中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
首页 机构 成果 学者
  
  1. CAS IR Grid
  2. 云南天文台
  3. 中国科学院云南天文台
  4. 星系类星体研究组
Prospects for time-domain and multi-messenger science with eXTP

文献类型：期刊论文

作者Yi, Shu-Xu10; Zhao, Wen11; Xu, Ren-Xin12,13; Wu, Xue-Feng14; Stratta, Giulia41; Dall’Osso, Simone40; Xu, Yan-Jun10; Santangelo, Andrea10,39; Zane, Silvia38; Zhang, Shuang-Nan10
刊名SCIENCE CHINA-PHYSICS MECHANICS & ASTRONOMY
出版日期2025-09-25
卷号68期号:11
关键词eXTP mission time-domain astronomy multi-messenger astronomy high-energy astrophysics
ISSN号1674-7348
DOI10.1007/s11433-025-2782-2
产权排序第33完成单位
文献子类Review
英文摘要In this new era of time-domain and multi-messenger astronomy, various new transients and new phenomena are constantly being discovered thanks to the rapid advances in observations, which provide the excellent opportunity to study the physics in the extreme environments. The enhanced X-ray Timing and Polarimetry mission (eXTP), planned to be launched in 2030, has several key advantages, including advanced polarimetry, high sensitivity & large effective area, and wide energy range coverage, which make it a groundbreaking project in high-energy astrophysics. In this article, we briefly introduce the potential time-domain and multi-messenger targets for eXTP, including gravitational-wave (GW) counterparts, gamma-ray bursts (GRBs), magnetars and fast radio bursts (FRBs), tidal disruption events (TDEs), supernovae, high energy neutrinos and TeV active galactic nucleus (AGNs), and so on. We discuss the advantages of future eXTP observations for detecting these sources, their detection capabilities, the abilities to distinguish theoretical models, and their applications in gravity and cosmology.
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GAMMA-RAY-BURST ; MASSIVE BLACK-HOLE ; TIDAL DISRUPTION EVENTS ; QUASI-PERIODIC OSCILLATIONS ; SOFT-X-RAY ; SELF-ORGANIZED CRITICALITY ; SUPER-EDDINGTON ACCRETION ; BLUE OPTICAL TRANSIENT ; FAST RADIO-BURSTS ; MINIMUM VARIATION TIMESCALES
资助项目China's Space Origins Exploration Program; Chinese Academy of Sciences[E32983U810]; National Natural Science Foundation of China[12325301]; National Natural Science Foundation of China[12233002]; National Natural Science Foundation of China[12041306]; National Natural Science Foundation of China[12333007]; National SKA Program of China[2020SKA0120300]; Strategic Priority Research Program of the Chinese Academy of Sciences[113111KYSB20190020]; Strategic Priority Research Program of the Chinese Academy of Sciences[XDB0550300]; Beijing Municipal Natural Science Foundation[1242032]; Youth Innovation Promotion Association of the Chinese Academy of Sciences[2022056]; National Key Research and Development Program of China[2022YFC2205201]; National Key Research and Development Program of China[2020YFC2201400]; European Union-NextGenerationEU[RFF M4C2 1.1]; European Union-NextGenerationEU[2022RJL-WHN URKA]; INAF 2023 Theory Grant[ObFu 1.05.23.06.06]
WOS研究方向Physics
语种英语
WOS记录号WOS:001585079900001
出版者SCIENCE PRESS
资助机构China's Space Origins Exploration Program ; Chinese Academy of Sciences[E32983U810] ; National Natural Science Foundation of China[12325301, 12233002, 12041306, 12333007] ; National SKA Program of China[2020SKA0120300] ; Strategic Priority Research Program of the Chinese Academy of Sciences[113111KYSB20190020, XDB0550300] ; Beijing Municipal Natural Science Foundation[1242032] ; Youth Innovation Promotion Association of the Chinese Academy of Sciences[2022056] ; National Key Research and Development Program of China[2022YFC2205201, 2020YFC2201400] ; European Union-NextGenerationEU[RFF M4C2 1.1, 2022RJL-WHN URKA] ; INAF 2023 Theory Grant[ObFu 1.05.23.06.06]
版本出版稿
源URL[http://ir.ynao.ac.cn/handle/114a53/28636]  
专题星系类星体研究组
通讯作者Yi, Shu-Xu; Zhao, Wen; Xu, Ren-Xin; Wu, Xue-Feng
作者单位1.Yunnan Observatories, Chinese Academy of Sciences, Kunming, 650011, China;
2.University of Chinese Academy of Sciences, Chinese Academy of Sciences, Beijing, 100049, China;
3.Universität Heidelberg, Zentrum für Astronomie (ZAH), Institut für Theoretische Astrophysik, Heidelberg, 69120, Germany
4.Astronomy Department, IAG-USP, São Paulo, SP, 05508-090, Brazil;
5.Department of Physics, University of Rome “Tor Vergata”, Rome, I-00133, Italy;
6.Max-Planck-Institut für Gravitationsphysik (Albert-Einstein-Institut), Potsdam-Golm, D-14476, Germany;
7.INAF-Istituto di Astrofisica Spaziale e Fisica Cosmica di Milano, Milano, 20133, Italy;
8.School of Physics and Centre for Space Research, University College Dublin, Belfield, D04 V1W8, Dublin, Ireland;
9.INAF-Osservatorio Astronomico di Padova, Padova, I-35122, Italy;
10.State Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, Chinese Academy of Sciences, Beijing, 100049, China;
推荐引用方式
GB/T 7714		 Yi, Shu-Xu,Zhao, Wen,Xu, Ren-Xin,et al. Prospects for time-domain and multi-messenger science with eXTP[J]. SCIENCE CHINA-PHYSICS MECHANICS & ASTRONOMY,2025,68(11).
APA Yi, Shu-Xu.,Zhao, Wen.,Xu, Ren-Xin.,Wu, Xue-Feng.,Stratta, Giulia.,...&Sá, L. M. de.(2025).Prospects for time-domain and multi-messenger science with eXTP.SCIENCE CHINA-PHYSICS MECHANICS & ASTRONOMY,68(11).
MLA Yi, Shu-Xu,et al."Prospects for time-domain and multi-messenger science with eXTP".SCIENCE CHINA-PHYSICS MECHANICS & ASTRONOMY 68.11(2025).

入库方式： OAI收割

来源：云南天文台

浏览0
下载0
收藏0
其他版本

除非特别说明，本系统中所有内容都受版权保护，并保留所有权利。