Institute &School of Physics and Astronomy, Shanghai Jiao Tong University, Shanghai 200240, China;¹⁴Key Laboratory for Research in Galaxies and Cosmology, Shanghai Astronomical Observatory, Chinese Academy of Sciences, Shanghai 200030, China;¹⁵Key Laboratory of Cosmic Rays (Tibet University), Ministry of Education, Lhasa 850000, Tibet, China;¹⁶National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100101, China;¹⁷School of Physics and Astronomy (Zhuhai) &School of Physics (Guangzhou) &Sino-French Institute of Nuclear Engineering and Technology (Zhuhai), Sun Yat-sen University, Zhuhai 519000 &Guangzhou 510275, China;¹⁸School of Physics and Astronomy, Yunnan University, Kunming 650091, China;¹⁹Département de Physique Nucléaire et Corpusculaire, Faculté de Sciences, Université de Genève, 24 Quai Ernest Ansermet, 1211 Geneva, Switzerland;²⁰Institute of Frontier and Interdisciplinary Science, Shandong University, Qingdao 266237, China;²¹APC, Universit'e Paris Cit'e, CNRS/IN2P3, CEA/IRFU, Observatoire de Paris, 119 75205 Paris, France;²²Department of Engineering Physics, Tsinghua University, Beijing 100084, China;²³School of Physics and Microelectronics, Zhengzhou University, Zhengzhou 450001, China;²⁴Yunnan Observatories, Chinese Academy of Sciences, Kunming 650216, China;²⁵College of Physics, Sichuan University, Chengdu 610065, China;²⁶Institute for Nuclear Research of Russian Academy of Sciences, Moscow 117312, Russia;²⁷Moscow Institute of Physics and Technology, Moscow 141700, Russia;²⁸School of Physics, Peking University, Beijing 100871, China;²⁹School of Physical Science and Technology, Guangxi University, Nanning 530004, China;³⁰Department of Physics, Faculty of Science, Mahidol University, Bangkok 10400, Thailand;³¹Center for Relativistic Astrophysics and High Energy Physics, School of Physics and Materials Science &Institute of Space Science and Technology, Nanchang University, Nanchang 330031, China;³²National Space Science Center, Chinese Academy of Sciences, Beijing 100190, China ）
出处： Chinese Physics C 2024 Vol.48 No.6 P065001
摘要： The full array of the Large High Altitude Air Shower Observatory has been in operation since July 2021. For its kilometer-square array , we optimized

期刊

Early warning system for ice collapses and river blockages in the Sedongpu Valley, southeastern Tibetan Plateau Scopus文摘索引数据库(荷)

作者： W. Yang，Z. Wang，B. An，B. An，Y. Chen，C. Zhao，C. Zhao，C. Li，Y. Wang，W. Wang，J. Li，G. Wu，L. Bai，F. Zhang，T. Yao （ ¹State Key Laboratory of Tibetan Plateau Earth System, Environment and Resources (TPESER), Institute of Tibetan Plateau Research, Chinese Academy of Sciences, Beijing 100101, China;²School of Science, Tibet University, Lhasa 850011, China;³College of Earth and Environmental Sciences, Lanzhou University, Lanzhou 730000, China ）
出处： Natural Hazards and Earth System Sciences 2023 Vol.23 P3015-3029
摘要： The Tibetan Plateau and its surroundings have recently experienced several catastrophic glacier-related disasters. It is of great scientific and pract

