Physics and astrophysics of strong magnetic field systems with eXTP

Tarih
2019
Yazar
Gogus, Ersin
LU, FangJun
BERNARDINI, Federico
BUCCIANTINI, Niccolo'
FEROCI, Marco
FURST, Felix
JI, Long
Prescod-Weinstein, Chanda
SANTANGELO, Andrea
Zane, Silvia
FENG, Hua
XU, RenXin
DOROSHENKO, Victor
BOZZO, Enrico
PAUL, Biswajit
MIKUSINCOVA, Romana
MEREGHETTI, Sandro
Gungor, Can
MANOUSAKIS, Antonios
Caiazzo, Ilaria
ZELATI, Francesco Coti
ESPOSITO, Paolo
Gonzalez-Caniulef, Denis
Heyl, Jeremy
Huppenkothen, Daniela
ISRAEL, Gianluca
LI, ZhaoSheng
LIN, Lin
MIGNANI, Roberto
Younes, George
TIENGO, Andrea
XU, YuPeng
WATTS, Anna
ZHANG, Shu
ZHAN, Shuang-Nan
REA, Nanda
ORLANDINI, Mauro
TAVERNA, Roberto
TONG, Hao
Turolla, Roberto
BAGLIO, Cristina
Üst veri
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Özet
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.
Bağlantı
http://hdl.handle.net/20.500.12627/85496
https://doi.org/10.1007/s11433-018-9234-3
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