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期刊文章列表

  • 李和意1,2,张仁友1,2,马文淦1,2,蒋一1,2,李晓周1,2(State Key Laboratory of Particle Detection and Electronics, University of Science and Technology of China;Department of Modern Physics, University of Science and Technology of China).e+e-γ production at photon-photon colliders at complete electroweak NLO accuracy[J].中国物理C(英文版),2022,第4期
  • 韦斯纳,冯兆庆(School of Physics and Optoelectronics, South China University of Technology).Dark matter with chiral symmetry admixed with hadronic matter in compact stars[J].中国物理C(英文版),2022,第4期
  • 王同征1,钱卫良2,3,4,Juan Fernando Zapata Zapata2,林恺1(Hubei Subsurface Multi-scale Imaging Key Laboratory, Institute of Geophysics and Geomatics,China University of Geosciences;Escola de Engenharia de Lorena, Universidade de S?o Paulo;Faculdade de Engenharia de Guaratinguetá, Universidade Estadual Paulista;Center for Gravitation and Cosmology, College of Physical Science and Technology, Yangzhou University).Scalar and Dirac quasinormal modes of scalar-tensor-Gauss-Bonnet black holes[J].中国物理C(英文版),2022,第4期
  • Kumar Nilanjana,Nomura Takaaki,Okada Hiroshi.A multi-charged particle model with local U(1)_(mu-tau) to explain muon g-2, flavor physics, and possible collider signature[J].中国物理(C),2022,第4期
  • H.G.Ganev(Joint Institute for Nuclear Research).Proton-neutron symplectic model description of 20Ne[J].中国物理C(英文版),2022,第4期
  • V.Dehghani1,S.A.Alavi1,R.Razavi2,A.Soylu3,F.Koyuncu4(Department of Physics, University of Sistan and Baluchestan;Physics Department, Faculty of Science, Imam Hossein Comprehensive University;Department of Physics, Nigde ?mer Halisdemir University;Program of Opticianry, G?lhisar Vocational School of Health Services, Burdur Mehmet Akif Ersoy University).Cluster decay half-lives using asymmetry dependent densities[J].中国物理C(英文版),2022,第4期
  • Jie Ren,Xichao Ruan,Wei Jiang,Jie Bao,Jincheng Wang,Qiwei Zhang,Guangyuan Luan,Hanxiong Huang,Yangbo Nie,Zhigang Ge,Qi An,Huaiyong Bai,Yu Bao,Ping Cao,Haolei Chen,Qiping Chen,Yonghao Chen,Yukai Chen,Zhen Chen,Zengqi Cui,Ruirui Fan,Changqing Feng,Keqing Gao,Minhao Gu,Changcai Han,Zijie Han,Guozhu He,Yongcheng He,Yang Hong,Weiling Huang,Xiru Huang,Xiaolu Ji,Xuyang Ji,Haoyu Jiang,Zhijie Jiang,Hantao Jing,Ling Kang,Mingtao Kang,Bo Li,Chao Li,Jiawen Li,Lun Li,Qiang Li,Xiao Li,Yang Li,Rong Liu,Shubin Liu,Xingyan Liu,Qili Mu,Changjun Ning,Binbin Qi,Zhizhou Ren,Yingpeng Song,Zhaohui Song,Hong Sun,Kang Sun,Xiaoyang Sun,Zhijia Sun,Zhixin Tan,Hongqing Tang,Jingyu Tang,Xinyi Tang,Binbin Tian,Lijiao Wang,Pengcheng Wang,Qi Wang,Taofeng Wang,Zhaohui Wang,Jie Wen,Zhongwei Wen,Qingbiao Wu,Xiaoguang Wu,Xuan Wu,Likun Xie,Yiwei Yang,Han Yi,Li Yu,Tao Yu,Yongji Yu,Guohui Zhang,Linhao Zhang,Xianpeng Zhang,Yuliang Zhang,Zhiyong Zhang,Yubin Zhao,Luping Zhou,Zuying Zhou,Danyang Zhu,Kejun Zhu,Peng Zhu,The CSNS Back-n Collaboration(Key Laboratory of Nuclear Data,China Institute of Atomic Energy,Beijing 102413,China;Institute of High Energy Physics,Chinese Academy of Sciences(CAS),Beijing 100049,China;Spallation Neutron Source Science Center,Dongguan 523803,China;State Key Laboratory of Particle Detection and Electronics;Department of Modern Physics,University of Science and Technology of China,Hefei 230026,China;State Key Laboratory of Nuclear Physics and Technology,School of Physics,Peking University,Beijing 100871,China;Institute of Nuclear Physics and Chemistry,China Academy of Engineering Physics,Mianyang 621900,China;Institute of High Energy Physics,Chinese Academy of Sciences(CAS),Beijing 100049,China;Spallation Neutron Source Science Center,Dongguan 523803,China;State Key