期刊

Pointing calibration of LHAASO-WFCTA telescopes using bright stars

作者： Zhen Cao，F. Aharonian，Q. An，Axikegu，Y.X. Bai，Y.W. Bao，D. Bastieri，X.J. Bi，Y.J. Bi，J.T. Cai，Q. Cao，W.Y. Cao，Zhe Cao，J. Chang，J.F. Chang，A.M. Chen，E.S. Chen，Liang Chen，Lin Chen，Long Chen，M.J. Chen，M.L. Chen，Q.H. Chen，S.H. Chen，S.Z. Chen，T.L. Chen，Y. Chen，N. Cheng，Y.D. Cheng，M.Y. Cui，S.W. Cui，X.H. Cui，Y.D. Cui，B.Z. Dai，H.L. Dai，Z.G. Dai，Danzengluobu，D. della Volpe，X.Q. Dong，K.K. Duan，J.H. Fan，Y.Z. Fan，J. Fang，K. Fang，C.F. Feng，L. Feng，S.H. Feng，X.T. Feng，Y.L. Feng，S. Gabici，B. Gao，C.D. Gao，L.Q. Gao，Q. Gao，W. Gao，W.K. Gao，M.M. Ge，L.S. Geng，G. Giacinti，G.H. Gong，Q.B. Gou，M.H. Gu，F.L. Guo，X.L. Guo，Y.Q. Guo，Y.Y. Guo，Y.A. Han，H.H. He，H.N. He，J.Y. He，X.B. He，Y. He，M. Heller，Y.K. Hor，B.W. Hou，C. Hou，X. Hou，H.B. Hu，Q. Hu，S.C. Hu，D.H. Huang，T.Q. Huang，W.J. Huang，X.T. Huang，X.Y. Huang，Y. Huang，Z.C. Huang，X.L. Ji，H.Y. Jia，K. Jia，K. Jiang，X.W. Jiang，Z.J. Jiang，M. Jin，M.M. Kang，T. Ke，D. Kuleshov，K. Kurinov，B.B. Li，Cheng Li，Cong Li，D. Li，F. Li，H.B. Li，H.C. Li，H.Y. Li，J. Li，Jian Li，Jie Li，K. Li，W.L. Li，W.L. Li，X.R. Li，Xin Li，Y.Z. Li，Zhe Li，Zhuo Li，E.W. Liang，Y.F. Liang，S.J. Lin，B. Liu，C. Liu，D. Liu，H. Liu，H.D. Liu，J. Liu，J.L. Liu，J.Y. Liu，M.Y. Liu，R.Y. Liu，S.M. Liu，W. Liu，Y. Liu，Y.N. Liu，R. Lu，Q. Luo，H.K. Lv，B.Q. Ma，L.L. Ma，X.H. Ma，J.R. Mao，Z. Min，W. Mitthumsiri，H.J. Mu，Y.C. Nan，A. Neronov，Z.W. Ou，B.Y. Pang，P. Pattarakijwanich，Z.Y. Pei，M.Y. Qi，Y.Q. Qi，B.Q. Qiao，J.J. Qin，D. Ruffolo，A. Sáiz，D. Semikoz，C.Y. Shao，L. Shao，O. Shchegolev，X.D. Sheng，F.W. Shu，H.C. Song，Yu.V. Stenkin，V. Stepanov，Y. Su，Q.N. Sun，X.N. Sun，Z.B. Sun，P.H.T. Tam，Q.W. Tang，Z.B. Tang，W.W. Tian，C. Wang，C.B. Wang，G.W. Wang，H.G. Wang，H.H. Wang，J.C. Wang，K. Wang，L.P. Wang，L.Y. Wang，P.H. Wang，R. Wang，W. Wang，X.G. Wang，X.Y. Wang，Y. Wang，Y.D. Wang，Y.J. Wang，Z.H. Wang，Z.X. Wang，Zhen Wang，Zheng Wang，D.M. Wei，J.J. Wei，Y.J. Wei，T. Wen，C.Y. Wu，H.R. Wu，S. Wu，X.F. Wu，Y.S. Wu，S.Q. Xi，J. Xia，J.J. Xia，G.M. Xiang，D.X. Xiao，G. Xiao，G.G. Xin，Y.L. Xin，Y. Xing，Z. Xiong，D.L. Xu，R.F. Xu，R.X. Xu，W.L. Xu，L. Xue，D.H. Yan，J.Z. Yan，T. Yan，C.W. Yang，F. Yang，F.F. Yang，H.W. Yang，J.Y. Yang，L.L. Yang，M.J. Yang，R.Z. Yang，S.B. Yang，Y.H. Yao，Z.G. Yao，Y.M. Ye，L.Q. Yin，N. Yin，X.H. You，Z.Y. You，Y.H. Yu，Q. Yuan，H. Yue，H.D. Zeng，T.X. Zeng，W. Zeng，M. Zha，B.B. Zhang，F. Zhang，H.M. Zhang，H.Y. Zhang，J.L. Zhang，L.X. Zhang，Li Zhang，P.F. Zhang，P.P. Zhang，R. Zhang，S.B. Zhang，S.R. Zhang，S.S. Zhang，X. Zhang，X.P. Zhang，Y.F. Zhang，Yi Zhang，Yong Zhang，B. Zhao，J. Zhao，L. Zhao，L.Z. Zhao，S.P. Zhao，F. Zheng，B. Zhou，H. Zhou，J.N. Zhou，M. Zhou，P. Zhou，R. Zhou，X.X. Zhou，C.G. Zhu，F.R. Zhu，H. Zhu，K.J. Zhu，X. Zuo，LHAASO Collaboration （ ¹Key Laboratory of Particle Astrophysics & Experimental Physics Division & Computing Center, Institute of High Energy Physics, Chinese Academy of Sciences, 100049 Beijing, China;²University of Chinese Academy of Sciences, 100049 Beijing, China;³TIANFU Cosmic Ray Research Center, Chengdu, Sichuan, China;⁴Dublin Institute for Advanced Studies, 31 Fitzwilliam Place, 2 Dublin, Ireland;⁵Max–Planck-Institute for Nuclear Physics, P.O. Box 103980, 69029 