机构:
Nanjing Foreign Language Sch, Nanjing 210000, Jiangsu, Peoples R ChinaNanjing Foreign Language Sch, Nanjing 210000, Jiangsu, Peoples R China
Chen, Ruijie
[1
]
机构:
[1] Nanjing Foreign Language Sch, Nanjing 210000, Jiangsu, Peoples R China
来源:
3RD INTERNATIONAL FORUM ON GEOSCIENCE AND GEODESY
|
2021年
/
658卷
关键词:
EMISSION;
D O I:
10.1088/1755-1315/658/1/012053
中图分类号:
X [环境科学、安全科学];
学科分类号:
08 ;
0830 ;
摘要:
Cosmological observations indicate that most of the matter in the universe is dark matter. Dark matter is neither ordinary baryonic matter, nor composed of any known particles of the standard model. It does not interact electromagnetically but does interact via gravity that affects various aspects of the structure of the universe. Three complementary methods including direct detection, indirect detection and manmade dark matter in laboratory were applied by astronomers to identify dark matter. Meanwhile, some models such as axion and supersymmetric standard model were proposed to satisfy the existing observations. The nature of dark matter is still a mystery. This paper briefly introduced the background information of discovery of dark matter, and summarized the latest development of dark matter detection in recent years and the model theories of dark matter. It also discussed the current understanding of dark matter and dark energy.
机构:
Chinese Acad Sci, Key Lab Dark Matter & Space Astron, Purple Mt Observ, Nanjing 210023, Peoples R China
Univ Sci & Technol China, Sch Astron & Space Sci, Hefei 230026, Peoples R ChinaChinese Acad Sci, Key Lab Dark Matter & Space Astron, Purple Mt Observ, Nanjing 210023, Peoples R China
机构:
Johns Hopkins Univ, William H Miller III Dept Phys & Astron, 3400 North Charles St, Baltimore, MD 21218 USAJohns Hopkins Univ, William H Miller III Dept Phys & Astron, 3400 North Charles St, Baltimore, MD 21218 USA
Bernal, Jose Luis
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机构:
Caputo, Andrea
Sato-Polito, Gabriela
论文数: 0引用数: 0
h-index: 0
机构:
Johns Hopkins Univ, William H Miller III Dept Phys & Astron, 3400 North Charles St, Baltimore, MD 21218 USAJohns Hopkins Univ, William H Miller III Dept Phys & Astron, 3400 North Charles St, Baltimore, MD 21218 USA
Sato-Polito, Gabriela
论文数: 引用数:
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机构:
Mirocha, Jordan
Kamionkowski, Marc
论文数: 0引用数: 0
h-index: 0
机构:
Johns Hopkins Univ, William H Miller III Dept Phys & Astron, 3400 North Charles St, Baltimore, MD 21218 USAJohns Hopkins Univ, William H Miller III Dept Phys & Astron, 3400 North Charles St, Baltimore, MD 21218 USA