pith. machine review for the scientific record. sign in

arxiv: 1812.04020 · v1 · submitted 2018-12-10 · 🌌 astro-ph.IM · astro-ph.HE

Recognition: unknown

The enhanced X-ray Timing and Polarimetry mission - eXTP

ShuangNan Zhang , Andrea Santangelo , Marco Feroci , Yupeng Xu , Fangjun Lu , Yong Chen , Hua Feng , Shu Zhang
show 141 more authors
S{\o}ren Brandt Margarita Hernanz Luca Baldini Enrico Bozzo Riccardo Campana Alessandra De Rosa Yongwei Dong Yuri Evangelista Vladimir Karas Norbert Meidinger Aline Meuris Kirpal Nandra Teng Pan Giovanni Pareschi Piotr Orleanski Qiushi Huang Stephane Schanne Giorgia Sironi Daniele Spiga Jiri Svoboda Gianpiero Tagliaferri Christoph Tenzer Andrea Vacchi Silvia Zane Dave Walton Zhanshan Wang Berend Winter Xin Wu Jean J.M. in 't Zand Mahdi Ahangarianabhari Giovanni Ambrosi Filippo Ambrosino Marco Barbera Stefano Basso J\"org Bayer Ronaldo Bellazzini Pierluigi Bellutti Bruna Bertucci Giuseppe Bertuccio Giacomo Borghi XueLei Cao Franck Cadoux Francesco Ceraudo Tianxiang Chen YuPeng Chen Jerome Chevenez Marta Civitani Wei Cui Weiwei Cui Thomas Dauser Ettore Del Monte Sergio Di Cosimo Sebastian Diebold Victor Doroshenko Michal Dovciak YuanYuan Du Lorenzo Ducci Qingmei Fan Yannick Favre Fabio Fuschino Jos\'e Luis G\'alvez Min Gao Mingyu Ge Olivier Gevin Marco Grassi QuanYing Gu YuDong Gu DaWei Han Bin Hong Wei Hu Long Ji Shumei Jia WeiChun Jiang Thomas Kennedy Ingo Kreykenbohm Irfan Kuvvetli Claudio Labanti Luca Latronico Gang Li MaoShun Li Xian Li Wei Li Zhengwei Li Olivier Limousin Hongwei Liu Xiaojing Liu Bo Lu Tao Luo Daniele Macera Piero Malcovati Adrian Martindale Malgorzata Michalska Bin Meng Massimo Minuti Alfredo Morbidini Fabio Muleri Stephane Paltani Emanuele Perinati Antonino Picciotto Claudio Piemonte JinLu Qu Alexandre Rachevski Irina Rashevskaya Jerome Rodriguez Thomas Schanz Zhengxiang Shen LiZhi Sheng JiangBo Song Liming Song Carmelo Sgro Liang Sun Ying Tan Phil Uttley Juan Wang LangPing Wang Yusa Wang Anna L. Watts XiangYang Wen J\"orn Wilms Shaolin Xiong Jiawei Yang Sheng Yang YanJi Yang Nian Yu Wenda Zhang Gianluigi Zampa Nicola Zampa Andrzej A. Zdziarski AiMei Zhang Chengmo Zhang Fan Zhang Long Zhang Tong Zhang Yi Zhang Xiaoli Zhang ZiLiang Zhang BaoSheng Zhao Shijie Zheng Yupeng Zhou Nicola Zorzi J. Frans Zwart
Authors on Pith no claims yet
classification 🌌 astro-ph.IM astro-ph.HE
keywords missionextpwilldensityenhancedfundamentalgravitymatter
0
0 comments X
read the original abstract

In this paper we present the enhanced X-ray Timing and Polarimetry mission - eXTP. eXTP is a space science mission designed to study fundamental physics under extreme conditions of density, gravity and magnetism. The mission aims at determining the equation of state of matter at supra-nuclear density, measuring effects of QED, and understanding the dynamics of matter in strong-field gravity. In addition to investigating fundamental physics, eXTP will be a very powerful observatory for astrophysics that will provide observations of unprecedented quality on a variety of galactic and extragalactic objects. In particular, its wide field monitoring capabilities will be highly instrumental to detect the electro-magnetic counterparts of gravitational wave sources. The paper provides a detailed description of: (1) the technological and technical aspects, and the expected performance of the instruments of the scientific payload; (2) the elements and functions of the mission, from the spacecraft to the ground segment.

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.

Forward citations

Cited by 2 Pith papers

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

  1. Detectability of Magnetar-Induced Vacuum Birefringence with IXPE and eXTP

    hep-ph 2026-05 unverdicted novelty 4.0

    Vacuum birefringence time delays from magnetars are an order of magnitude larger than previous estimates and should be quantitatively measurable by IXPE and eXTP, especially for 1RXS J170849.0-400910.

  2. Polarization Signatures from GRMHD Simulations of Black Hole Accretion

    astro-ph.HE 2026-05 unverdicted novelty 2.0

    Polarization signatures from GRMHD simulations of black hole accretion can help probe disk, corona, and jet properties when combined with X-ray polarimetry observations.