Heidelberg, Germany;⁶State Key Laboratory of Particle Detection and Electronics, China;⁷University of Science and Technology of China, 230026 Hefei, Anhui, China;⁸School of Physical Science and Technology & School of Information Science and Technology, Southwest Jiaotong University, 610031 Chengdu, Sichuan, China;⁹School of Astronomy and Space Science, Nanjing University, 210023 Nanjing, Jiangsu, China;¹⁰Center for Astrophysics, Guangzhou University, 510006 Guangzhou, Guangdong, China;¹¹Hebei Normal University, 050024 Shijiazhuang, Hebei, China;¹²Key Laboratory of Dark Matter and Space Astronomy & Key Laboratory of Radio Astronomy, Purple Mountain Observatory, Chinese Academy of Sciences, 210023 Nanjing, Jiangsu, China;¹³Tsung-Dao Lee Institute & School of Physics and Astronomy, Shanghai Jiao Tong University, 200240 Shanghai, China;¹⁴Key Laboratory for Research in Galaxies and Cosmology, Shanghai Astronomical Observatory, Chinese Academy of Sciences, 200030 Shanghai, China;¹⁵Key Laboratory of Cosmic Rays (Tibet University), Ministry of Education, 850000 Lhasa, Tibet, China;¹⁶National Astronomical Observatories, Chinese Academy of Sciences, 100101 Beijing, China;¹⁷School of Physics and Astronomy (Zhuhai) & School of Physics (Guangzhou) & Sino-French Institute of Nuclear Engineering and Technology (Zhuhai), Sun Yat-sen University, 519000 Zhuhai & 510275 Guangzhou, Guangdong, China;¹⁸School of Physics and Astronomy, Yunnan University, 650091 Kunming, Yunnan, China;¹⁹Département de Physique Nucléaire et Corpusculaire, Faculté de Sciences, Université de Genève, 24 Quai Ernest Ansermet, 1211 Geneva, Switzerland;²⁰Institute of Frontier and Interdisciplinary Science, Shandong University, 266237 Qingdao, Shandong, China;²¹APC, Université Paris Cité, CNRS/IN2P3, CEA/IRFU, Observatoire de Paris, 119 75205 Paris, France;²²Department of Engineering Physics, Tsinghua University, 100084 Beijing, China;²³School of Physics and Microelectronics, Zhengzhou University, 450001 Zhengzhou, Henan, China;²⁴Yunnan Observatories, Chinese Academy of Sciences, 650216 Kunming, Yunnan, China;²⁵College of Physics, Sichuan University, 610065 Chengdu, Sichuan, China;²⁶Institute for Nuclear Research of Russian Academy of Sciences, 117312 Moscow, Russia;²⁷School of Physics, Peking University, 100871 Beijing, China;²⁸School of Physical Science and Technology, Guangxi University, 530004 Nanning, Guangxi, China;²⁹Department of Physics, Faculty of Science, Mahidol University, Bangkok 10400, Thailand;³⁰Moscow Institute of Physics and Technology, 141700 Moscow, Russia;³¹Center for Relativistic Astrophysics and High Energy Physics, School of Physics and Materials Science & Institute of Space Science and Technology, Nanchang University, 330031 Nanchang, Jiangxi, China;³²National Space Science Center, Chinese Academy of Sciences, 100190 Beijing, China ）
出处： Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment 2023 Vol.1056 P168662
摘要： One of the main scientific objectives of the Large High Altitude Air Shower Observatory is to perform accurate measurements of the energy spectra for
点击量：2

