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Tao LIU (The Hong Kong University of Science and Technology)14/01/2021, 12:58
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Jack COLLINS (SLAC National Accelerator Laboratory)14/01/2021, 13:00Theory
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Chandrashekhar JOSHI (University of California, Los Angeles)14/01/2021, 13:00Accelerator
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Joao GUIMARAES DA COSTA (Institute of High Energy Physics, Chinese Academy of Sciences)14/01/2021, 13:00
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Mogens DAM (Niels Bohr Institute, University of Copenhagen)14/01/2021, 13:05
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Mihoko NOJIRI (High Energy Accelerator Research Organization (KEK))14/01/2021, 13:30Theory
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Chunhui CHEN (Iowa State University)14/01/2021, 13:45
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Warren MORI (University of California, Los Angeles)14/01/2021, 13:50Accelerator
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Haipeng AN (Tsinghua University)14/01/2021, 14:00Theory
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Carl LINDSTRØM (Deutsches Elektronen-Synchrotron (DESY))14/01/2021, 14:20Accelerator
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Changzheng YUAN (Institute of High Energy Physics, Chinese Academy of Sciences)14/01/2021, 14:40
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Sunghoon JUNG (Seoul National University)14/01/2021, 14:40Theory
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Wei LU (Tsinghua University)14/01/2021, 14:50Accelerator
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Ke-Pan XIE (Seoul National University)14/01/2021, 15:10Theory
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Yuehong XIE (CERN)14/01/2021, 15:25
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Xiaoning WANG (Institute of High Energy Physics, Chinese Academy of Sciences)14/01/2021, 15:30Accelerator
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Roberto FRANCESCHINI (Roma Tre University)14/01/2021, 15:40Theory
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Christopher DOSS (University of Colorado, Boulder)14/01/2021, 15:50Accelerator
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Asher BERLIN (New York University)14/01/2021, 21:00Theory
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Paolo AZZURRI (INFN Sezione di Pisa, Universita' e Scuola Normale Superiore)14/01/2021, 21:00
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Ralph Wolfgang ASSMANN (Deutsches Elektronen-Synchrotron (DESY))14/01/2021, 21:00Accelerator
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Yotam SOREQ (Technion – Israel Institute of Technology)14/01/2021, 21:30Theory
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Jia LIU (Peking University)14/01/2021, 21:45
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Markus BUESCHER (Forschungszentrum Jülich)14/01/2021, 21:50Accelerator
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Roni HARNIK (Fermi National Accelerator Laboratory)14/01/2021, 22:00Theory
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Shiyu ZHOU (Tsinghua University)14/01/2021, 22:10Accelerator
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Ian LOW (Northwestern University)14/01/2021, 22:40Theory
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Leo PIILONEN (Virginia Tech)14/01/2021, 22:40
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Min CHEN (Shanghai Jiao Tong University)14/01/2021, 22:40Accelerator
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Francesco RIVA (University of Geneva)14/01/2021, 23:10Theory
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Wenjun MA (Peking University)14/01/2021, 23:10Accelerator
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Thomas HEMMICK (Stony Brook University)14/01/2021, 23:25
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Shuang LIU (Tsinghua University)14/01/2021, 23:40Accelerator
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Adam MARTIN (University of Notre Dame)14/01/2021, 23:40Theory
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Jing SHU (Institute of Theoretical Physics, Chinese Academy Sciences)15/01/2021, 00:10
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Zhengkang ZHANG (California Institute of Technology)15/01/2021, 13:00Theory
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Guy WILKINSON (CERN)15/01/2021, 13:00
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Mark J. HOGAN (SLAC National Accelerator Laboratory)15/01/2021, 13:00Accelerator
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Daniel CARNEY (University of Maryland)15/01/2021, 13:30Theory
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Zhijun LIANG (Institute of High Energy Physics, Chinese Academy of Sciences)15/01/2021, 13:45
