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Prospects for Time-Domain and Multi-Messenger Science with eXTP

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arxiv 2506.08368 v2 pith:I3LWBPSM submitted 2025-06-10 astro-ph.HE astro-ph.COastro-ph.GA

Prospects for Time-Domain and Multi-Messenger Science with eXTP

Shu-Xu Yi , Wen Zhao , Ren-Xin Xu , Xue-Feng Wu , Giulia Stratta , Simone Dall'Osso , Yan-Jun Xu , Andrea Santangelo
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Silvia Zane Shuang-Nan Zhang Hua Feng Huan Yang Junjie Mao Junqiang Ge Lijing Shao Mi-Xiang Lan He Gao Lin Lin Ning Jiang Qingwen Wu Tong Liu Yun-Wei Yu Xiang-Yu Wang Jin Zhang Dafne Guetta Jin-Jun Geng Di Xiao Yong-Feng Huang Yacheng Kang Tian-Yong Cao Zhen Zhang Zhenwei Lyu Zhen Pan Yunfeng Chen Yong Gao Ang Li Yu-Cong Fu Shuo Xiao Wei-Yang Wang Fayin Wang Zhenyin Zhao Weihua Lei Rong-Feng Shen Lixin Dai Guang-Lei Wu Liang-Duan Liu Bing Li Xilong Fan Xing-Jiang Zhu Youjun Lu Fan Xu Kangfa Cheng Da-Bin Lin Xiao-Hong Zhao Jun-Jie We Bin-Bin Zhang Ji-Rong Mao Yongquan Xue Xinwen Shu Wenjie Zhang Wei-Li Lin Achille Fiore Zhuo Li Antonio Martin-Carrillo Joseph Fisher Fei Xie Ye Li Sandro Mereghetti Shao-Lin Xiong Yu-Han Yang Eleonora Troja Zi-Gao Dai Da-Ming We En-Wei Liang J.E. Horvath G. R. Cunha Sampaio L.G. Barao L. M. de Sa
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classification astro-ph.HE astro-ph.COastro-ph.GA
keywords extpmulti-messengertime-domainadvantagesburstsenergyhighincluding
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In this new era of time-domain and multi-messenger astronomy, various new transients and new phenomena are constantly being discovered thanks to the rapid advances in observations, which provide the excellent opportunity to study the physics in the extreme environments. The enhanced X-ray Timing and Polarimetry mission (eXTP), planned to be launched in 2030, has several key advantages, including advanced polarimetry, high sensitivity & large effective area, and wide energy range coverage, which make it a groundbreaking project in high-energy astrophysics. In this article, we briefly introduce the potential time-domain and multi-messenger targets for eXTP, including gravitational-wave (GW) counterparts, gamma-ray bursts (GRBs), magnetars and fast radio bursts (FRBs), tidal disruption events (TDEs), supernovae, high energy neutrinos and TeV active galactic nucleus (AGNs), and so on. We discuss the advantages of future eXTP observations for detecting these sources, their detection capabilities, the abilities to distinguish theoretical models, and their applications in gravity and cosmology.

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Cited by 1 Pith paper

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  1. Physics and Astrophysics of Black Holes with eXTP

    astro-ph.HE 2026-07 accept novelty 2.0

    eXTP’s larger effective area and simultaneous polarimetry will tighten black-hole spin and Kerr-deviation constraints relative to NICER for the same exposure.