期刊

A tera-electron volt afterglow from a narrow jet in an extremely bright gamma-ray burst Scopus文摘索引数据库(荷)

作者： Cao,Zhen，Aharonian,F.，An,Q.，Axikegu，Bai,L.X.，Bai,Y.X.，Bao,Y.W.，Bastieri,D.，Bi,X.J.，Bi,Y.J.，Cai,J.T.，Cao,Q.，Cao,W.Y.，Cao,Zhe，Chang,J.，Chang,J.F.，Chen,E.S.，Chen,Liang，Chen,Lin，Chen,Long，Chen,M.J.，Chen,M.L.，Chen,Q.H.，Chen,S.H.，Chen,S.Z.，Chen,T.L.，Chen,Y.，Cheng,H.L.，Cheng,N.，Cheng,Y.D.，Cui,S.W.，Cui,X.H.，Cui,Y.D.，Dai,B.Z.，Dai,H.L.，Dai,Z.G.，Danzengluobu，Della Volpe,D.，Dong,X.Q.，Duan,K.K.，Fan,J.H.，Fan,Y.Z.，Fang,J.，Fang,K.，Feng,C.F.，Feng,L.，Feng,S.H.，Feng,X.T.，Feng,Y.L.，Gao,B.，Gao,C.D.，Gao,L.Q.，Gao,Q.，Gao,W.，Gao,W.K.，Ge,M.M.，Geng,L.S.，Gong,G.H.，Gou,Q.B.，Gu,M.H.，Guo,F.L.，Guo,X.L.，Guo,Y.Q.，Guo,Y.Y.，Han,Y.A.，He,H.H.，He,H.N.，He,J.Y.，He,X.B.，He,Y.，Heller,M.，Hor,Y.K.，Hou,B.W.，Hou,C.，Hou,X.，Hu,H.B.，Hu,Q.，Hu,S.C.，Huang,D.H.，Huang,T.Q.，Huang,W.J.，Huang,X.T.，Huang,X.Y.，Huang,Y.，Huang,Z.C.，Ji,X.L.，Jia,H.Y.，Jia,K.，Jiang,K.，Jiang,X.W.，Jiang,Z.J.，Jin,M.，Kang,M.M.，Ke,T.，Kuleshov,D.，Kurinov,K.，Li,B.B.，Li,Cheng，Li,Cong，Li,D.，Li,F.，Li,H.B.，Li,H.C.，Li,H.Y.，Li,J.，Li,Jian，Li,Jie，Li,K.，Li,W.L.，Li,W.L.，Li,X.R.，Li,Xin，Li,Y.Z.，Li,Zhe，Li,Zhuo，Liang,E.W.，Liang,Y.F.，Lin,S.J.，Liu,B.，Liu,C.，Liu,D.，Liu,H.，Liu,H.D.，Liu,J.，Liu,J.L.，Liu,J.L.，Liu,J.S.，Liu,J.Y.，Liu,M.Y.，Liu,R.Y.，Liu,S.M.，Liu,W.，Liu,Y.，Liu,Y.N.，Long,W.J.，Lu,R.，Luo,Q.，Lv,H.K.，Ma,B.Q.，Ma,L.L.，Ma,X.H.，Mao,J.R.，Min,Z.，Mitthumsiri,W.，Nan,Y.C.，Ou,Z.W.，Pang,B.Y.，Pattarakijwanich,P.，Pei,Z.Y.，Qi,M.Y.，Qi,Y.Q.，Qiao,B.Q.，Qin,J.J.，Ruffolo,D.，Sáiz,A.，Shao,C.Y.，Shao,L.，Shchegolev,O.，Sheng,X.D.，Song,H.C.，Stenkin,Y.V.，Stepanov,V.，Su,Y.，Sun,Q.N.，Sun,X.N.，Sun,Z.B.，Tam,P.H.T.，Tang,Z.B.，Tian,W.W.，Wang,C.，Wang,C.B.，Wang,G.W.，Wang,H.G.，Wang,H.H.，Wang,J.C.，Wang,J.S.，Wang,K.，Wang,L.P.，Wang,L.Y.，Wang,P.H.，Wang,R.，Wang,W.，Wang,X.G.，Wang,X.Y.，Wang,Y.，Wang,Y.D.，Wang,Y.J.，Wang,Z.H.，Wang,Z.X.，Wang,Zhen，Wang,Zheng，Wei,D.M.，Wei,J.J.，Wei,Y.J.，Wen,T.，Wu,C.Y.，Wu,H.R.，Wu,S.，Wu,X.F.，Wu,Y.S.，Xi,S.Q.，Xia,J.，Xia,J.J.，Xiang,G.M.，Xiao,D.X.，Xiao,G.，Xin,G.G.，Xin,Y.L.，Xing,Y.，Xiong,Z.，Xu,D.L.，Xu,R.F.，Xu,R.X.，Xue,L.，Yan,D.H.，Yan,J.Z.，Yan,T.，Yang,C.W.，Yang,F.，Yang,F.F.，Yang,H.W.，Yang,J.Y.，Yang,L.L.，Yang,M.J.，Yang,R.Z.，Yang,S.B.，Yao,Y.H.，Yao,Z.G.，Ye,Y.M.，Yin,L.Q.，Yin,N.，You,X.H.，You,Z.Y.，Yu,Y.H.，Yuan,Q.，Yue,H.，Zeng,H.D.，Zeng,T.X.，Zeng,W.，Zeng,Z.K.，Zha,M.，Zhang,B.，Zhang,B.B.，Zhang,F.，Zhang,H.M.，Zhang,H.Y.，Zhang,J.L.，Zhang,L.X.，Zhang,L.，Zhang,P.F.，Zhang,P.P.，Zhang,R.，Zhang,S.B.，Zhang,S.R.，Zhang,S.S.，Zhang,X.，Zhang,X.P.，Zhang,Y.F.，Zhang,Y.，Zhang,Yong，Zhao,B.，Zhao,J.，Zhao,L.，Zhao,L.Z.，Zhao,S.P.，Zheng,F.，Zheng,J.H.，Zhou,B.，Zhou,H.，Zhou,J.N.，Zhou,P.，Zhou,R.，Zhou,X.X.，Zhu,C.G.，Zhu,F.R.，Zhu,H.，Zhu,K.J.