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Spencer GESSNER (SLAC National Accelerator Laboratory)15/01/2021, 13:50Accelerator
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Raffaele Tito D'AGNOLO (French Alternative Energies and Atomic Energy Commission (CEA))15/01/2021, 14:00Theory
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Zan NIE (University of California, Los Angeles)15/01/2021, 14:10Accelerator
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Piotr GASIK (CERN)15/01/2021, 14:40
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Masaki KANDO (National Institutes for Quantum and Radiological Science and Technology)15/01/2021, 14:40Accelerator
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Cen ZHANG (Institute of High Energy Physics, Chinese Academy of Sciences)15/01/2021, 14:40Theory
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Jiayin GU (Johannes Gutenberg University Mainz)15/01/2021, 15:10Theory
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Jiansheng LIU (Shanghai Normal University)15/01/2021, 15:10Accelerator
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Francesco GRANCAGNOLO (The Italian National Institute of Nuclear Physics)15/01/2021, 15:25
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Teng MA (Technion - Israel Institute of Technology)15/01/2021, 15:40Theory
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Ming ZENG (Institute of High Energy Physics, Chinese Academy of Sciences)15/01/2021, 15:40Accelerator
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Patric MUGGLI (Max Planck Institute for Physics)15/01/2021, 21:00Accelerator
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Lingfeng LI (The Hong Kong University of Science and Technology (IAS Postdoctoral Fellow))15/01/2021, 21:00Theory
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Imad LAKTINEH (Institute of Physics of the 2 Infinities of Lyon)15/01/2021, 21:00
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Roman POESCHL (Laboratory of the Physics of the 2 infinities Irène Joliot-Curie)15/01/2021, 21:20
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David SHIH (Rutgers University)15/01/2021, 21:30Theory
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Massimo FERRARIO (The Italian National Institute for Nuclear Physics)15/01/2021, 21:40Accelerator
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Roberto FERRARI (CERN)15/01/2021, 21:55
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Benjamin Philip NACHMAN (Lawrence Berkeley National Laboratory)15/01/2021, 22:00Theory
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Paramel Pattathil RAJEEV (Rutherford Appleton Laboratory)15/01/2021, 22:00Accelerator
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Baifei SHEN (Shanghai Normal University)15/01/2021, 22:40Accelerator
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Silvia DALLA TORRE (The Italian National Institute for Nuclear Physics)15/01/2021, 22:40
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Nathaniel CRAIG (University of California, Santa Barbara)15/01/2021, 22:40Theory
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Weiming AN (Beijing Normal University)15/01/2021, 23:10Accelerator
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Liantao WANG (University of Chicago)15/01/2021, 23:10Theory
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Michal KREPS (CERN)15/01/2021, 23:25
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Yuqiu GU (China Academy of Engineering Physics)15/01/2021, 23:30Accelerator
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Da LIU (University of California, Davis)15/01/2021, 23:40Theory
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Andrew G. COHEN (The Hong Kong University of Science and Technology (IAS Director, Acting Dean of Science and Lam Woo Foundation Professor))18/01/2021, 20:50Plenary
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Raman SUNDRUM (University of Maryland)18/01/2021, 21:00Plenary
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Oliver BRÜNING (CERN)18/01/2021, 21:45Plenary
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Jie GAO (Institute of High Energy Physics, Chinese Academy of Sciences)18/01/2021, 22:40Plenary
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Michael BENEDIKT (CERN)18/01/2021, 23:25Plenary
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Wei LU (Tsinghua University)19/01/2021, 16:00Accelerator
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Fotios KOUTROULIS (National Technical University of Athens)19/01/2021, 16:00Theory
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Peter SKANDS (Monash University)19/01/2021, 16:00Experiment / Detector
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Frank ZIMMERMANN (CERN)19/01/2021, 16:20Accelerator
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Marcel VOS (The Instituto de Física Corpuscular Valencia (UVEG/CSIC))19/01/2021, 16:20Experiment / Detector
