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作 者:Ariel Arza Quan Guo Lei Wu Qiaoli Yang Xiaolong Yang Qiang Yuan Bin Zhu Ariel Arza;郭铨;武雷;杨娇立;杨小龙;袁强;祝斌
机构地区:[1]Department of Physics and Institute of Theoretical Physics,Nanjing Normal University,Nanjing 210023,China [2]Shanghai Astronomical Observatory,Chinese Academy Sciences,Shanghai 200030,China [3]College of Physics and Optoelectronic Engineering,Department of Physics,Jinan University,Guangzhou 510632,China [4]Shanghai Key Laboratory of Space Navigation and Positioning Techniques,Shanghai 200030,China [5]Key Laboratory of Dark Matter and Space Astronomy,Purple Mountain Observatory,Chinese Academy of Sciences,Nanjing 210023,China [6]School of Astronomy and Space Science,University of Science and Technology of China,Hefei 230026,China [7]Department of Physics,Yantai University,Yantai 264005,China
出 处:《Science Bulletin》2024年第19期2971-2973,共3页科学通报(英文版)
基 金:supported by the National Natural Science Foundation of China(12275134,12275232,12335005,12147228,12150010,and 12103076);the Project for Young Scientists in Basic Research of Chinese Academy of Sciences(YSBR-061);the Ministry of Science and Technology of China(2020SKA0110200).
摘 要:The axion is nowadays one of the leading candidates to compose the dark matter of the universe.A great experimental effort has been performed by the so-called axion haloscopes experiments among others(for complete reviews on updated axion phenomenology,see Ref.[1]).
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