，Zuo,X. （ ¹Key Laboratory of Particle Astrophysics & Experimental Physics Division & Computing Center, Institute of High Energy Physics, Chinese Academy of Sciences, 100049, Beijing, China;²University of Chinese Academy of Sciences, 100049, Beijing, China;³Tianfu Cosmic Ray Research Center, Chengdu, 610000, Sichuan, China;⁴Dublin Institute for Advanced Studies, 31 Fitzwilliam Place, 2 Dublin, Ireland;⁵Max-Planck-Institute for Nuclear Physics, P.O. Box 103980, Heidelberg, 69029, Germany;⁶State Key Laboratory of Particle Detection and Electronics, China;⁷University of Science and Technology of China, Hefei, 230026, Anhui, China;⁸School of Physical Science and Technology & School of Information Science and Technology, Southwest Jiaotong University, Chengdu, 610031, Sichuan, China;⁹College of Physics, Sichuan University, Chengdu, 610065, Sichuan, China;¹⁰School of Astronomy and Space Science, Nanjing University, Nanjing, 210023, Jiangsu, China;¹¹Key Laboratory of Modern Astronomy and Astrophysics (Nanjing University), Ministry of Education, Nanjing, 210023, China;¹²Center for Astrophysics, Guangzhou University, Guangzhou, 510006, Guangdong, China;¹³Hebei Normal University, Shijiazhuang, 050024, Hebei, China;¹⁴Key Laboratory of Dark Matter and Space Astronomy & Key Laboratory of Radio Astronomy, Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing, 210023, Jiangsu, China;¹⁵Key Laboratory for Research in Galaxies and Cosmology, Shanghai Astronomical Observatory, Chinese Academy of Sciences, 200030, Shanghai, China;¹⁶Key Laboratory of Cosmic Rays (Tibet University), Ministry of Education, Lhasa, 850000, Tibet, China;¹⁷National Astronomical Observatories, Chinese Academy of Sciences, 100101, Beijing, China;¹⁸School of Physics and Astronomy (Zhuhai) & School of Physics (Guangzhou) & Sino-French Institute of Nuclear Engineering and Technology (Zhuhai), Sun Yat-sen University, Guangdong, China;¹⁹School of Physics and Astronomy, Yunnan University, Kunming, 650091, Yunnan, China;²⁰Département de Physique Nucléaire et Corpusculaire, Faculté de Sciences, Université de Genève, 24 Quai Ernest Ansermet, 1211, Geneva, Switzerland;²¹Institute of Frontier and Interdisciplinary Science, Shandong University, Qingdao, 266237, Shandong, China;²²Department of Engineering Physics, Tsinghua University, 100084, Beijing, China;²³School of Physics and Microelectronics, Zhengzhou University, Zhengzhou, 450001, Henan, China;²⁴Yunnan Observatories, Chinese Academy of Sciences, Kunming, 650216, Yunnan, China;²⁵Institute for Nuclear Research of Russian Academy of Sciences, 117312, Moscow, Russian Federation;²⁶Moscow Institute of Physics and Technology, 141700, Moscow, Russian Federation;²⁷Shanghai Jiao Tong University, Tsung-Dao Lee Institute & School of Physics and Astronomy, 200240, Shanghai, China;²⁸School of Physics, Peking University, 100871, Beijing, China;²⁹School of Physical Science and Technology, Guangxi University, Nanning, 530004, Guangxi, China;³⁰Department of Physics, Faculty of Science, Mahidol University, 10400, Bangkok, Thailand;³¹Chinese Academy of Sciences, National Space Science Center, 100190, Beijing, China;³²Nevada Center for Astrophysics, University of Nevada, Las Vegas, United States;³³Department of Physics and Astronomy, University of Nevada, Las Vegas, United States; ）
出处： Science (New York, N.Y.) 2023 Vol.380 No.6652 P1390-1396
摘要： Some gamma-ray bursts have a tera-electron volt afterglow, but the early onset of this has not been observed. We report observations with the Large
点击量：5