Laboratory of Particle Detection and Electronics;Institute of High Energy Physics,Chinese Academy of Sciences(CAS),Beijing 100049,China;State Key Laboratory of Particle Detection and Electronics;Northwest Institute of Nuclear Technology,Xi'an 710024,China;Institute of High Energy Physics,Chinese Academy of Sciences(CAS),Beijing 100049,China;Spallation Neutron Source Science Center,Dongguan 523803,China;University of Chinese Academy of Sciences,Beijing 100049,China;State Key Laboratory of Particle Detection and Electronics;Department of Engineering and Applied Physics,University of Science and Technology of China,Hefei 230026,China;School of Physics,Beihang University,Beijing 100083,China;Institute of High Energy Physics,Chinese Academy of Sciences(CAS),Beijing 100049,China;State Key Laboratory of Particle Detection and Electronics;University of Chinese Academy of Sciences,Beijing 100049,China).Neutron capture cross section of19Tm measured at the CSNS Back-n facility in the energy region from 30 to 300 keV[J].中国物理C(英文版),2022,第4期
  • 马欣华1,2,毕玉江1,2,曹臻1,2,3,陈明君1,2,陈松战1,2,程耀东1,2,3,龚光华4,顾旻皓1,何会海1,2,3,侯超1,2,黄文昊5,黄性涛5,刘成1,2,Oleg Shchegolev6,7,盛祥东1,2,Yuri Stenkin6,7,吴超勇1,2,吴含荣1,2,武莎1,2,肖刚1,2,姚志国1,2,张寿山1,2,张毅1,8,左雄1,2(Key Laboratory of Particle Astrophyics & Experimental Physics Division & Computing Center,Institute of High Energy Physics,Chinese Academy of Sciences;TIANFU Cosmic Ray Research Center;University of Chinese Academy of Sciences;Department of Engineering Physics,Tsinghua University;Institute of Frontier and Interdisciplinary Science,Shandong University;Institute for Nuclear Research of Russian Academy of Sciences;Moscow Institute of Physics and Technology;Key Laboratory of Dark Matter and Space Astronomy,Purple Mountain Observatory,Chinese Academy of Sciences).Chapter 1 LHAASO Instruments and Detector technology[J].中国物理C(英文版),2022,第3期
  • 王祥玉1,毕效军2,曹臻2,Piero Vallania3,吴含荣2,闫大海4,袁强5(School of Astronomy and Space Sciences,Nanjing University;Key Laboratory of Particle Astrophysics,Institute of High Energy Physics,Chinese Academy of Sciences;INAF-Osservatorio Astrofisico di Torino,Strada Osservatorio 20,10025 Pino Torinese (TO),Italy and INFN Sezione di Torino;Key Laboratory for the Structure and Evolution of Celestial Objects,Yunnan Observatories,Chinese Academy of Sciences;Key Laboratory of Dark Matter and Space Astronomy,Purple Mountain Observatory,Chinese Academy of Sciences).Chapter 3 Extra-galactic gamma-ray sources[J].中国物理C(英文版),2022,第3期
  • 陈阳1,毕效军2,方堃2,郭义庆2,刘烨3,谭柏轩4,S.Vernetto5,王仲翔6,杨睿智7,8,9,张潇1(School of Astronomy and Space Science,Nanjing University;Key Laboratory of Particle Astrophysics,Institute of High Energy Physics,CAS;School of Management Science and Engineering,Hebei University of Economics and Business;School of Physics and Astronomy,Sun Yat-Sen University;Istituto Nazionale di Astrofisica,OATO;Key Laboratory for Research in Galaxies and Cosmology,Shanghai Astronomical Observatory,Chinese Academy of Sciences;Department of Astronomy,School of Physical Sciences,University of Science and Technology of China;CAS Key Laboratory for Research in Galaxies and Cosmology,University of Science and Technology of China;School of Astronomy and Space Science,University of Science and Technology of China).Chapter 2 Galactic Gamma-ray Sources[J].中国物理C(英文版),2022,第3期
