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First Search for the Absorption of Fermionic Dark Matter with the PandaX-4T Experiment.
Gu, Linhui; Abdukerim, Abdusalam; Bo, Zihao; Chen, Wei; Chen, Xun; Chen, Yunhua; Cheng, Chen; Cheng, Yunshan; Cheng, Zhaokan; Cui, Xiangyi; Fan, Yingjie; Fang, Deqing; Fu, Changbo; Fu, Mengting; Geng, Lisheng; Giboni, Karl; Guo, Xuyuan; Han, Ke; He, Changda; He, Jinrong; Huang, Di; Huang, Yanlin; Huang, Zhou; Hou, Ruquan; Ji, Xiangdong; Ju, Yonglin; Li, Chenxiang; Li, Jiafu; Li, Mingchuan; Li, Shu; Li, Shuaijie; Lin, Qing; Liu, Jianglai; Lu, Xiaoying; Luo, Lingyin; Luo, Yunyang; Ma, Wenbo; Ma, Yugang; Mao, Yajun; Shaheed, Nasir; Meng, Yue; Ning, Xuyang; Qi, Ningchun; Qian, Zhicheng; Ren, Xiangxiang; Shang, Changsong; Shang, Xiaofeng; Shen, Guofang; Si, Lin; Sun, Wenliang.
Afiliação
  • Gu L; School of Physics and Astronomy, Shanghai Jiao Tong University, Key Laboratory for Particle Astrophysics and Cosmology (MoE), Shanghai Key Laboratory for Particle Physics and Cosmology, Shanghai 200240, China.
  • Abdukerim A; School of Physics and Astronomy, Shanghai Jiao Tong University, Key Laboratory for Particle Astrophysics and Cosmology (MoE), Shanghai Key Laboratory for Particle Physics and Cosmology, Shanghai 200240, China.
  • Bo Z; School of Physics and Astronomy, Shanghai Jiao Tong University, Key Laboratory for Particle Astrophysics and Cosmology (MoE), Shanghai Key Laboratory for Particle Physics and Cosmology, Shanghai 200240, China.
  • Chen W; School of Physics and Astronomy, Shanghai Jiao Tong University, Key Laboratory for Particle Astrophysics and Cosmology (MoE), Shanghai Key Laboratory for Particle Physics and Cosmology, Shanghai 200240, China.
  • Chen X; School of Physics and Astronomy, Shanghai Jiao Tong University, Key Laboratory for Particle Astrophysics and Cosmology (MoE), Shanghai Key Laboratory for Particle Physics and Cosmology, Shanghai 200240, China.
  • Chen Y; Shanghai Jiao Tong University Sichuan Research Institute, Chengdu 610213, China.
  • Cheng C; Yalong River Hydropower Development Company, Ltd., 288 Shuanglin Road, Chengdu 610051, China.
  • Cheng Y; School of Physics, Sun Yat-Sen University, Guangzhou 510275, China.
  • Cheng Z; Research Center for Particle Science and Technology, Institute of Frontier and Interdisciplinary Science, Shandong University, Qingdao 266237, Shandong, China.
  • Cui X; Key Laboratory of Particle Physics and Particle Irradiation of Ministry of Education, Shandong University, Qingdao 266237, Shandong, China.
  • Fan Y; Sino-French Institute of Nuclear Engineering and Technology, Sun Yat-Sen University, Zhuhai 519082, China.
  • Fang D; Tsung-Dao Lee Institute, Shanghai Jiao Tong University, Shanghai 200240, China.
  • Fu C; School of Physics, Nankai University, Tianjin 300071, China.
  • Fu M; Key Laboratory of Nuclear Physics and Ion-beam Application (MOE), Institute of Modern Physics, Fudan University, Shanghai 200433, China.
  • Geng L; Key Laboratory of Nuclear Physics and Ion-beam Application (MOE), Institute of Modern Physics, Fudan University, Shanghai 200433, China.
  • Giboni K; School of Physics, Peking University, Beijing 100871, China.
  • Guo X; School of Physics, Beihang University, Beijing 102206, China.
  • Han K; International Research Center for Nuclei and Particles in the Cosmos and Beijing Key Laboratory of Advanced Nuclear Materials and Physics, Beihang University, Beijing 100191, China.
  • He C; School of Physics and Microelectronics, Zhengzhou University, Zhengzhou, Henan 450001, China.
  • He J; School of Physics and Astronomy, Shanghai Jiao Tong University, Key Laboratory for Particle Astrophysics and Cosmology (MoE), Shanghai Key Laboratory for Particle Physics and Cosmology, Shanghai 200240, China.
  • Huang D; Yalong River Hydropower Development Company, Ltd., 288 Shuanglin Road, Chengdu 610051, China.
  • Huang Y; School of Physics and Astronomy, Shanghai Jiao Tong University, Key Laboratory for Particle Astrophysics and Cosmology (MoE), Shanghai Key Laboratory for Particle Physics and Cosmology, Shanghai 200240, China.
  • Huang Z; School of Physics and Astronomy, Shanghai Jiao Tong University, Key Laboratory for Particle Astrophysics and Cosmology (MoE), Shanghai Key Laboratory for Particle Physics and Cosmology, Shanghai 200240, China.
