Dense matter with eXTP

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英文篇名：Dense matter with eXTP 作者：Anna ; L.Watts ; 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 ; Jér?me ; 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 ; KurkelaTheoretical ; Physics ; Department ; CERN ; XiaoYu ; Lai ; Ang ; Li ; XiangDong ; Li ; ZhaoSheng ; Li ; Manuel ; Linares ; FangJun ; Lu ; Simin ; Mahmoodifar ; Mariano ; Méndez ; M.Coleman ; Miller ; Sharon ; Morsink ; Joonas ; N?ttil? ; Andrea ; Possenti ; Chanda ; Prescod-Weinstein ; JinLu ; Qu ; Alessandro ; Riggio ; Tuomo ; Salmi ; Andrea ; Sanna ; Andrea ; Santangelo ; Hendrik ; Schatz ; Achim ; Schwenk ; LiMing ; Song ; Eva?rámková ; Benjamin ; Stappers ; Holger ; Stiele ; Tod ; Strohmayer ; Ingo ; Tews ; Laura ; Tolos ; Gabriel ; T?r?k ; David ; Tsang ; Martin ; Urbanec ; Andrea ; Vacchi ; RenXin ; Xu ; YuPeng ; Xu ; Silvia ; Zane ; GuoBao ; Zhang ; ShuangNan ; Zhang ; WenDa ; Zhang ; ShiJie ; Zheng ; Xia ; Zhou 英文作者：Anna L.Watts;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;Jér?me 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 KurkelaTheoretical Physics Department, CERN;XiaoYu Lai;Ang Li;XiangDong Li;ZhaoSheng Li;Manuel Linares;FangJun Lu;Simin Mahmoodifar;Mariano Méndez;M.Coleman Miller;Sharon Morsink;Joonas N?ttil?;Andrea Possenti;Chanda Prescod-Weinstein;JinLu Qu;Alessandro Riggio;Tuomo Salmi;Andrea Sanna;Andrea Santangelo;Hendrik Schatz;Achim Schwenk;LiMing Song;Eva?rámková;Benjamin Stappers;Holger Stiele;Tod Strohmayer;Ingo Tews;Laura Tolos;Gabriel T?r?k;David Tsang;Martin Urbanec;Andrea Vacchi;RenXin Xu;YuPeng Xu;Silvia Zane;GuoBao Zhang;ShuangNan Zhang;WenDa Zhang;ShiJie Zheng;Xia Zhou;Anton Pannekoek Institute for Astronomy, University of Amsterdam;Shanghai Astronomical Observatory;Tuorla Observatory, Department of Physics and Astronomy, University of Turku;Nordita, KTH Royal Institute of Technology and Stockholm University;Institute of High Energy Physics, Chinese Academy Sciences;Tata Institute of Fundamental Research;Columbia Astrophysics Laboratory, Columbia University;Institut für Astronomie und Astrophysik Tübingen, Universit?t Tübingen;Leiden Observatory, Leiden University;Research Center for Computational Physics and Data Processing, Silesian University in Opava;Physics Department, Middle East Technical University;INAF, Osservatorio Astronomico di Roma;New York University Abu Dhabi;Dipartimento di Fisica Enrico Fermi, University of Pisa;INFN Italian National Institute for Nuclear Physics;Department of Physics and Astronomy, Michigan State University;Department of Astrophysical Sciences, Princeton University;Mathematical Sciences and STAG Research Centre, University of Southampton;MIT Kavli Institute for Astrophysics and Space Research;DTU Space, Technical University of Denmark;INAF/IASF Palermo,via Ugo La Malfa 153;Universita degli Studi di Palermo, Dipartimento di Fisica e Chimica;International Space Science Institute (ISSI);Faculty of Science, University of East Anglia;INAF, Istituto di Astrofisica e Planetologie Spaziali;Institut für Kernphysik, Technische Universit?t Darmstadt;ExtreMe Matter Institute EMMI, GSI Helmholtzzentrum für Schwerionenforschung GmbH;Instituto de Astrof′?sica, Pontificia Universidad Católica de Chile;Department of Physics & Astronomy, Kinard Lab of Physics, Clemson University;School of Physics and Astronomy, Monash University;SRON Netherlands Institute for Space Research;Department of Physics, The George Washington University;Faculty of Science and Technology, University of Stavanger;School of Physics and Mechanical & Electrical Engineering, Hubei University of Education;Department of Astronomy, Xiamen University (Haiyun Campus);School of Astronomy and Space Science, Nanjing University;Department of Physics, Xiangtan University;Departament de F′?sica, EEBE, Universitat Politècnica de Catalunya;NASA’s Goddard Space Flight Center, Greenbelt;Kapteyn Astronomical Institute, University of Groningen;Department of Astronomy and Joint Space-Science Institute, University of Maryland;Department of Physics, University of Alberta;INAF, Osservatorio Astronomico di Cagliari;Department of Physics, University of Washington;Dipartimento di Fisica, Universita degli Studi di Cagliari;JINA Center for the Evolution of the Elements, National Superconducting Cyclotron Laboratory,Michigan State University;Max-Planck-Institut für Kernphysik, Saupfercheckweg 1;Jodrell Bank Centre for Astrophysics, School of Physics and Astronomy, The University of Manchester;Institute for Astronomy, National Tsing Hua University;Institute for Nuclear Theory, University of Washington,Seattle;Institute of Space Sciences, IEEC-CSIC, Carrer Can Magrans s/n;Institut für Theoretische Physik, Goethe-Universit?t Frankfurt;Frankfurt Institute for Advanced Studies;Department of Mathematics, Computer Science and Physics, University of Udine;INFN Italian National Institute for Nuclear Physics, Trieste Section;School of Physics, State Key Laboratory of Nuclear Physics