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Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/7155
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dc.contributor.authorSantangelo, Andrea-
dc.contributor.authorZane, Silvia-
dc.contributor.authorPaul, Biswajit-
dc.contributor.author+ 36 Co-Authors-
dc.date.accessioned2019-02-12T18:12:24Z-
dc.date.available2019-02-12T18:12:24Z-
dc.date.issued2019-02-
dc.identifier.citationScience China Physics, Mechanics & Astronomy, 2019 Vol. 62, AR 029505en_US
dc.identifier.issn1674-7348-
dc.identifier.issn1869-1927 (Online)-
dc.identifier.urihttp://hdl.handle.net/2289/7155-
dc.descriptionRestricted Accessen_US
dc.description.abstractIn 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.en_US
dc.language.isoenen_US
dc.publisherScience China Pressen_US
dc.relation.urihttps://doi.org/10.1007/s11433-018-9234-3en_US
dc.relation.urihttps://arxiv.org/abs/1812.04460en_US
dc.rights⃝Science China Press and Springer-Verlag GmbH Germany, part of Springer Nature 2019en_US
dc.subjectneutron starsen_US
dc.subjectmagnetarsen_US
dc.subjectaccreting pulsarsen_US
dc.subjectAstrophysics - High Energy Astrophysical Phenomenaen_US
dc.titlePhysics and astrophysics of strong magnetic field systems with eXTPen_US
dc.typeArticleen_US
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