期刊

An ultrahigh-energy γ -ray bubble powered by a super PeVatron EI工程索引(美)

作者： Z. Cao，F. Aharonian，Q An，Axikegu，Y.X Bai，Y.W Bao，D Bastieri，X.J Bi，Y.J Bi，J.T Cai，Q Cao，W.Y Cao，Zhe Cao，J Chang，J.F Chang，A.M Chen，E.S Chen，Liang Chen，Lin Chen，Long Chen，M.J Chen，M.L Chen，Q.H Chen，S.H Chen，S.Z Chen，T.L Chen，Y Chen，N Cheng，Y.D Cheng，M.Y Cui，S.W Cui，X.H Cui，Y.D Cui，B.Z Dai，H.L Dai，Z.G Dai，Danzengluobu，D della Volpe，X.Q Dong，K.K Duan，J.H Fan，Y.Z Fan，J Fang，K Fang，C.F Feng，L Feng，S.H Feng，X.T Feng，Y.L Feng，S Gabici，B Gao，C.D Gao，L.Q Gao，Q Gao，W Gao，W.K Gao，M.M Ge，L.S Geng，G Giacinti，G.H Gong，Q.B Gou，M.H Gu，F.L Guo，X.L Guo，Y.Q Guo，Y.Y Guo，Y.A Han，H.H He，H.N He，J.Y He，X.B He，Y He，M Heller，Y.K Hor，B.W Hou，C Hou，X Hou，H.B Hu，Q Hu，S.C Hu，D.H Huang，T.Q Huang，W.J Huang，X.T Huang，X.Y Huang，Y Huang，Z.C Huang，X.L Ji，H.Y Jia，K Jia，K Jiang，X.W Jiang，Z.J Jiang，M Jin，M.M Kang，T Ke，D Kuleshov，K Kurinov，B.B Li，Cheng Li，Cong Li，D Li，F Li，H.B Li，H.C Li，H.Y Li，J Li，Jian Li，Jie Li，K Li，W.L Li，W.L Li，X.R Li，Xin Li，Y.Z Li，Zhe Li，Zhuo Li，E.W Liang，Y.F Liang，S.J Lin，B Liu，C Liu，D Liu，H Liu，H.D Liu，J Liu，J.L Liu，J.Y Liu，M.Y Liu，R.Y Liu，S.M Liu，W Liu，Y Liu，Y.N Liu，R Lu，Q Luo，H.K Lv，B.Q Ma，L.L Ma，X.H Ma，J.R Mao，Z Min，W Mitthumsiri，H.J Mu，Y.C Nan，A Neronov，Z.W Ou，B.Y Pang，P Pattarakijwanich，Z.Y Pei，M.Y Qi，Y.Q Qi，B.Q Qiao，J.J Qin，D Ruffolo，A Sáiz，D Semikoz，C.Y Shao，L Shao，O Shchegolev，X.D Sheng，F.W Shu，H.C Song，Yu.V Stenkin，V Stepanov，Y Su，Q.N Sun，X.N Sun，Z.B Sun，P.H.T Tam，Q.W Tang，Z.B Tang，W.W Tian，C Wang，C.B Wang，G.W Wang，H.G Wang，H.H Wang，J.C Wang，K Wang，L.P Wang，L.Y Wang，P.H Wang，R Wang，W Wang，X.G Wang，X.Y Wang，Y Wang，Y.D Wang，Y.J Wang，Z.H Wang，Z.X Wang，Zhen Wang，Zheng Wang，D.M Wei，J.J Wei，Y.J Wei，T Wen，C.Y Wu，H.R Wu，S Wu，X.F Wu，Y.S Wu，S.Q Xi，J Xia，J.J Xia，G.M Xiang，D.X Xiao，G Xiao，G.G Xin，Y.L Xin，Y Xing，Z Xiong，D.L Xu，R.F Xu，R.X Xu，W.L Xu，L Xue，D.H Yan，J.Z Yan，T Yan，C.W Yang，F Yang，F.F Yang，H.W Yang，J.Y Yang，L.L Yang，M.J Yang，R.Z Yang，S.B Yang，Y.H Yao，Z.G Yao，Y.M Ye，L.Q Yin，N Yin，X.H You，Z.Y You，Y.H Yu，Q Yuan，H Yue，H.D Zeng，T.X Zeng，W Zeng，M Zha，B.B Zhang，F Zhang，H.M Zhang，H.Y Zhang，J.L Zhang，L.X Zhang，Li Zhang，P.F Zhang，P.P Zhang，R Zhang，S.B Zhang，S.R Zhang，S.S Zhang，X Zhang，X.P Zhang，Y.F Zhang，Yi Zhang，Yong Zhang，B Zhao，J Zhao，L Zhao，L.Z Zhao，S.P Zhao，F Zheng，B Zhou，H Zhou，J.N Zhou，M Zhou，P Zhou，R Zhou，X.X Zhou，C.G Zhu，F.R Zhu，H Zhu，K.J Zhu，X Zuo （ ¹Key Laboratory of Particle Astrophyics & Experimental Physics Division & Computing Center, Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, China;²University of Chinese Academy of Sciences, Beijing 100049, China;³TIANFU Cosmic Ray Research Center, Chengdu 610000, China;⁴Dublin Institute for Advanced Studies, 31 Fitzwilliam Place, 2 Dublin, Ireland;⁵Max-Planck-Institut for Nuclear Physics, Heidelberg 69026, Germany;⁶State Key Laboratory of Particle Detection and Electronics, China;⁷University of Science and Technology of China, Hefei 230026, China;⁸School of Physical Science and Technology, School of Information Science and Technology, Southwest Jiaotong University, Chengdu 610031, China;⁹School of Astronomy and Space Science, Nanjing University, Nanjing 210023, China;¹⁰Center for Astrophysics, Guangzhou University, Guangzhou 510006, China;¹¹Hebei Normal University, Shijiazhuang 050024, China;¹²Key Laboratory of Dark Matter and Space Astronomy, Key Laboratory of Radio Astronomy, Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing 210023, China;¹³Tsung-Dao Lee Institute, School of Physics and Astronomy, Shanghai Jiao Tong University, Shanghai 200240, China;¹⁴Key Laboratory for Research in Galaxies and Cosmology, Shanghai Astronomical Observatory, Chinese Academy of Sciences, Shanghai 200030, China;¹⁵Key Laboratory of Cosmic Rays (Tibet University), Ministry of Education, Lhasa 850000, China;¹⁶National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100101, China;¹⁷School of Physics and Astronomy (Zhuhai), School of Physics (Guangzhou) & Sino-French Institute of Nuclear Engineering and Technology (Zhuhai), Sun Yat-sen University, Zhuhai 519000 & Guangzhou 510275, China;¹⁸School of Physics and Astronomy, Yunnan University, Kunming 650091, China;¹⁹Département de Physique Nucléaire et Corpusculaire, Faculté de Sciences, Université de Genève, 24 Quai Ernest Ansermet, 1211 Geneva, Switzerland;²⁰Institute of Frontier and Interdisciplinary Science, Shandong University, Qingdao 266237, China;²¹APC, Universit’e Paris Cit’e, CNRS/IN2P3, CEA/IRFU, Observatoire de Paris, Paris 119 75205, France;²²Department of Engineering Physics, Tsinghua University, Beijing 100084, China;²³School of Physics and Microelectronics, Zhengzhou University, Zhengzhou 450001, China;²⁴Yunnan Observatories, Chinese Academy of Sciences, Kunming 650216, China;²⁵College of Physics, Sichuan University, Chengdu 610065, China;²⁶Institute for Nuclear Research of Russian Academy of Sciences, Moscow 117312, Russia;²⁷Moscow Institute of Physics and Technology, Moscow 141700, Russia;²⁸School of Physics, Peking University, Beijing 100871 China;²⁹School of Physical Science and Technology, Guangxi University, Nanning 530004, China;³⁰Department of Physics, Faculty of Science, Mahidol University, Bangkok 10400, Thailand;³¹Center for Relativistic Astrophysics and High Energy Physics, School of Physics and Materials Science, Institute of Space Science and Technology, Nanchang University, Nanchang 330031, China;³²National Space Science Center, Chinese Academy of Sciences, Beijing 100190, China ）
出处： Science Bulletin 2023
摘要： We report the detection of a γ -ray bubble spanning at least 100 deg 2 in ultra high energy up to a few PeV in the direction of the star-forming regi