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Madan SINGH (M. N. S Government College Bhiwani)19/01/2021, 16:24Theory
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Chenghui YU (Institute of High Energy Physics, Chinese Academy of Sciences)19/01/2021, 16:40Accelerator
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Daniel JEANS (High Energy Accelerator Research Organization (KEK))19/01/2021, 16:40Experiment / Detector
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Álvaro JESUS (International Institute of Physics / Federal University of Rio Grande do Norte)19/01/2021, 16:48Theory
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Yiwei WANG (Institute of High Energy Physics, Chinese Academy of Sciences)19/01/2021, 17:00Accelerator
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Bruce MELLADO GARCIA (University of the Witwatersrand)19/01/2021, 17:00
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Sven HEINEMEYER (Spanish National Research Council (CSIC))19/01/2021, 17:12Theory
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Bin WANG (Institute of High Energy Physics, Chinese Academy of Sciences)19/01/2021, 17:20Accelerator
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Manqi RUAN (Institute of High Energy Physics, Chinese Academy of Sciences)19/01/2021, 17:20Experiment / Detector
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Yoxara Sánchez VILLAMIZAR (International Institute of Physics, Federal University of Rio Grande do Norte)19/01/2021, 17:36Theory
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Dou WANG (Institute of High Energy Physics, Chinese Academy of Sciences)19/01/2021, 17:40Accelerator
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Giulio MEZZADRI (The Italian National Institute for Nuclear Physics)19/01/2021, 17:40Experiment / Detector
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Valentina DIOLAITI (Bologna University)19/01/2021, 18:00Experiment / Detector
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Anton BOGOMYAGKOV (Budker Institute of Nuclear Physics)19/01/2021, 21:00Plenary
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Yukiyoshi OHNISHI (High Energy Accelerator Research Organization (KEK))19/01/2021, 21:45Plenary
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Anatoly SIDORIN (Joint Institute for Nuclear Research (JINR))19/01/2021, 22:40Plenary
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Andrei SERYI (Thomas Jefferson National Accelerator Facility)19/01/2021, 23:25Plenary
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Jia LIU (Peking University)20/01/2021, 16:00Theory
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Ralph Wolfgang ASSMANN (Deutsches Elektronen-Synchrotron (DESY))20/01/2021, 16:00Accelerator
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Lingfeng LI (The Hong Kong University of Science and Technology (IAS Postdoctoral Fellow))20/01/2021, 16:00Experiment / Detector
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Cai MENG (Institute of High Energy Physics, Chinese Academy of Sciences)20/01/2021, 16:20Accelerator
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Francesco GRANCAGNOLO (The Italian National Institute for Nuclear Physics - Lecce Section)20/01/2021, 16:20Experiment / Detector
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Xiaoping WANG (Beihang University)20/01/2021, 16:24Theory
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Jinhui CHEN (Institute of High Energy Physics, Chinese Academy of Sciences)20/01/2021, 16:40Accelerator
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Valentin VOLKL (CERN)20/01/2021, 16:40Experiment / Detector
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Wei SU (University of Adelaide)20/01/2021, 16:48Theory
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Jiyuan ZHAI (Institute of High Energy Physics, Chinese Academy of Sciences)20/01/2021, 17:00Accelerator
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Yong LIU (Institute of High Energy Physics, Chinese Academy of Sciences)20/01/2021, 17:00Experiment / Detector
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Shao-Feng GE (Tsung-Dao Lee Institute, Shanghai Jiao Tong University)20/01/2021, 17:12Theory
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Marco LUCCHINI (Princeton University)20/01/2021, 17:20Experiment / Detector
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Zusheng ZHOU (Institute of High Energy Physics, Chinese Academy of Sciences)20/01/2021, 17:20Accelerator
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Zihui WANG (New York University)20/01/2021, 17:36Theory
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Yongsheng MA (Institute of High Energy Physics, Chinese Academy of Sciences)20/01/2021, 17:40Accelerator
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Hiroyuki NAKAYAMA (High Energy Accelerator Research Organization (KEK))20/01/2021, 17:40
