Physics and astrophysics of strong magnetic field systems with eXTP

查看全文 作　　者：Andrea [1,2]Santangelo;Silvia [3]Zane;Hua [4]Feng;RenXin [5]Xu;Victor [1]Doroshenko;Enrico [6]Bozzo;Ilaria [7]Caiazzo;Francesco Coti [8,9,10]Zelati;Paolo [9]Esposito;Denis González-[3]Caniulef;Jeremy [7]Heyl;Daniela [11]Huppenkothen;Gianluca [12]Israel;ZhaoSheng [13]Li;Lin [14]Lin;Roberto [15,16]Mignani;Nanda [17,9]Rea;Mauro [18]Orlandini;Roberto [19,20]Taverna;Hao [3,19]Tong;Roberto [21]Turolla;Cristina [21]Baglio;Federico [22]Bernardini;Niccolo'[23,24]Bucciantini;Marco [25]Feroci;Felix [26]Fürst;Ersin G??ü?[2];Can [1]Güngör;Long [2]Ji;FangJun [27,28]Lu;Antonios [15]Manousakis;Sandro [29]Mereghetti;Romana [30]Mikusincova;Biswajit [31]Paul;Chanda Prescod-[32]Weinstein;George [33]Younes;Andrea [2]Tiengo;YuPeng [2]Xu;Anna [9]Watts;Shu [2]Zhang;Shuang-Nan [2]Zhang

机构地区：[1]Institut für Astronomie und Astrophysik,Eberhard Karls Universität;[2]Key Laboratory for Particle Astrophysics,Institute of High Energy Physics;[3]Mullard Space Science Laboratory,University College London,Holmbury St Mary;[4]Department of Engineering Physics and Center for Astrophysics,Tsinghua University;[5]School of Physics,Peking University;[6]Department of Astronomy,University of Geneva;[7]Department of Physics and Astronomy,University of British Columbia;[8]Universitädell’Insubria;[9]Anton Pannekoek Institute for Astronomy,University of Amsterdam;[10]INAF-Osservatorio Astronomico di Brera;[11]Center for Data Science,New York University;[12]INAF-Osservatorio Astronomico di Roma;[13]Department of Physics,Xiangtan University;[14]Department of Astronomy,Beijing Normal University;[15]INAF-Istituto di Astrofisica Spaziale e Fisica Cosmica Milano;[16]Janusz Gil Institute of Astronomy,University of Zielona Góra;[17]Instituto de Ciencias del Espacio(ICE),CSIC-IEEC;[18]INAF-Istituto di Astrofisica Spaziale e Fisica Cosmica Bologna;[19]Department of Physics and Astronomy,University of Padova;[20]School of Physics and Electronic Engineering,Guangzhou University;[21]NYU Abu Dhabi,Saadiyat Campus P.O.;[22]NAF Osservatorio di Arcetri,Largo Enrico Fermi 5;[23]INAF-Istituto di Astrofisica e Planetologia Spaziali;[24]INFN-Roma Tor Vergata;[25]European Space Astronomy Centre(ESA/ESAC),Science Operations Department;[26]Sabanci University,Faculty of Engineering and Natural Sciences;[27]Centrum Astronomiczne im.M.Kopernika;[28]Department of Physics,Sultan Qaboos University;[29]Institute of Theoretical Physics,Faculty of Mathematics and Physics,Charles University in Prague;[30]Raman Research Institute Sadashivanagar;[31]Department of Astronomy,University of Washington;[32]The George Washington University Physics department 725 21st St NW;[33]Scuola Universitaria Superiore IUSS Pavia,Palazzo del Broletto

出　　处：《Science China(Physics,Mechanics & Astronomy)》索引2019年第62卷第2期,共23页

基　　金：support of the Chinese Academy of Sciences through the Strategic Priority Research Program of the Chinese Academy of Sciences(Grant No.XDA15020100);supported by the Bundesministerium fuer Wirtschaft und Technologie through the Deutsches Zentrum fuer Luft-und Raumfahrte.V.(DLR)(Grant No.FKZ 50 OO 1701);Financial contribution from the agreement between the Italian Space Agency and the Istituto Nazionale di Astrofisica ASI-INAF n.2017-14H.O 摘　　要：In this paper we present the science potential of the enhanced X-ray Timing and Polarimetry(eXTP) mission for studies of strongly magnetized objects. We will focus on the physics and astrophysics of strongly magnetized objects, namely magnetars, accreting X-ray pulsars, and rotation powered pulsars. We also discuss the science potential of eXTP for QED studies. Developed 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. 关键词：neutron stars QED MAGNETARS accreting pulsars eXTP

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Physics and astrophysics of strong magnetic field systems with eXTP

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