CERN Accelerating science

Published Articles
Title Dense matter with eXTP
Author(s) Watts, Anna L (Amsterdam U., Astron. Inst.) ; Yu, WenFei (Shanghai, Astron. Observ.) ; Poutanen, Juri (Tuorla Observ. ; Nordita) ; Zhang, Shu (Beijing, Inst. High Energy Phys.) ; Bhattacharyya, Sudip (Tata Inst.) ; Bogdanov, Slavko (Columbia U., Astron. Astrophys.) ; Ji, Long (Tubingen U., IAAT) ; Patruno, Alessandro (Leiden Observ.) ; Riley, Thomas E (Amsterdam U., Astron. Inst.) ; Bakala, Pavel (Silesian U., Czech Republic) ; Baykal, Altan (Middle East Tech. U., Ankara) ; Bernardini, Federico (Rome Observ. ; New York U., Abu Dhabi) ; Bombaci, Ignazio (Pisa U.) ; Brown, Edward (Michigan State U.) ; Cavecchi, Yuri (Princeton U., Astrophys. Sci. Dept. ; U. Southampton (main)) ; Chakrabarty, Deepto (MIT, MKI) ; Chenevez, Jérôme (Denmark, Tech. U.) ; Degenaar, Nathalie (Amsterdam U., Astron. Inst.) ; Santo, Melania (IASF, Palermo) ; Salvo, Tiziana (Palermo U.) ; Doroshenko, Victor (Tubingen U., IAAT) ; Falanga, Maurizio (ISSI, Bern) ; Ferdman, Robert D (East Anglia U.) ; Feroci, Marco (INAF, IAPS, Rome) ; Gambino, Angelo F (Palermo U.) ; Ge, MingYu (Beijing, Inst. High Energy Phys.) ; Greif, Svenja K (Darmstadt, Tech. U. ; Darmstadt, EMMI) ; Guillot, Sebastien (Pontificia U. Catol. Chile, Santiago) ; Gungor, Can (Beijing, Inst. High Energy Phys.) ; Hartmann, Dieter H (Clemson U.) ; Hebeler, Kai (Darmstadt, Tech. U. ; Darmstadt, EMMI) ; Heger, Alexander (Monash U.) ; Homan, Jeroen (MIT, MKI) ; Iaria, Rosario (Palermo U.) ; in't Zand, Jean (SRON, Utrecht) ; Kargaltsev, Oleg (George Washington U.) ; Kurkela, Aleksi (CERN ; Stavanger U.) ; Lai, XiaoYu (Hubei U. Educ.) ; Li, Ang (Xiamen U.) ; Li, XiangDong (Nanjing U. (main)) ; Li, ZhaoSheng (Xiangtan U.) ; Linares, Manuel (Barcelona, Polytechnic U.) ; Lu, FangJun (Beijing, Inst. High Energy Phys.) ; Mahmoodifar, Simin (NASA, Goddard) ; Méndez, Mariano (Kapteyn Astron. Inst., Groningen) ; Coleman Miller, M (Maryland U., College Park) ; Morsink, Sharon (Alberta U.) ; Nättilä, Joonas (Tuorla Observ. ; Nordita) ; Possenti, Andrea (Cagliari Observ.) ; Prescod-Weinstein, Chanda (Washington U., Seattle) ; Qu, JinLu (Beijing, Inst. High Energy Phys.) ; Riggio, Alessandro (Cagliari U.) ; Salmi, Tuomo (Tuorla Observ.) ; Sanna, Andrea (Cagliari U.) ; Santangelo, Andrea (Tubingen U., IAAT ; Beijing, Inst. High Energy Phys.) ; Schatz, Hendrik (Michigan State U., JINA) ; Schwenk, Achim (Darmstadt, Tech. U. ; Darmstadt, EMMI ; Heidelberg, Max Planck Inst.) ; Song, LiMing (Beijing, Inst. High Energy Phys.) ; Šrámková, Eva (Silesian U., Czech Republic) ; Stappers, Benjamin (Jodrell Bank) ; Stiele, Holger (Taiwan, Natl. Tsing Hua U.) ; Strohmayer, Tod (NASA, Goddard) ; Tews, Ingo (Washington U., Seattle ; Michigan State U., JINA) ; Tolos, Laura (Barcelona, IEEC ; Frankfurt U. ; Frankfurt U., FIAS) ; Török, Gabriel (Silesian U., Czech Republic) ; Tsang, David (U. Southampton (main)) ; Urbanec, Martin (Silesian U., Czech Republic) ; Vacchi, Andrea (Udine U. ; INFN, Trieste) ; Xu, RenXin (Peking U., SKLNPT) ; Xu, YuPeng (Beijing, Inst. High Energy Phys.) ; Zane, Silvia (Mullard Space Sci. Lab.) ; Zhang, GuoBao (Yunnan Observ.) ; Zhang, ShuangNan (Beijing, Inst. High Energy Phys.) ; Zhang, WenDa (Charles U., Astro. Inst.) ; Zheng, ShiJie (Beijing, Inst. High Energy Phys.) ; Zhou, Xia (Urumqi Astron. Observ.)
Publication 2019
In: Sci. China Phys. Mech. Astron. 62 (2019) 29503
DOI 10.1007/s11433-017-9188-4
Subject category Astrophysics and Astronomy
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.

Corresponding record in: Inspire


 Journalen skapades 2019-04-13, och modifierades senast 2022-01-14