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Junsong CANG (Institute of High Energy Physics, Chinese Academy of Sciences)20/01/2021, 18:00
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Gaosong LI (Institute of High Energy Physics, Chinese Academy of Sciences)20/01/2021, 18:00Experiment / Detector
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Max KLEIN (University of Liverpool)20/01/2021, 18:20
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Yongchao ZHANG (Southeast University)20/01/2021, 18:25
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Shinichiro MICHIZONO (High Energy Accelerator Research Organization (KEK))20/01/2021, 21:00Plenary
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Steinar STAPNES (CERN)20/01/2021, 21:45Plenary
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Matthew Philip MCCULLOUGH (CERN)20/01/2021, 22:40Plenary
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Tao HAN (University of Pittsburgh)20/01/2021, 23:25Plenary
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Michael KORATZINOS (CERN and Massachusetts Institute of Technology)21/01/2021, 16:00Accelerator
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Martin ALEKSA (CERN)21/01/2021, 16:00Experiment / Detector
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João SEABRA (Instituto Superior Técnico)21/01/2021, 16:00Theory
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Sha BAI (Institute of High Energy Physics, Chinese Academy of Sciences)21/01/2021, 16:20Accelerator
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Adrian IRLES (IFIC - CSIC/UV)21/01/2021, 16:20Experiment / Detector
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Bin YAN (Los Alamos National Laboratory)21/01/2021, 16:24Theory
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Yingshun ZHU (Institute of High Energy Physics, Chinese Academy of Sciences)21/01/2021, 16:40Accelerator
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Hwi Dong YOO (Yonsei University)21/01/2021, 16:40Experiment / Detector
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Huayang SONG (University of Arizona)21/01/2021, 16:48Theory
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Wen KANG (Institute of High Energy Physics, Chinese Academy of Sciences)21/01/2021, 17:00Accelerator
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Magnus MAGER (CERN)21/01/2021, 17:00Experiment / Detector
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Krzysztof JODLOWSKI (National Centre for Nuclear Research)21/01/2021, 17:12Theory
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Yanfeng SUI (Institute of High Energy Physics, Chinese Academy of Sciences)21/01/2021, 17:20Accelerator
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Claudia BERTELLA (CERN)21/01/2021, 17:20Experiment / Detector
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Bruce Mellado GARCIA (University of the Witwatersrand)21/01/2021, 17:36Theory
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Sebastian GRINSTEIN (The Institute for High Energy Physics of Barcelona)21/01/2021, 17:40Experiment / Detector
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Qingjin XU (Institute of High Energy Physics, Chinese Academy of Sciences)21/01/2021, 17:40Accelerator
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Wei LIU (Nanjing University of Science and Technology)21/01/2021, 18:00
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Huirong QI (Institute of High Energy Physics, Chinese Academy of Sciences)21/01/2021, 18:00Experiment / Detector
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Vladimir SHILTSEV (Fermi National Accelerator Laboratory)21/01/2021, 21:00Plenary
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Jesse THALER (Massachusetts Institute of Technology)21/01/2021, 21:45Plenary
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Hitoshi YAMAMOTO (Tohoku University), Michael BENEDIKT (CERN), Raman SUNDRUM (University of Maryland), Steinar STAPNES (CERN), Tao HAN (University of Pittsburgh), Vladimir SHILTSEV (Fermi National Accelerator Laboratory), Yifang WANG (Institute of High Energy Physics, Chinese Academy of Sciences)21/01/2021, 22:30Plenary
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Tao LIU (The Hong Kong University of Science and Technology)21/01/2021, 23:30Plenary
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Sebastian TROJANOWSKI (Nicolaus Copernicus Astronomical Center)
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TBCExperiment / Detector
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Madan Singh (M. N. S Government College Bhiwani Haryana India)
In the present analysis, I have constructed the CP odd weak basis invariants (WB) at low energies, for Majorana neutrino mass matrix having a condition of two zeros and an equality between arbitrary non-zero elements in the flavor basis, where charged lepton mass matrix is diagonal. This particular form of neutrino mass matrix, also known as hybrid texture, is found to be viable with the...
