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Physics of strong magnetism with eXTP

文献类型：期刊论文

作者Ge, Mingyu24; Ji, Long25,26; Taverna, Roberto27; Tsygankov, Sergey28; Xu, Yanjun24; Santangelo, Andrea2,24,29; Zane, Silvia30; Zhang, Shuang-Nan24; Feng, Hua24; Chen, Wei31
刊名SCIENCE CHINA-PHYSICS MECHANICS & ASTRONOMY
出版日期2025-09-25
卷号68期号:11
关键词neutron stars QED magnetars accreting pulsars eXTP
ISSN号1674-7348
DOI10.1007/s11433-025-2796-y
产权排序第10完成单位
文献子类Review
英文摘要In this paper we present the science potential of the enhanced X-ray Timing and Polarimetry (eXTP) mission, in its new configuration, for studies of strongly magnetized compact objects. We discuss the scientific potential of eXTP for quantum electrodynamic (QED) studies, especially leveraging the recent observations made with the NASA IXPE mission. Given eXTP's unique combination of timing, spectroscopy, and polarimetry, we focus on the perspectives for physics and astrophysics studies of strongly magnetized compact objects, such as magnetars and accreting X-ray pulsars. Developed by an international Consortium led by the Institute of High Energy Physics of the Chinese Academy of Sciences, the eXTP mission is expected to launch in early 2030.
学科主题天文学 ; 恒星与银河系
URL标识查看原文
出版地16 DONGHUANGCHENGGEN NORTH ST, BEIJING 100717, PEOPLES R CHINA
WOS关键词X-RAY PULSAR ; ISOLATED NEUTRON-STARS ; FAST RADIO-BURSTS ; CENTRAL COMPACT OBJECT ; ROTATING VECTOR MODEL ; SOFT GAMMA-REPEATERS ; ANTI-GLITCH ; ACCRETING PULSAR ; CYCLOTRON LINE ; SPIN-DOWN
资助项目China's Space Origins Exploration Program; National Key R&D Program of China[2021YFA0718500]; National Natural Science Foundation of China[12373051]; National Natural Science Foundation of China[12273028]; National Natural Science Foundation of China[12173103]; National Natural Science Foundation of China[12261141691]; National Natural Science Foundation of China[12003009]; National Natural Science Foundation of China[12333007]; National Natural Science Foundation of China[12373041]; National Natural Science Foundation of China[12422306]; Italian MUR[PRIN 2022-2022LW-PEXW]; Italian MUR[CUP C53D23001180006]; German Research Foundation (DFG)[WE 1312/59-1]; UKRI Stephen Hawking fellowship; UKRI STFC[ST/W507891/1]; International Partnership Program of Chinese Academy of Sciences[113111KYSB20190020]; Strategic Priority Research Program of Chinese Academy of Sciences[XDA15020100]; Bagui Scholars Program; STFC[ST/Y001060/1]
WOS研究方向Physics
语种英语
WOS记录号WOS:001585079900002
出版者SCIENCE PRESS
资助机构China's Space Origins Exploration Program ; National Key R&D Program of China[2021YFA0718500] ; National Natural Science Foundation of China[12373051, 12273028, 12173103, 12261141691, 12003009, 12333007, 12373041, 12422306] ; Italian MUR[PRIN 2022-2022LW-PEXW, CUP C53D23001180006] ; German Research Foundation (DFG)[WE 1312/59-1] ; UKRI Stephen Hawking fellowship ; UKRI STFC[ST/W507891/1] ; International Partnership Program of Chinese Academy of Sciences[113111KYSB20190020] ; Strategic Priority Research Program of Chinese Academy of Sciences[XDA15020100] ; Bagui Scholars Program ; STFC[ST/Y001060/1]
版本出版稿
源URL[http://ir.ynao.ac.cn/handle/114a53/28637]  
专题星系类星体研究组
通讯作者Ge, Mingyu; Ji, Long; Taverna, Roberto; Tsygankov, Sergey
作者单位1.Yunnan Observatories, Chinese Academy of Sciences, Kunming, 650216, China;
2.Xinjiang Key Laboratory of Radio Astrophysics, Urumqi, 830011, China
3.Xinjiang Astronomical Observatory, Chinese Academy of Sciences, Urumqi, 830011, China;
4.Department of Astronomy, Huazhong University of Science and Technology, Wuhan, 430074, China;
5.Department of Physics and Institute of Theoretical Physics, Nanjing Normal University, Nanjing, 210023, China;
6.Department of Astronomy, School of Physics and Technology, Wuhan University, Wuhan, 430072, China;
7.School of Physical Science and Technology, Southwest Jiaotong University, Chengdu, 611756, China;
8.Department of Astronomy, Tsinghua University, Beijing, 100084, China;
9.School of Astronomy and Space Science, University of Science and Technology of China, Hefei, 230026, China;
10.Department of Astronomy, University of Science and Technology of China, Hefei, 230026, China;
推荐引用方式
GB/T 7714		 Ge, Mingyu,Ji, Long,Taverna, Roberto,et al. Physics of strong magnetism with eXTP[J]. SCIENCE CHINA-PHYSICS MECHANICS & ASTRONOMY,2025,68(11).
APA Ge, Mingyu.,Ji, Long.,Taverna, Roberto.,Tsygankov, Sergey.,Xu, Yanjun.,...&Zhou, Xia.(2025).Physics of strong magnetism with eXTP.SCIENCE CHINA-PHYSICS MECHANICS & ASTRONOMY,68(11).
MLA Ge, Mingyu,et al."Physics of strong magnetism with eXTP".SCIENCE CHINA-PHYSICS MECHANICS & ASTRONOMY 68.11(2025).

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来源：云南天文台

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