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Physics and astrophysics of strong magnetic field systems with eXTP

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arxiv 1812.04460 v1 pith:Y7E5KAJL submitted 2018-12-11 astro-ph.HE

Andrea Santangelo , Silvia Zane , Hua Feng , RenXin Xu , Victor Doroshenko , Enrico Bozzo , Ilaria Caiazzo , Francesco Coti Zelati
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Paolo Esposito Denis González-Caniulef Jeremy Heyl Daniela Huppenkothen Gianluca Israel ZhaoSheng Li Lin Lin Roberto Mignani Nanda Rea Mauro Orlandini Roberto Taverna Hao Tong Roberto Turolla Cristina Baglio Federico Bernardini Niccoló Bucciantini Marco Feroci Felix Fürst Ersin Göğüş Can Güngör Long Ji FangJun Lu Antonios Manousakis Sandro Mereghetti Romana Mikusincova Biswajit Paul Chanda Prescod-Weinstein George Younes Andrea Tiengo YuPeng Xu Anna Watts Shu Zhang Shuang-Nan Zhan
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keywords extpphysicsastrophysicsmagnetizedmissionobjectspotentialpulsars
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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.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Proof of Concept Measurements of Laterally Graded Multilayers for Soft X-ray Spectropolarimetry

    astro-ph.IM 2026-07 conditional novelty 5.0 of 10

    Cr/Sc and W/B4C laterally graded multilayer mirrors modulate soft X-ray reflection with polarization angle, showing ~100% modulation at Brewster angle and ~80% at 30° incidence.

  2. Physics of Strong Magnetism with eXTP

    astro-ph.HE 2025-06 unverdicted novelty 3.0 of 10

    The eXTP mission's planned instruments would enable more sensitive X-ray polarization and timing observations of magnetars and accreting pulsars, potentially testing vacuum birefringence and probing magnetic field structures.

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