中国天眼新视角：毫秒脉冲星与引力波探针

周云刚; 王德华; 张承民; 崔翔翰; 吴鑫基; 杨智尧; 马书

doi:10.3981/j.issn.1000-7857.2024.08.01001

科技导报 >

2025 , Vol. 43 >Issue 5: 45 - 54

DOI: https://doi.org/10.3981/j.issn.1000-7857.2024.08.01001

特色专题：大科学装置

中国天眼新视角：毫秒脉冲星与引力波探针

周云刚 ^,¹ ,
王德华 ^,¹^,* ,
张承民 ^,²^,³^,⁴^,* ,
崔翔翰 ²^,³^,⁴ ,
吴鑫基 ⁵ ,
杨智尧 ¹ ,
马书 ¹

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1. 贵州师范大学物理与电子科学学院，贵阳 550025
2. 中国科学院国家天文台，北京 100101
3. 中国科学院大学物理科学学院，北京 100049
4. 中国科学院 FAST 重点实验室，北京 100101
5. 北京大学天文系，北京 100091

王德华(通信作者)，教授，研究方向为MSP与低质量X射线双星，电子信箱：wangdh@gznu.edu.cn

张承民(共同通信作者)，研究员，研究方向为脉冲星与中子星天体物理，电子信箱：zhangcm@bao.ac.cn

周云刚，硕士研究生，研究方向为中子星与MSP，电子信箱：222100070261@gznu.edu.cn

收稿日期: 2024-08-13

网络出版日期: 2025-04-11

基金资助

国家自然科学基金项目(12163001)

国家自然科学基金项目(12463007)

国家自然科学天文联合基金项目(U1938117)

贵州师范大学学术新苗基金项目(黔师新苗〔2022〕5号)

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New view of FAST telescope: Millisecond pulsars and gravitational waves probes

Yungang ZHOU ^,¹ ,
Dehua WANG ^,¹^,* ,
Chengmin ZHANG ^,²^,³^,⁴^,* ,
Xianghan CUI ²^,³^,⁴ ,
Xinji WU ⁵ ,
Zhiyao YANG ¹ ,
Shu MA ¹

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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

Received date: 2024-08-13

Online published: 2025-04-11

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摘要

综述了自毫秒脉冲星发现42年以来的研究进展，包括其物理性质、形成与演化、毫秒脉冲星计时阵列与引力波探测等方面的构想与新进展。介绍了球状星团中的毫秒脉冲星，这为认识它的演化提供了新的视角，并且有助于揭示脉冲星演化的关键过程。凭借FAST的高精度和高灵敏度优势，有望在未来从球状星团中发现新的特殊类型脉冲星和奇异天体，如双毫秒脉冲星系统（MSP-MSP）、毫秒脉冲星—黑洞系统（MSP-BH）、亚毫秒脉冲星等，这将极大地丰富对中子星种类和特性的认识。此外，FAST还将在纳赫兹引力波的探测中发挥重要作用，这为认识宇宙提供更加深入的洞察，揭示更多的奥秘。

关键词： 脉冲星; 中子星; 毫秒脉冲星; 引力波; 中国天眼

本文引用格式

周云刚 , 王德华 , 张承民 , 崔翔翰 , 吴鑫基 , 杨智尧 , 马书 . 中国天眼新视角：毫秒脉冲星与引力波探针[J]. 科技导报, 2025 , 43(5) : 45 -54 . DOI: 10.3981/j.issn.1000-7857.2024.08.01001

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