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Prof. Shao-Feng Ge (TDLI-SJTU)
We demonstrate how probes of CP-violating observables in Higgs di-tau decays at prospective future lepton colliders could provide a test of weak scale baryogenesis with significant discovery potential. Measurements at the Circular Electron Positron Collider, for example, could exclude a CP phase larger than 2.9∘ (5.6∘) at 68% (95%) C.L. assuming the Standard Model value for magnitude of the...
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Ms Yoxara Sánchez Villamizar (nternational Institute of Physics (IIP) and Department of Theoretical and Experimental Physics- UFRN), Mr Álvaro Santos de jesus (International Institute of Physics), Prof. Sergey Kovalenko (Departamento de Ciencias Físicas Universidad Andres Bello), Prof. C.A. de S Pires (Departamento de Física, Universidade Federal da Paraíba), Prof. Farinaldo Queiroz (International Institute of Physics)
We have witnessed a persistent puzzling anomaly in the muon magnetic moment that cannot be accounted for in the Standard Model even considering the existing large hadronic uncertainties. A new measurement is forthcoming, and it might give rise to a 5 σ claim for physics beyond the Standard Model. Motivated by it, we explore the implications of this new result to five models based on the...
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Dr Bin Yan (Los Alamos National Laboratory)
Search for charged lepton flavor violation (CLFV) is one of the core elements to discover new physics beyond the SM. In this talk, I will perform a comprehensive and systematic analysis of the CLFV sensitivity at the EIC, LHC and low energy data in the framework of the SMEFT.
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Zihui Wang (NYU)
Multiple microlensing surveys have been conducted to place limits on primordial black holes in nearby dark matter halos. We show that these existing limits on PBHs can be recasted to constrain dark matter lenses that are more spatially extended than PBHs. As two representative cases, we consider NFW subhalos and boson stars, which are predicted in many models such as axion miniclusters and...
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Prof. Xiaoping Wang (Beihang University)
We propose novel CP-violating observables in complex two-Higgs-doublet models
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and undertake a systematic study of the interplay between Higgs alignment and CP-violation, which enables us to distinguish two separate sources of CP-violation in the scalar sector: in the mixing and in the decay, and identify a scenario where departures from Higgs alignment could be present independently of... -
Nestor Armesto Perez (Universidade de Santiago de Compostela (ES))
The Large Hadron-electron Collider (LHeC) is a proposed upgrade of the LHC at CERN. It consists of an ERL providing electrons to collide with the HL-LHC, HE-LHC and the FCC-hh proton beams achieving centre-of-mass energies 1.3-3.5 TeV and luminosities $\sim 10^{34}$ cm$^{−2}$ s$^{−1}$, respectively. These large energies and luminosities lead to charged current Higgs production cross sections...
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Sven Heinemeyer (CSIC (Madrid, ES))
In view of the current and possible future measurements of (g-2)_mu we investigate several SUSY scenarios. In all cases the (g-2)_mu measurements set upper limits on SUSY particle masses and several light EW particles are guaranteed. These predictions are analyzed in view of future collider searches (pp and e+e-).
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Ke-Pan Xie (Seoul National University)
An electroweak baryogenesis (EWBG) mechanism mediated by $\tau$ lepton transport is proposed. We extend the Standard Model with a real singlet scalar $S$ to trigger the strong first-order electroweak phase transition (SFOEWPT), and with a set of leptophilic dimension-5 operators to provide sufficient CP violating source. We demonstrate this model is able to generate the observed baryon...
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Krzysztof Jodlowski (National Centre for Nuclear Research)
Many Beyond Standard Model (BSM) physics scenarios contain new long-lived particles (LLPs), leading to interesting experimental signatures such as e.g. highly-displaced decay signatures. Examples of such minimal models are so-called portals which include coupling of New Physics particle to SM particles through a renormalizable interaction. Going beyond such simple realisations of BSM physics,...
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João Seabra (Instituto Superior Técnico)
Jet identification tools are crucial for new physics searches at the LHC and at future colliders. We introduce the concept of Mass Unspecific Supervised Tagging (MUST) which relies on considering both jet mass and transverse momentum varying over wide ranges as input variables - together with jet substructure observables - of a multivariate tool. This approach not only provides a single...