期刊

Constraints on Heavy Decaying Dark Matter from 570 Days of LHAASO Observations EI工程索引(美)

作者： Zhen Cao, F Aharonian, Q An, Axikegu, L X Bai, Y X Bai, Y W Bao, D Bastieri, X J Bi, Y J Bi, J T Cai, Zhe Cao, J Chang, J F Chang, E S Chen, Liang Chen, Liang Chen, Long Chen, M J Chen, M L Chen, Q H Chen, S H Chen, S Z Chen, T L Chen, Y Chen, H L Cheng, N Cheng, Y D Cheng, S W Cui, X H Cui, Y D Cui, B D'Ettorre Piazzoli, B Z Dai, H L Dai, Z G Dai, Danzengluobu, D Della Volpe, K K Duan, J H Fan, Y Z Fan, Z X Fan, J Fang, K Fang, C F Feng, L Feng, S H Feng, X T Feng, Y L Feng, B Gao, C D Gao, L Q Gao, Q Gao, W Gao, W K Gao, M M Ge, L S Geng, G H Gong, Q B Gou, M H Gu, F L Guo, J G Guo, X L Guo, Y Q Guo, Y Y Guo, Y A Han, H H He, H N He, S L He, X B He, Y He, M Heller, Y K Hor, C Hou, X Hou, H B Hu, Q Hu, S Hu, S C Hu, X J Hu, D H Huang, W H Huang, X T Huang, X Y Huang, Y Huang, Z C Huang, X L Ji, H Y Jia, K Jia, K Jiang, Z J Jiang, M Jin, M M Kang, T Ke, D Kuleshov, K Levochkin, B B Li, Cheng Li, Cong Li, F Li, H B Li, H C Li, H Y Li, J Li, Jian Li, Jie Li, K Li, W L Li, X R Li, Xin Li, Xin Li, Y Z Li, Zhe Li, Zhuo Li, E W Liang, Y F Liang, S J Lin, B Liu, C Liu, D Liu, H Liu, H D Liu, J Liu, J L Liu, J S Liu, J Y Liu, M Y Liu, R Y Liu, S M Liu, W Liu, Y Liu, Y N Liu, W J Long, R Lu, Q Luo, H K Lv, B Q Ma, L L Ma, X H Ma, J R Mao, A Masood, Z Min, W Mitthumsiri, Y C Nan, Z W Ou, B Y Pang, P Pattarakijwanich, Z Y Pei, M Y Qi, Y Q Qi, B Q Qiao, J J Qin, D Ruffolo, A Sáiz, C Y Shao, L Shao, O Shchegolev, X D Sheng, J Y Shi, H C Song, Yu V Stenkin, V Stepanov, Y Su, Q N Sun, X N Sun, Z B Sun, P H T Tam, Z B Tang, W W Tian, B D Wang, C Wang, H Wang, H G Wang, J C Wang, J S Wang, L P Wang, L Y Wang, R Wang, R N Wang, W Wang, X G Wang, X Y Wang, Y Wang, Y D Wang, Y J Wang, Y P Wang, Z H Wang, Z X Wang, Zhen Wang, Zheng Wang, D M Wei, J J Wei, Y J Wei, T Wen, C Y Wu, H R Wu, S Wu, X F Wu, Y S Wu, S Q Xi, J Xia, J J Xia, G M Xiang, D X Xiao, G Xiao, G G Xin, Y L Xin, Y Xing, Z Xiong, D L Xu, R X Xu, L Xue, D H Yan, J Z Yan, C W Yang, F F Yang, H W Yang, J Y Yang, L L Yang, M J Yang, R Z Yang, S B Yang, Y H Yao, Z G Yao, Y M Ye, L Q Yin, N Yin, X H You, Z Y You, Y H Yu, Q Yuan, H Yue, H D Zeng, T X Zeng, W Zeng, Z K Zeng, M Zha, X X Zhai, B B Zhang, F Zhang, H M Zhang, H Y Zhang, J L Zhang, L X Zhang, Li Zhang, Lu Zhang, P F Zhang, P P Zhang, R Zhang, S B Zhang, S R Zhang, S S Zhang, X Zhang, X P Zhang, Y F Zhang, Y L Zhang, Yi Zhang, Yong Zhang, B Zhao, J Zhao, L Zhao, L Z Zhao, S P Zhao, F Zheng, Y Zheng, B Zhou, H Zhou, J N Zhou, P Zhou, R Zhou, X X Zhou, C G Zhu, F R Zhu, H Zhu, K J Zhu, X Zuo, S Ando, M Chianese, D F G Fiorillo, G Miele, K C Y Ng， LHAASO Collaboration （ Affiliations ¹ Key Laboratory of Particle Astrophyics 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, 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, 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 Key Laboratory of Dark Matter and Space Astronomy, Purple Mountain Observatory, Chinese Academy of Sciences, 210023 Nanjing, Jiangsu, China. ¹³ Key Laboratory for Research in Galaxies and Cosmology, Shanghai Astronomical Observatory, Chinese Academy of Sciences, 200030 Shanghai, China. ¹⁴ Key Laboratory of Cosmic Rays (Tibet University), Ministry of Education, 850000 Lhasa, Tibet, China. ¹⁵ National Astronomical Observatories, Chinese Academy of Sciences, 100101 Beijing, China. ¹⁶ Hebei Normal University, 050024 Shijiazhuang, Hebei, China. ¹⁷ 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 & 510275 Guangzhou, Guangdong, China. ¹⁸ Dipartimento di Fisica dell'Università di Napoli "Federico II," Complesso Universitario di Monte Sant'Angelo, via Cinthia, 80126 Napoli, Italy. ¹⁹ School of Physics and Astronomy, Yunnan University, 650091 Kunming, Yunnan, China. ²⁰ Département de Physique Nucléaire et Corpusculaire, Faculté de Sciences, Université de Genève, 24 Quai Ernest Ansermet, 1211 Geneva, Switzerland. ²¹ Institute of Frontier and Interdisciplinary Science, Shandong University, 266237 Qingdao, Shandong, China. ²² Department of Engineering Physics, Tsinghua University, 100084 Beijing, China. ²³ School of Physics and Microelectronics, Zhengzhou University, 450001 Zhengzhou, Henan, China. ²⁴ Yunnan Observatories, Chinese Academy of Sciences, 650216 Kunming, Yunnan, China. ²⁵ Institute for Nuclear Research of Russian Academy of Sciences, 117312 Moscow, Russia. ²⁶ School of Physics, Peking University, 100871 Beijing, China. ²⁷ School of Physical Science and Technology, Guangxi University, 530004 Nanning, Guangxi, China. ²⁸ Tsung-Dao Lee Institute & School of Physics and Astronomy, Shanghai Jiao Tong University, 200240 Shanghai, China. ²⁹ Department of Physics, Faculty of Science, Mahidol University, Bangkok 10400, Thailand. ³⁰ Moscow Institute of Physics and Technology, 141700 Moscow, Russia. ³¹ National Space Science Center, Chinese Academy of Sciences, 100190 Beijing, China. ³² GRAPPA Institute, University of Amsterdam, 1098 XH Amsterdam, The Netherlands. ³³ Kavli Institute for the Physics and Mathematics of the Universe (KavliIPMU,WPI), University of Tokyo, Kashiwa, Chiba 277-8583, Japan. ³⁴ Dipartimento di Fisica "Ettore Pancini," Università degli studi di Napoli "Federico II", Complesso Univ. Monte S. Angelo, I-80126 Napoli, Italy. ³⁵ INFN - Sezione di Napoli, Complesso Univ. Monte S. Angelo, I-80126 Napoli, Italy. ³⁶ Niels Bohr International Academy, Niels Bohr Institute, University of Copenhagen, Copenhagen, Denmark. ³⁷ Scuola Superiore Meridionale, Università degli studi di Napoli "Federico II", Largo San Marcellino 10, 80138 Napoli, Italy. ³⁸ Department of Physics, The Chinese University of Hong Kong, Shatin, New Territories, Hong Kong, China. ）
出处： Physical review letters 2022 Vol.129 No.26 P261103
关键词： LIMITS NEUTRINOS SEARCH RAYS
摘要： The kilometer square array of the large high altitude air shower observatory aims at surveying the northern γ-ray sky at energies above 10 TeV with