  • Benedetto D'Ettorre Piazzoli1,刘四明2,Domenico della Volpe3,曹臻4,5,Andrea Chiavassa6,Benedetto D'Ettorre Piazzoli1,郭义庆4,5,Leonid T.Ksenofontov7,Olivier Martineau-Huynh8,Diane Martraire4,马玲玲4,5,马欣华4,5,Yuri Stenkin9,10,袁强11,曾厚敦11,张寿山4,5,张毅11,朱辉12(Dipartimento di Fisica dell'Universitàdi Napoli “Federico Ⅱ”,Complesso Universitario di Monte Sant'Angelo;School of Physical Science and Technology,Southwest Jiaotong University;Département de Physique Nucléaire et Corpusculaire,Facultéde Sciences,Université de Genève;Key Laboratory of Particle Astrophyics,Institute of High Energy Physics,Chinese Academy of Sciences;TIANFU Cosmic Ray Research Center;Dipartimento di Fisica,Università degli Studi di Torino;Yu.G.Shafer Institute of Cosmophysical Research and Aeronomy SB RAS;Laboratoire de Physique Nucléaire et des Hautes Energies,CNRS-IN2P3,Universités Paris Ⅵ et Ⅶ;Institute for Nuclear Research of Russian Academy of Sciences;Moscow Institute of Physics and Technology;Key Laboratory of Dark Matter and Space Astronomy,Purple Mountain Observatory,Chinese Academy of Sciences;National Astronomical Observatories,Chinese Academy of Sciences).Chapter 4 Cosmic-Ray Physics[J].中国物理C(英文版),2022,第3期
  • 贾焕玉1,封莉2,D.Ruffolo3,Yu.V.Stenkin4,5,周勋秀1(School of Physical Science and Technology,Southwest Jiaotong University;Key Laboratory of Dark Matter and Space Astronomy,Purple Mountain Observatory,Chinese Academy of Sciences;Department of Physics,Faculty of Science,Mahidol University;Institute for Nuclear Research of Russian Academy of Sciences;Moscow Institute of Physics and Technology).Chapter 7 Solar and Heliospheric Physics and Interdisciplinary Research with LHAASO[J].中国物理C(英文版),2022,第3期
  • 黎卓1,2,Giuseppe Di Sciascio3,苟全补4,郭义庆4,贺昊宁5,柳若愚6,7,王凯8(Department of Astronomy,School of Physics,Peking University;Kavli Institute for Astronomy and Astrophysics,Peking University;INFN-Roma Tor Vergata;Key Laboratory of Particle Astrophysics,Institute of High Energy Physics,Chinese Academy of Sciences;Key Laboratory of Dark Matter and Space Astronomy,Purple Mountain Observatory,Chinese Academy of Sciences;School of Astronomy and Space Science,Nanjing University;Key laboratory of Modern Astronomy and Astrophysics (Nanjing University),Ministry of Education;Department of Astronomy,School of Physics,Huazhong University of Science and Technology).Chapter 6 Multimessenger Physics[J].中国物理C(英文版),2022,第3期
  • 毕效军1,Andrea Addazi2,3,Konstantin Belotsky4,Vitaly Beylin5,Marco Cirelli6,Arman Esmaili7,Nicolao Fornengo8,9,甘庆余2,Michael Kachekriess10,Maxim Khlopov11,4,5,Vladimir Korchagin5,Alexander Korochkin11,Vladimir Kuksa5,Antonino Marciano12,3,Andrei Neronov11,13,Paolo Panci14,Roman Pasechnick15,Alexander Sakharov16,17,Filippo Sala6,Giuseppe Di Sciascio18,Dimiri Semikoz11,4,Pasquale Dario Serpico19,Nikolay Volchanskiy5,20,殷鹏飞1(Key Laboratory of Particle Astrophysics,Institute of High Energy Physics,Chinese Academy of Sciences;Center for Theoretical Physics,College of Physics Science and Technology,Sichuan University;Laboratori Nazionali di Frascati INFN;National Research Nuclear University MEPHI (Moscow State Engineering Physics Institute);Institute of Physics,Southern Federal University Stachki 194;LPTHE,CNRS and Sorbonne Universit'e;Departamento de Fisica,Pontificia Universidade Catolica do Rio de Janeiro;Dipartimento di Fisica,Universita di Torino;Istituto Nazionale di Fisica Nucleare,Sezione di Torino;Institutt for fysikk,NTNU;Universite de Paris,CNRS,Astroparticule et Cosmologie;Department of Physics and Center for Field Theory and Particle Physics,Fudan University;Astronomy Department,University of Geneve;Dipartimento di Fisica,Universita di Pisa and INFN,Sezione di Pisa Largo Pontecorvo 3;Department of Astronomy and Theoretical Physics,Lund University;Experimental Physics Department,CERN;Department of Physics,New York University;INFN sezione Roma Tor Vergata;LAPTh,Univ.Grenoble Alpes,USMB,CNRS;Bogoliubov Laboratory of Theoretical Pjysics,JINR).Chapter 5 Dark Matter and New Physics Beyond the Standard Model with LHAASO[J].中国物理C(英文版),2022,第3期
