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

Abstract

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.

accepted for publication in the SCIENCE CHINA Physics, Mechanics & Astronomy

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• Fast and Luminous Transients from the Explosions of Long Lived Massive White Dwarf Merger Remnants
• Examining High Energy Radiation Mechanisms of Knots and Hotspots in Active Galactic Nucleus Jets
• Probing Magnetic Fields of GRB X-ray Flares with Polarization Observations
• Joint Observations of Space-based Gravitational-wave Detectors: Source Localization and Implication for Parity-violating gravity
• X-ray fluorescence from super-Eddington accreting black holes
• A highly magnetized long-period radio transient exhibiting unusual emission features
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• Discussions on the nature of GLEAM-X J162759.5-523504.3
• Kilonova and Optical Afterglow from Binary Neutron Star Mergers. II. Optimal Search Strategy for Serendipitous Observations and Target-of-opportunity Observations of Gravitational-wave Triggers
• Electromagnetic Follow-up Observations of Binary Neutron Star Mergers with Early Warnings from Decihertz Gravitational-wave Observatories
• Testing the binary black hole paradigm through the Fe Kalpha line profile: application to 3C 273
• Discovery of the linear energy-dependence of the spectral lag of X-ray bursts from SGR J1935+2154
• Resolving phase transition properties of dense matter through tidal-excited g-mode from inspiralling neutron stars
• Rates of Stellar Tidal Disruption Events around Intermediate-Mass Black Holes
• Polarization of GRB Prompt Emission and its Application to POLAR's Data
• The effects of a magnetar engine on the gamma-ray burst-associated supernovae: Application to double-peaked SN 2006aj
• Recent progresses in strange quark stars
• Search for gravitational waves emitted from SN 2023ixf
• CHIME/FRB Discovery of an Unusual Circularly Polarized Long-Period Radio Transient with an Accelerating Spin Period
• GRB X-Ray Flare Properties among Different GRB Subclasses
• Possible origin of AT2021any: a failed GRB from a structured jet
• Simultaneous Radio and Optical Polarimetry of GRB 191221B Afterglow
• Chandra Imaging of the Western Hotspot in the Radio Galaxy Pictor A: Image Deconvolution and Variability Analysis
• Rotation of polarization angle in gamma-ray burst prompt phase
• Precession of magnetars: dynamical evolutions and modulations on polarized electromagnetic waves
• Composite profile of the Fe K$\alpha$ spectral line emitted from a binary system of supermassive black holes
• Realistic Detection and Early Warning of Binary Neutron Stars with Decihertz Gravitational-wave Observatories
• Tidal torque induced by orbital decay in compact object binaries
• Determining the nature of white dwarfs from low-frequency gravitational waves
• Magnetar central engines in gamma-ray busts follow the universal relation of accreting magnetic stars
• Relativistic X-ray reverberation from super-Eddington accretion flow
• Probing nuclear physics with supernova gravitational waves and machine learning
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• FRB 171019: An event of binary neutron star merger?
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• Pulsar and Magnetar Navigation with Fermi/GBM and GECAM
• An X-ray study for white dwarf binary AR Scorpii
• Testing Models for the Shallow Decay Phase of Gamma-Ray Burst Afterglows with Polarization Observations
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