and Technology, Peking University;Mullard Space Science Laboratory, University College London;Yunnan Observatory, Chinese Academy of Sciences;Astronomical Institute of the Academy of Sciences;Xinjiang Astronomical Observatory, Chinese Academy of Sciences; 英文关键词：neutron;;X-rays;;dense matter;;equation of state 中文刊名：JGXG 英文刊名：中国科学:物理学 力学 天文学(英文版) 机构：Anton Pannekoek Institute for Astronomy, University of Amsterdam;Shanghai Astronomical Observatory;Tuorla Observatory, Department of Physics and Astronomy, University of Turku;Nordita, KTH Royal Institute of Technology and Stockholm University;Institute of High Energy Physics, Chinese Academy Sciences;Tata Institute of Fundamental Research;Columbia Astrophysics Laboratory, Columbia University;Institut für Astronomie und Astrophysik Tübingen, Universit?t Tübingen;Leiden Observatory, Leiden University;Research Center for Computational Physics and Data Processing, Silesian University in Opava;Physics Department, Middle East Technical University;INAF, Osservatorio Astronomico di Roma;New York University Abu Dhabi;Dipartimento di Fisica Enrico Fermi, University of Pisa;INFN Italian National Institute for Nuclear Physics;Department of Physics and Astronomy, Michigan State University;Department of Astrophysical Sciences, Princeton University;Mathematical Sciences and STAG Research Centre, University of Southampton;MIT Kavli Institute for Astrophysics and Space Research;DTU Space, Technical University of Denmark;INAF/IASF Palermo,via Ugo La Malfa 153;Universita degli Studi di Palermo, Dipartimento di Fisica e Chimica;International Space Science Institute (ISSI);Faculty of Science, University of East Anglia;INAF, Istituto di Astrofisica e Planetologie Spaziali;Institut für Kernphysik, Technische Universit?t Darmstadt;ExtreMe Matter Institute EMMI, GSI Helmholtzzentrum für Schwerionenforschung GmbH;Instituto de Astrof′?sica, Pontificia Universidad Católica de Chile;Department of Physics & Astronomy, Kinard Lab of Physics, Clemson University;School of Physics and Astronomy, Monash University;SRON Netherlands Institute for Space Research;Department of Physics, The George Washington University;Faculty of Science and Technology, University of Stavanger;School of Physics and Mechanical & Electrical Engineering, Hubei University of Education;Department of Astronomy, Xiamen University (Haiyun Campus);School of Astronomy and Space Science, Nanjing University;Department of Physics, Xiangtan University;Departament de F′?sica, EEBE, Universitat Politècnica de Catalunya;NASA’s Goddard Space Flight Center, Greenbelt;Kapteyn Astronomical Institute, University of Groningen;Department of Astronomy and Joint Space-Science Institute, University of Maryland;Department of Physics, University of Alberta;INAF, Osservatorio Astronomico di Cagliari;Department of Physics, University of Washington;Dipartimento di Fisica, Universita degli Studi di Cagliari;JINA Center for the Evolution of the Elements, National Superconducting Cyclotron Laboratory,Michigan State University;Max-Planck-Institut für Kernphysik, Saupfercheckweg 1;Jodrell Bank Centre for Astrophysics, School of Physics and Astronomy, The University of Manchester;Institute for Astronomy, National Tsing Hua University;Institute for Nuclear Theory, University of Washington,Seattle;Institute of Space Sciences, IEEC-CSIC, Carrer Can Magrans s/n;Institut für Theoretische Physik, Goethe-Universit?t Frankfurt;Frankfurt Institute for Advanced Studies;Department of Mathematics, Computer Science and Physics, University of Udine;INFN Italian National Institute for Nuclear Physics, Trieste Section;School of Physics, State Key Laboratory of Nuclear Physics and Technology, Peking University;Mullard Space Science Laboratory, University College London;Yunnan Observatory, Chinese Academy of Sciences;Astronomical Institute of the Academy of Sciences;Xinjiang Astronomical Observatory, Chinese Academy of Sciences; 出版日期：2018-08-22 18:11 出版单位：Science China(Physics,Mechanics & Astronomy) 年：2019 期：v.62 基金：support from ERC Starting (Grant No. 639217 CSINEUTRONSTAR);; support from a Netherlands Organization for Scientific Research (NWO) Vidi Fellowship;; suported by the European Union Horizon 2020 research and innovation programme under the Marie Sklodowska-Curie Global Fellowship (Grant No. 703916);; supported in part by the DFG through Grant SFB 1245 and the ERC (Grant No. 307986 STRONGINT);; support of the Chinese Academy of Sciences through the Strategic Priority Research Program of the Chinese Academy of Sciences (Grant No. XDA15020100) 语种：英文; 页：JGXG201902003 页数：17 CN：02 ISSN：11-5849/N 分类号：32-48

摘要

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 2020 s.
        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 2020 s.

引文

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    1)The assumed fluxes are as follows:Sco X-1, 0.5-10 keV flux of 1.6×10-7erg/cm2/s[118]; Aql X-1, 0.5-10 keV flux of 3.3×10-9erg/cm2/s[119];XTE J1807–294, 0.5-10 keV flux of 1.7×10-10erg/cm2/s[120].