期刊

建国后十七年西藏文学书写的中华认同研究

作者：李军（西藏大学文学院）
出处：西藏科技 2021 第2期
点击量：1

期刊

清代至民国西藏文学书写中的中华文化认同研究

作者：李军（西藏大学文学院）
出处：西藏大学学报(社会科学版) 2021 第36卷第1期 P80-85
关键词：中华文化认同西藏文学交往交流
摘要：文章研究了清代至民国西藏文学书写中的中华文化认同之路。清代西藏贵族代表文学书写体现的'神话情结''八思巴情结''文殊情结''唐朝公主情结'表现出中华文化认同的明显特征。民国间文学书写中的中华认同呈现两种态势:贵族精英的认同表现为弥足珍贵的坚定,平民文学书写呈现构建未来的准备特征。这些文学是西藏地方在

期刊

Line-of-shower triggermethod to lower energy threshold for GRB detection using LHAASO-WCDA

作者： Aharonian F，An Q，Axikegu，Bai LX，Bai YX，Bao YW，Bastieri D，Bi XJ，Bi YJ，Cai H，Cai JT，Cao Z，Cao Z，Chang J，Chang JF，Chang XC，Chen BM，Chen J，Chen L，Chen L，Chen L，Chen MJ，Chen ML，Chen QH，Chen SH，Chen SZ，Chen TL，Chen XL，Chen Y，Cheng N，Cheng YD，Cui SW，Cui XH，Cui YD，Dai BZ，Dai HL，Dai ZG，Danzengluobu，della Volpe D，D'Ettorre Piazzoli B，Dong XJ，Fan JH，Fan YZ，Fan ZX，Fang J，Fang K，Feng CF，Feng L，Feng SH，Feng YL，Gao B，Gao CD，Gao Q，Gao W，Ge MM，Geng LS，Gong GH，Gou QB，Gu MH，Guo JG，Guo XL，Guo YQ，Guo YY，Han YA，He HH，He HN，He JC，He SL，He XB，He Y，Heller M，HoRYK，Hou C，Hou X，Hu HB，Hu S，Hu SC，Hu XJ，Huang DH，Huang QL，Huang WH，Huang XT，Huang ZC，Ji F，Ji XL，Jia HY，Jiang K，Jiang ZJ，Jin C，Kuleshov D，Levochkin K，Li BB，Li C，Li C，Li F，Li HB，Li HC，Li HY，Li J，Li K，Li WL，Li X，Li X，Li XR，Li Y，Li YZ，Li Z，Li Z，Liang EW，Liang YF，Lin SJ，Liu B，Liu C，Liu D，Liu H，Liu HD，Liu J，Liu JL，Liu JS，Liu JY，Liu MY，Liu RY，Liu SM，Liu W，Liu YN，Liu ZX，Long W J （ Dublin Institute for Advanced Studies；Max-Planck-Institut for Nuclear Physics，Germany；State Key Laboratory of Particle Detection and Electronics，State Key Laboratory of Particle Detection and Electronics；University of Science and Technology of China，Anhui；School of Physical Science and Technology & School of Information Science and Technology，Southwest Jiaotong University；College of Physics，Sichuan University；Experimental Physics Division & Computing Center，Institute of High Energy Physics，Chinese Academy of Sciences，Key Laboratory of Particle Astrophysics，Chinese Academy of Sciences；TIANFU Cosmic Ray Research Center；School of Astronomy and Space Science，Nanjing University；Center for Astrophysics，Guangzhou University；University of Chinese Academy of Sciences；School of Physics and Technology，Wuhan University；Purple Mountain Observatory，Chinese Academy of Sciences，Key Laboratory of Dark Matter and Space Astronomy，Chinese Academy of Sciences；Hebei Normal University，Hebei；Shanghai Astronomical Observatory，Chinese Academy of Sciences，Key Laboratory for Research in Galaxies and Cosmology，Chinese Academy of Sciences；Tibet University，Key Laboratory of Cosmic Rays，Ministry of Education；National Astronomical Observatories，Chinese Academy of Sciences；School of Physics and Astronomy & School of Physics (Guangzhou)，Sun Yat-sen University；School of Physics and Astronomy，Yunnan University；Departement de Physique Nucleaire et Corpusculaire，Faculte de Sciences，Universite de Geneve；Dipartimento di Fisica dell'Universita di Napoli “Federico II”，Complesso Universitario di Monte Sant'Angelo，via Cinthia；Institute of Frontier and Interdisciplinary Science，Shandong University；Department of Engineering Physics，Tsinghua University；School of Physics and Microelectronics，Zhengzhou University；Yunnan Observatories，Chinese Academy of Sciences；Institute for Nuclear Research of Russian Academy of Sciences，Russia；School of Physics，Peking University；School of Physical Science and Technology，Guangxi University；Tsung-Dao Lee Institute & School of Physics and Astronomy，Shanghai Jiao Tong University ）
出处： Radiation Detection Technology and Methods 2021 第5卷第4期 P531-541
关键词： LHAASO WCDA GRB
摘要： Purpose Observation of high energy and very high emission from Gamma Ray Bursts is crucial to study the gigantic explosion and the underline processe

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