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Fotis Koutroulis (National Technical University of Athens)
We construct the zero temperature (no compact dimensions) effective action for an SU(2) Yang-Mills theory in five dimensions, with boundary conditions that reduce the symmetry on the four-dimensional boundary located at the origin to a U(1)-complex scalar system. In order to be sensitive to the Higgs phase, we need to include higher dimensional operators in the effective action, which can be...
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Jing Shu (ITP-CAS)
We derive the generalized partial wave expansion for N → M scattering amplitude in terms of spinor helicity variables. The basis amplitudes of the expansion with definite angular momentum j consist of the Poincar ́e Clebsch-Gordan coefficients. Moreover, we obtain a series of selection rules that restrict the anomalous dimension matrix of effective operators and the way how effective operators...
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Huayang Song (University of Arizona)Theory
The naturalness problem motivates new physics beyond the Standard Model (SM). The Higgs sector in neutral naturalness models provides a portal to the hidden QCD sector, and thus Higgs coupling measurements play a central role in exploring the model parameter space. We investigate a class of neutral naturalness models, in which the Higgs boson is a pseudo-Goldstone boson with the radial mode at...
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Dr Wei Liu (Nanjing University of Science and Technology)Theory
In this talk, we study some of the consequence of one example of a beyond the Standard Model theory. Namely, we discuss a model based on a spontaneously broken $B-L$ gauge symmetry. It can explain the light neutrino masses via a Type-I seesaw mechanism with heavy neutrinos. From the limits on the light neutrinos masses due to double beta decay experiments and cosmological observations together...
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Junsong Cang (Chinese Academy of Sciences)Theory
Cascade of particles injected due to the decay and annihilation of dark matter (DM) particles and Primordial black hole (PBH), which has gained increasing interests as an alternative candidate for DM, can potentially change the cosmic recombination history by ionizing and heating the intergalactic medium, which results in altering the anisotropy spectra of the Cosmic Microwave Background...
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Wei Su (University of Adelaide)
The electroweak phase transition can be made first order by extending the Standard Model (SM) Higgs sector with extra scalars.
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In this talk, we focus one the a strong first order electroweak phase transition (SFOEWPT) in the type-I and type-II two Higgs doublet models (2HDM). Through a parameter space scan, we find that SFOEWPT suggests upper limits on the masses of the heavy Higgs... -
Dr Huirong Qi (Institute of High Energy Physics, CAS)
To achieve the physical goals in the future circular collider, the high resolution tracker for the particle track reconstruction and particle identification are demanded. Time Projection Chamber(TPC) is one of the main concept proposal of the central tracker detector, it has an excellent performance on the moment measurement, $dE/dx$ measurement and the spation resolution.
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Based on the... -
Bruce Mellado Garcia (University of the Witwatersrand)
Based on a number of features from proton-proton collisions taken during Run 1 data taking period at the LHC, a boson with a mass around the Electro-Weak scale was postulated such that a significant fraction of its decays would comprise the Standard Model (SM) Higgs boson and an additional scalar, S. One of the phenomenological implications of a simplified model, where S is treated a SM Higgs...
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Yongchao Zhang (Southeast University)Theory
Abstract: A light CP-even scalar $S$ with mass below GeV-scale exists in may beyond standard model (SM) scenarios. Such a light particle can be produced abundantly in the stars, such as the Sun, red giants, white dwarfs, horizontal-branch stars, neutron star mergers, and supernovae. In this talk I will show the state-of-art stellar limits on $S$. Assuming the couplings of $S$ to the SM...
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Ms Álvaro Jesus (International Institute of Physics / Federal University of Rio )Theory
We investigate simplified models involving an inert scalar triplet and vector-like leptons that can account for the muon g−2 anomaly. These simplified scenarios are embedded in a model that features W' and Z' bosons, which are subject to stringent collider bounds. The constraints coming from the muon g−2 anomaly are put into perspective with collider bounds, as well as bounds coming from...
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