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Physics and astrophysics of strong magnetic field systems with eXTP

Santangelo, Andrea and Zane, Silvia and Feng, Hua and Xu, RenXin and Doroshenko, Victor and Bozzo, Enrico and Caiazzo, Ilaria and Zelati, Francesco Coti and Esposito, Paolo and Gonzalez-Caniulef, Denis and Heyl, Jeremy and Huppenkothen, Daniela and Israel, Gianluca and Li, ZhaoSheng and Lin, Lin and Mignani, Roberto and Rea, Nanda and Orlandini, Mauro and Taverna, Roberto and Tong, Hao and Turolla, Roberto and Baglio, Cristina and Bernardini, Federico and Bucciantini, Niccolo and Feroci, Marco and Furst, Felix and Göğüş, Ersin and Güngör, Can and Ji, Long and Lu, FangJun and Manousakis, Antonios and Mereghetti, Sandro and Mikusincova, Romana and Paul, Biswajit and Prescod-Weinstein, Chanda and Younes, George and Tiengo, Andrea and Xu, YuPeng and Watts, Anna and Zhang, Shu and Zhan, Shuang-Nan (2019) Physics and astrophysics of strong magnetic field systems with eXTP. Science China: Physics, Mechanics and Astronomy (SI), 62 (2). ISSN 1674-7348 (Print) 1869-1927 (Online)

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Official URL: http://dx.doi.org/10.1007/s11433-018-9234-3

Abstract

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.

Item Type:Article
Uncontrolled Keywords:neutron stars; QED; magnetars; accreting pulsars; eXTP
Subjects:Q Science > QB Astronomy > QB460-466 Astrophysics
ID Code:37412
Deposited By:Ersin Göğüş
Deposited On:26 Aug 2019 22:21
Last Modified:26 Aug 2019 22:21

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