WATTS, Anna L., WenFei YU, Juri POUTANEN, Shu ZHANG, Sudip BHATTACHARYYA, Slavko BOGDANOV, Long JI, Alessandro PATRUNO, Thomas E. RILEY, Pavel BAKALA, Altan BAYKAL, Federico BERNARDINI, Ignazio BOMBACI, Edward BROWN, Yuri CAVECCHI, Deepto CHAKRABARTY, Jérome CHENEVEZ, Nathalie DEGENAAR, Melania DEL SANTO, Tiziana DI SALVO, Victor DOROSHENKO, Maurizio FALANGA, Robert D. FERDMAN, Marco FEROCI, Angelo F. GAMBINO, MingYu GE, Svenja K. GREIF, Sebastien GUILLOT, Can GUNGOR, Dieter H. HARTMANN, Kai HEBELER, Alexander HEGER, Jeroen HOMAN, Rosario IARIA, Jean IN ’T ZAND, Oleg KARGALTSEV, Aleksi KURKELA, XiaoYu LAI, Ang LI, XiangDong LI, ZhaoSheng LI, Manuel LINARES, FangJun LU, Simin MAHMOODIFAR, Mariano MÉNDEZ, Coleman MILLER, Sharon MORSINK, Joonas NATTILA, Andrea POSSENTI, Chand PRESCOD-WEINSTEIN, JinLu QU, Alessandro RIGGIO, Tuomo SALMI, Andrea SANNA, Andrea SANTANGELO, Hendrik SCHATZ, Achim SCHWENK, LiMing SONG, Eva ŠRÁMKOVÁ, Benjamin STAPPERS, Holger STIELE, Tod STROHMAYER, Ingo TEWS, Laura TOLOS, Gabriel TÖRÖK, David TSANG, Martin URBANEC, Andrea VACCHI, RenXin XU, YuPeng XU, Silvia ZANE, GuoBao ZHANG, ShuangNan ZHANG, WenDa ZHANG, ShiJie ZHENG and Xia ZHOU. Dense matter with eXTP. Science China. Physics, Mechanics & Astronomy. 2019, vol. 62, No 2, p. "029503-1"-"029503-17", 17 pp. ISSN 1674-7348. Available from: https://dx.doi.org/10.1007/s11433-017-9188-4.
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Basic information
Original name Dense matter with eXTP
Authors WATTS, Anna L., WenFei YU, Juri POUTANEN, Shu ZHANG, Sudip BHATTACHARYYA, Slavko BOGDANOV, Long JI, Alessandro PATRUNO, Thomas E. RILEY, Pavel BAKALA (203 Czech Republic, belonging to the institution), Altan BAYKAL, Federico BERNARDINI, Ignazio BOMBACI, Edward BROWN, Yuri CAVECCHI, Deepto CHAKRABARTY, Jérome CHENEVEZ, Nathalie DEGENAAR, Melania DEL SANTO, Tiziana DI SALVO, Victor DOROSHENKO, Maurizio FALANGA (756 Switzerland), Robert D. FERDMAN, Marco FEROCI, Angelo F. GAMBINO, MingYu GE, Svenja K. GREIF, Sebastien GUILLOT, Can GUNGOR, Dieter H. HARTMANN, Kai HEBELER, Alexander HEGER, Jeroen HOMAN, Rosario IARIA, Jean IN ’T ZAND, Oleg KARGALTSEV, Aleksi KURKELA, XiaoYu LAI, Ang LI, XiangDong LI, ZhaoSheng LI, Manuel LINARES, FangJun LU, Simin MAHMOODIFAR, Mariano MÉNDEZ, Coleman MILLER, Sharon MORSINK, Joonas NATTILA, Andrea POSSENTI, Chand PRESCOD-WEINSTEIN, JinLu QU, Alessandro RIGGIO, Tuomo SALMI, Andrea SANNA, Andrea SANTANGELO, Hendrik SCHATZ, Achim SCHWENK, LiMing SONG, Eva ŠRÁMKOVÁ (203 Czech Republic, belonging to the institution), Benjamin STAPPERS, Holger STIELE, Tod STROHMAYER, Ingo TEWS, Laura TOLOS, Gabriel TÖRÖK (203 Czech Republic, belonging to the institution), David TSANG, Martin URBANEC (203 Czech Republic, belonging to the institution), Andrea VACCHI, RenXin XU, YuPeng XU, Silvia ZANE, GuoBao ZHANG, ShuangNan ZHANG, WenDa ZHANG, ShiJie ZHENG and Xia ZHOU.
Edition Science China. Physics, Mechanics & Astronomy, 2019, 1674-7348.
Other information
Original language English
Type of outcome Article in a journal
Field of Study 10308 Astronomy
Country of publisher China
Confidentiality degree is not subject to a state or trade secret
WWW URL
RIV identification code RIV/47813059:19240/19:A0000557
Organization unit Faculty of Philosophy and Science in Opava
Doi http://dx.doi.org/10.1007/s11433-017-9188-4
UT WoS 000452406800001
Keywords in English Enhanced X-ray Timing and Polarimetry (eXTP) mission; dense matter; neutron stars; equation of state; accretion flows
Tags , HighlyCitedPaper, RCCPDP, RIVOK
Tags International impact, Reviewed
Changed by Changed by: Ing. Petra Skoumalová, učo 50554. Changed: 21/4/2020 11:42.
Abstract
In this White Paper we present the potential of the Enhanced X-ray Timing and Polarimetry (eXTP) mission for determining the nature of dense matter; neutron star cores host an extreme density regime which cannot be replicated in a terrestrial laboratory. The tightest statistical constraints on the dense matter equation of state will come from pulse profile modelling of accretion-powered pulsars, burst oscillation sources, and rotation-powered pulsars. Additional constraints will derive from spin measurements, burst spectra, and properties of the accretion flows in the vicinity of the neutron star. Under development by an international Consortium led by the Institute of High Energy Physics of the Chinese Academy of Sciences, the eXTP mission is expected to be launched in the mid 2020s.
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