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  5. Physics and astrophysics of strong magnetic field systems with eXTP
 

Physics and astrophysics of strong magnetic field systems with eXTP

Journal
SCIENCE CHINA. PHYSICS, MECHANICS & ASTRONOMY  
Date Issued
2019
Author(s)
Santangelo, Andrea
•
Zane, Silvia
•
Feng, Hua
•
Xu, RenXin
•
Doroshenko, Victor
•
Bozzo, Enrico
•
Caiazzo, Ilaria
•
Zelati, Francesco Coti
•
ESPOSITO, PAOLO  
•
González-Caniulef, Denis
•
Heyl, Jeremy
•
Huppenkothen, Daniela
•
ISRAEL, Gian Luca  
•
Li, ZhaoSheng
•
Lin, Lin
•
MIGNANI, Roberto  
•
Rea, Nanda
•
ORLANDINI, MAURO  
•
Taverna, Roberto
•
Tong, Hao
•
Turolla, Roberto
•
Baglio, Cristina
•
BERNARDINI, Federico  
•
BUCCIANTINI, NICCOLO'  
•
FEROCI, MARCO  
•
Fürst, Felix
•
Göğüș, Ersin
•
Güngör, Can
•
Ji, Long
•
Lu, FangJun
•
Manousakis, Antonios
•
MEREGHETTI, Sandro  
•
MIKUSINCOVA, Romana  
•
Paul, Biswajit
•
Prescod-Weinstein, Chanda
•
Younes, George
•
TIENGO, ANDREA  
•
Xu, YuPeng
•
Watts, Anna
•
Zhang, Shu
•
Zhan, Shuang-Nan
DOI
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.
Volume
62
Issue
2
Start page
29505
Uri
http://hdl.handle.net/20.500.12386/28831
Url
https://link.springer.com/article/10.1007/s11433-018-9234-3
Issn Identifier
1674-7348
Ads BibCode
2019SCPMA..6229505S
Rights
open.access
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Santangelo2018_Article_PhysicsAndAstrophysicsOfStrong.pdf

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eXTP.pdf

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