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New view of FAST telescope: Millisecond pulsars and gravitational waves probes
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Yungang ZHOU1, Dehua WANG1, *, Chengmin ZHANG2, 3, 4, *, Xianghan CUI2, 3, 4, Xinji WU5, Zhiyao YANG1, Shu MA1
Science & Technology Review | 2025, 43(5) : 45 - 54
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Science & Technology Review | 2025, 43(5): 45-54
Exclusive: Large-Scale Scientific Facilities
New view of FAST telescope: Millisecond pulsars and gravitational waves probes
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Yungang ZHOU1, Dehua WANG1, *, Chengmin ZHANG2, 3, 4, *, Xianghan CUI2, 3, 4, Xinji WU5, Zhiyao YANG1, Shu MA1
Affiliations
  • 1. School of Physics and Electronic Science, Guizhou Normal University, Guiyang 550025, China
  • 2. National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100101, China
  • 3. School of Physical Sciences, University of Chinese Academy of Sciences, Beijing 100049, China
  • 4. Key Laboratory of FAST, Chinese Academy of Sciences, Beijing 100101, China
  • 5. Department of Astronomy, Peking University, Beijing 100091, China
Published: 2025-03-13 doi: 10.3981/j.issn.1000-7857.2024.08.01001
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The discovery of millisecond pulsars has opened up a rich field for astrophysics. The FAST telescope plays an important role in the study of millisecond pulsars. This paper reviews the research progress of millisecond pulsars since their discovery 42 years ago, including their physical properties, formation and evolution, millisecond pulsar timing arrays and gravitational wave detection. The physical parameter distribution of millisecond pulsars is studied by statistical method, showing the unique properties of millisecond pulsars. In addition, this paper also introduces millisecond pulsars in globular clusters, which provides us with a new perspective on their evolution and helps to reveal the key process of pulsar evolution. With the advantages of FAST's high precision and high sensitivity, it is expected to discover new special types of pulsars and exotic objects from globular clusters in the future, e.g., double millisecond pulsar systems (MSP-MSP), millisecond pulsar-black hole systems (MSP-BH), and submillisecond pulsars, which will greatly enrich our analysis of neutron star types and characteristics. In addition, FAST will also play an important role in the detection of nanohertz gravitational waves, which will provide us with deeper insights into the universe and reveal more mysteries of the universe.

pulsar  /  neutron star  /  millisecond pulsar  /  gravitational wave  /  FAST telescope
Yungang ZHOU, Dehua WANG, Chengmin ZHANG, Xianghan CUI, Xinji WU, Zhiyao YANG, Shu MA. New view of FAST telescope: Millisecond pulsars and gravitational waves probes[J]. Science & Technology Review, 2025 , 43 (5) : 45 -54 . DOI: 10.3981/j.issn.1000-7857.2024.08.01001
Year 2025 volume 43 Issue 5
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Article Info
doi: 10.3981/j.issn.1000-7857.2024.08.01001
  • Receive Date:2024-08-13
  • Online Date:2025-06-29
  • Published:2025-03-13
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History
  • Received:2024-08-13
  • Revised:2024-09-26
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Affiliations
    1. School of Physics and Electronic Science, Guizhou Normal University, Guiyang 550025, China
    2. National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100101, China
    3. School of Physical Sciences, University of Chinese Academy of Sciences, Beijing 100049, China
    4. Key Laboratory of FAST, Chinese Academy of Sciences, Beijing 100101, China
    5. Department of Astronomy, Peking University, Beijing 100091, China
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表12种不同金属材料的力学参数

Family
属数
Number of
genus
种数
Number of
species
占总种数比例
Percentage of
total species (%)

Genus
种数
Number of
species
占总种数比例
Percentage of total
species (%)
鹅膏菌科Amanitaceae 2 11 5.26 鹅膏菌属 Amanita 10 4.78
小菇科 Mycenaceae 2 12 5.74 丝盖伞属 Inocybe 5 2.39
多孔菌科 Polyporaceae 8 14 6.70 蜡蘑属 Laccaria 5 2.39
红菇科 Russulaceae 3 23 11.00 小皮伞属 Marasmius 6 2.87
小菇属 Mycena 11 5.26
光柄菇属 Pluteus 5 2.39
红菇属 Russula 17 8.13
栓菌属 Trametes 5 2.39
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