TY - JOUR
T1 - Physics and astrophysics of strong magnetic field systems with eXTP
AU - Santangelo, Andrea
AU - Zane, Silvia
AU - Feng, Hua
AU - Xu, Ren Xin
AU - Doroshenko, Victor
AU - Bozzo, Enrico
AU - Caiazzo, Ilaria
AU - Zelati, Francesco Coti
AU - Esposito, Paolo
AU - González-Caniulef, Denis
AU - Heyl, Jeremy
AU - Huppenkothen, Daniela
AU - Israel, Gianluca
AU - Li, Zhao Sheng
AU - Lin, Lin
AU - Mignani, Roberto
AU - Rea, Nanda
AU - Orlandini, Mauro
AU - Taverna, Roberto
AU - Tong, Hao
AU - Turolla, Roberto
AU - Baglio, Cristina
AU - Bernardini, Federico
AU - Bucciantini, Niccolo’
AU - Feroci, Marco
AU - Fürst, Felix
AU - Göğüş, Ersin
AU - Güngör, Can
AU - Ji, Long
AU - Lu, Fang Jun
AU - Manousakis, Antonios
AU - Mereghetti, Sandro
AU - Mikusincova, Romana
AU - Paul, Biswajit
AU - Prescod-Weinstein, Chanda
AU - Younes, George
AU - Tiengo, Andrea
AU - Xu, Yu Peng
AU - Watts, Anna
AU - Zhang, Shu
AU - Zhan, Shuang Nan
N1 - Funding Information:
The Chinese team acknowledges the support of the Chinese Academy of Sciences through the Strategic Priority Research Program of the Chinese Academy of Sciences (Grant No. XDA15020100). This work was 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.2017-14-H.O is acknowledged.
Publisher Copyright:
© 2018, Science China Press and Springer-Verlag GmbH Germany, part of Springer Nature.
PY - 2019/2/1
Y1 - 2019/2/1
N2 - 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.
AB - 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.
KW - QED
KW - accreting pulsars
KW - eXTP
KW - magnetars
KW - neutron stars
UR - http://www.scopus.com/inward/record.url?scp=85052732116&partnerID=8YFLogxK
UR - http://www.scopus.com/inward/citedby.url?scp=85052732116&partnerID=8YFLogxK
U2 - 10.1007/s11433-018-9234-3
DO - 10.1007/s11433-018-9234-3
M3 - Review article
AN - SCOPUS:85052732116
VL - 62
JO - Science in China, Series G: Physics Astronomy
JF - Science in China, Series G: Physics Astronomy
SN - 1674-7348
IS - 2
M1 - 29505
ER -