  • Zhen Cao(LHAASO Collaboration).Preface[J].中国物理C(英文版),2022,第3期
  • 袁子懿1,柏栋1,任中洲1,2,王震1(School of Physics Science and Engineering,Tongji University;Key Laboratory of Advanced Micro-Structure Materials,Ministry of Education).Theoretical predictions on α-decay properties of some unknown neutrondeficient actinide nuclei using machine learning[J].Chinese Physics C,2022,第2期
  • 陈永静1,宿阳1,董国香2,刘丽乐1,葛智刚1,王小保2(China Nuclear Data Center,China Institute of Atomic Energy;School of Science,Huzhou University).Energy density functional analysis of the fission properties of 240Pu:The effect of pairing correlations[J].Chinese Physics C,2022,第2期
  • 王晓倩1,2,孙向向3,周善贵1,2,3(CAS Key Laboratory of Theoretical Physics,Institute of Theoretical Physics,Chinese Academy of Science;School of Physical Sciences,University of Chinese Academy of Sciences;School of Nuclear Science and Technology,University of Chinese Academy of Sciences).Microscopic study of higher-order deformation effects on the ground states of superheavy nuclei around 270Hs[J].Chinese Physics C,2022,第2期
  • 王凯雷1,2,钟显辉3,4(Department of Electronic Information and Physics,Changzhi University;Synergetic Innovation Center for Quantum Effects and Applications SICQEA,Hunan Normal University;Department of Physics,Hunan Normal University,and Key Laboratory of Low-Dimensional Quantum Structures and Quantum Control of Ministry of Education;Synergetic Innovation Center for Quantum Effects and Applications (SICQEA),Hunan Normal University).Toward discovering low-lying P-wave excited Σc baryon states[J].Chinese Physics C,2022,第2期
  • 董宇兵1,沈彭年2(Institute of High Energy Physics,Chinese Academy of Sciences;School of Physical Sciences,University of Chinese Academy of Sciences).Possible dibaryon production at ?anda with a Lagrangian approach[J].Chinese Physics C,2022,第2期
  • 韦能昌1,朱一鸣2,黄飞1(School of Nuclear Science and Technology,University of Chinese Academy of Sciences;School of Physical Sciences,University of Chinese Academy of Sciences).Photoproduction reaction γn → K*0 Λ in an effective Lagrangian approach[J].Chinese Physics C,2022,第2期
  • 陈诗乐,王梓岳,庄鹏飞(Physics Department,Tsinghua University).Equal-time kinetic equations in a rotational field[J].Chinese Physics C,2022,第2期
  • 李明哲,牟一岑,饶浩民,赵德浩(Interdisciplinary Center for Theoretical Study,University of Science and Technology of China;Peng Huanwu Center for Fundamental Theory).Gravitational leptogenesis in teleparallel and symmetric teleparallel gravities[J].Chinese Physics C,2022,第2期
  • 凌意1,2,吴孟和3,4(Institute of High Energy Physics,Chinese Academy of Sciences;School of Physics,University of Chinese Academy of Sciences;School of Mathematics,Physics and Statistics,Shanghai University of Engineering Science;Center of Application and Research of Computational Physics,Shanghai University of Engineering Science).Modified regular black holes with time delay and 1-loop quantum correction[J].Chinese Physics C,2022,第2期
  • 魏明华1,2,姜寅3,黄梅1(School of Nuclear Science and Technology,University of Chinese Academy of Sciences;Institute of High Energy Physics,Chinese Academy of Sciences;Department of Physics,BeiHang University).Mass splitting of vector mesons and spontaneous spin polarization under rotation[J].Chinese Physics C,2022,第2期
  • 程凯旋1,许昌2,马春旺1,普洁1,王玉廷1(School of Physics,Henan Normal University;School of Physics,Nanjing University).Pauli blocking potential applied to heavy-ion fusion reactions[J].Chinese Physics C,2022,第2期
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