File Download

There are no files associated with this item.

  Links for fulltext
     (May Require Subscription)
Supplementary

Article: Probing the strong gravity region of black holes with eXTP

TitleProbing the strong gravity region of black holes with eXTP
Authors
Bu, QingcuiBambi, CosimoGou, LijunXu, YanjunUttley, Philde Rosa, AlessandraSantangelo, AndreaZane, SilviaFeng, HuaZhang, Shuang-NanJin, ChichuanPan, HaiwuShu, XinwenUrsini, FrancescoWang, YananWu, JianfengYou, BeiYuan, YefeiZhang, WendaBianchi, StefanoDai, LixinDi Salvo, TizianaDovčiak, MichalFeng, YuanGuo, HengxiaoIngram, AdamJiang, JiachenKaras, VladimírLi, DongyueLiu, HonghuiMasteroserio, GuglielmoMatt, GiorgioMotta, SaraMou, GuobinNosirov, AbdurakhmonPan, ZhenQiao, ErlinShen, RongfengShui, QingcangSong, YujiaSvoboda, JiříTao, LianVeledina, AlexandraYan, ZhenZhao, Tong
Keywordsactive galactic nuclei
black holes
stars
X-ray astronomy
X-ray binaries
X-ray polarimetry
Issue Date23-Sep-2025
PublisherSpringer
Citation
SCIENCE CHINA Physics, Mechanics and Astronomy, 2025, v. 68, n. 11, p. 1-30 How to Cite?
DOI: http://dx.doi.org/10.1007/s11433-025-2789-2
Abstract

We present the novel capabilities of the enhanced X-ray Timing and Polarimetry (eXTP) mission to study the strong gravity region around stellar-mass black holes in X-ray binary systems and supermassive black holes in active galactic nuclei. eXTP can combine X-ray spectral, timing, and polarimetric techniques to study the accretion process near black holes, measure black hole masses and spins, and test Einstein’s theory of General Relativity in the strong field regime. We show how eXTP can improve the current measurements of black holes of existing X-ray missions and we discuss the scientific questions that can be addressed.


Persistent Identifierhttp://hdl.handle.net/10722/369594
ISSN
1674-7348
2023 Impact Factor: 6.4
2023 SCImago Journal Rankings: 1.165

 

DC FieldValueLanguage
dc.contributor.authorBu, Qingcui-
dc.contributor.authorBambi, Cosimo-
dc.contributor.authorGou, Lijun-
dc.contributor.authorXu, Yanjun-
dc.contributor.authorUttley, Phil-
dc.contributor.authorde Rosa, Alessandra-
dc.contributor.authorSantangelo, Andrea-
dc.contributor.authorZane, Silvia-
dc.contributor.authorFeng, Hua-
dc.contributor.authorZhang, Shuang-Nan-
dc.contributor.authorJin, Chichuan-
dc.contributor.authorPan, Haiwu-
dc.contributor.authorShu, Xinwen-
dc.contributor.authorUrsini, Francesco-
dc.contributor.authorWang, Yanan-
dc.contributor.authorWu, Jianfeng-
dc.contributor.authorYou, Bei-
dc.contributor.authorYuan, Yefei-
dc.contributor.authorZhang, Wenda-
dc.contributor.authorBianchi, Stefano-
dc.contributor.authorDai, Lixin-
dc.contributor.authorDi Salvo, Tiziana-
dc.contributor.authorDovčiak, Michal-
dc.contributor.authorFeng, Yuan-
dc.contributor.authorGuo, Hengxiao-
dc.contributor.authorIngram, Adam-
dc.contributor.authorJiang, Jiachen-
dc.contributor.authorKaras, Vladimír-
dc.contributor.authorLi, Dongyue-
dc.contributor.authorLiu, Honghui-
dc.contributor.authorMasteroserio, Guglielmo-
dc.contributor.authorMatt, Giorgio-
dc.contributor.authorMotta, Sara-
dc.contributor.authorMou, Guobin-
dc.contributor.authorNosirov, Abdurakhmon-
dc.contributor.authorPan, Zhen-
dc.contributor.authorQiao, Erlin-
dc.contributor.authorShen, Rongfeng-
dc.contributor.authorShui, Qingcang-
dc.contributor.authorSong, Yujia-
dc.contributor.authorSvoboda, Jiří-
dc.contributor.authorTao, Lian-
dc.contributor.authorVeledina, Alexandra-
dc.contributor.authorYan, Zhen-
dc.contributor.authorZhao, Tong-
dc.date.accessioned2026-01-28T00:35:22Z-
dc.date.available2026-01-28T00:35:22Z-
dc.date.issued2025-09-23-
dc.identifier.citationSCIENCE CHINA Physics, Mechanics and Astronomy, 2025, v. 68, n. 11, p. 1-30-
dc.identifier.issn1674-7348-
dc.identifier.urihttp://hdl.handle.net/10722/369594-
dc.description.abstract<p>We present the novel capabilities of the enhanced X-ray Timing and Polarimetry (eXTP) mission to study the strong gravity region around stellar-mass black holes in X-ray binary systems and supermassive black holes in active galactic nuclei. eXTP can combine X-ray spectral, timing, and polarimetric techniques to study the accretion process near black holes, measure black hole masses and spins, and test Einstein’s theory of General Relativity in the strong field regime. We show how eXTP can improve the current measurements of black holes of existing X-ray missions and we discuss the scientific questions that can be addressed.<br></p>-
dc.languageeng-
dc.publisherSpringer-
dc.relation.ispartofSCIENCE CHINA Physics, Mechanics and Astronomy-
dc.subjectactive galactic nuclei-
dc.subjectblack holes-
dc.subjectstars-
dc.subjectX-ray astronomy-
dc.subjectX-ray binaries-
dc.subjectX-ray polarimetry-
dc.titleProbing the strong gravity region of black holes with eXTP-
dc.typeArticle-
dc.identifier.doi10.1007/s11433-025-2789-2-
dc.identifier.scopuseid_2-s2.0-105021315272-
dc.identifier.volume68-
dc.identifier.issue11-
dc.identifier.spage1-
dc.identifier.epage30-
dc.identifier.eissn1869-1927-
dc.identifier.issnl1869-1927-

Export via OAI-PMH Interface in XML Formats

OR

Export to Other Non-XML Formats