  • Hou R; Yalong River Hydropower Development Company, Ltd., 288 Shuanglin Road, Chengdu 610051, China.
  • Ji X; School of Physics and Astronomy, Shanghai Jiao Tong University, Key Laboratory for Particle Astrophysics and Cosmology (MoE), Shanghai Key Laboratory for Particle Physics and Cosmology, Shanghai 200240, China.
  • Ju Y; School of Medical Instrument and Food Engineering, University of Shanghai for Science and Technology, Shanghai 200093, China.
  • Li C; School of Physics and Astronomy, Shanghai Jiao Tong University, Key Laboratory for Particle Astrophysics and Cosmology (MoE), Shanghai Key Laboratory for Particle Physics and Cosmology, Shanghai 200240, China.
  • Li J; Shanghai Jiao Tong University Sichuan Research Institute, Chengdu 610213, China.
  • Li M; Department of Physics, University of Maryland, College Park, Maryland 20742, USA.
  • Li S; School of Mechanical Engineering, Shanghai Jiao Tong University, Shanghai 200240, China.
  • Li S; School of Physics and Astronomy, Shanghai Jiao Tong University, Key Laboratory for Particle Astrophysics and Cosmology (MoE), Shanghai Key Laboratory for Particle Physics and Cosmology, Shanghai 200240, China.
  • Lin Q; School of Physics, Sun Yat-Sen University, Guangzhou 510275, China.
  • Liu J; Yalong River Hydropower Development Company, Ltd., 288 Shuanglin Road, Chengdu 610051, China.
  • Lu X; School of Mechanical Engineering, Shanghai Jiao Tong University, Shanghai 200240, China.
  • Luo L; Tsung-Dao Lee Institute, Shanghai Jiao Tong University, Shanghai 200240, China.
  • Luo Y; State Key Laboratory of Particle Detection and Electronics, University of Science and Technology of China, Hefei 230026, China.
  • Ma W; Department of Modern Physics, University of Science and Technology of China, Hefei 230026, China.
  • Ma Y; School of Physics and Astronomy, Shanghai Jiao Tong University, Key Laboratory for Particle Astrophysics and Cosmology (MoE), Shanghai Key Laboratory for Particle Physics and Cosmology, Shanghai 200240, China.
  • Mao Y; Shanghai Jiao Tong University Sichuan Research Institute, Chengdu 610213, China.
  • Shaheed N; Tsung-Dao Lee Institute, Shanghai Jiao Tong University, Shanghai 200240, China.
  • Meng Y; Research Center for Particle Science and Technology, Institute of Frontier and Interdisciplinary Science, Shandong University, Qingdao 266237, Shandong, China.
  • Ning X; Key Laboratory of Particle Physics and Particle Irradiation of Ministry of Education, Shandong University, Qingdao 266237, Shandong, China.
  • Qi N; School of Physics, Peking University, Beijing 100871, China.
  • Qian Z; Department of Modern Physics, University of Science and Technology of China, Hefei 230026, China.
  • Ren X; School of Physics and Astronomy, Shanghai Jiao Tong University, Key Laboratory for Particle Astrophysics and Cosmology (MoE), Shanghai Key Laboratory for Particle Physics and Cosmology, Shanghai 200240, China.
  • Shang C; Key Laboratory of Nuclear Physics and Ion-beam Application (MOE), Institute of Modern Physics, Fudan University, Shanghai 200433, China.
  • Shang X; School of Physics, Peking University, Beijing 100871, China.
  • Shen G; Research Center for Particle Science and Technology, Institute of Frontier and Interdisciplinary Science, Shandong University, Qingdao 266237, Shandong, China.
  • Si L; Key Laboratory of Particle Physics and Particle Irradiation of Ministry of Education, Shandong University, Qingdao 266237, Shandong, China.
  • Sun W; School of Physics and Astronomy, Shanghai Jiao Tong University, Key Laboratory for Particle Astrophysics and Cosmology (MoE), Shanghai Key Laboratory for Particle Physics and Cosmology, Shanghai 200240, China.
Phys Rev Lett ; 129(16): 161803, 2022 Oct 14.
Article em En | MEDLINE | ID: mdl-36306747
Compared with the signature of dark matter elastic scattering off nuclei, the absorption of fermionic dark matter by nuclei opens up a new searching channel for light dark matter with a characteristic monoenergetic signal. In this Letter, we explore the 95.0-day data from the PandaX-4T commissioning run and report the first dedicated searching results of the fermionic dark matter absorption signal through a neutral current process. No significant signal was found, and the lowest limit on the dark matter-nucleon interaction cross section is set to be 1.5×10^{-50} cm^{2} for a fermionic dark matter mass of 40 MeV/c^{2} with 90% confidence level.
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Texto completo: 1 Coleções: 01-internacional Base de dados: MEDLINE Idioma: En Revista: Phys Rev Lett Ano de publicação: 2022 Tipo de documento: Article País de afiliação: China País de publicação: Estados Unidos
Texto completo
Adicionar na Minha BVS
Imprimir
XML
PubMed Links
Buscar no Google

Texto completo: 1 Coleções: 01-internacional Base de dados: MEDLINE Idioma: En Revista: Phys Rev Lett Ano de publicação: 2022 Tipo de documento: Article País de afiliação: China País de publicação: Estados Unidos