Dense Matter in Neutron Stars with eXTP
arXiv:2506.08104 · doi:10.1007/s11433-025-2761-4
Abstract
In this White Paper, we present the potential of the enhanced X-ray Timing and Polarimetry (eXTP) mission to constrain the equation of state of dense matter in neutron stars, exploring regimes not directly accessible to terrestrial experiments. By observing a diverse population of neutron stars - including isolated objects, X-ray bursters, and accreting systems - eXTP's unique combination of timing, spectroscopy, and polarimetry enables high-precision measurements of compactness, spin, surface temperature, polarimetric signals, and timing irregularity. These multifaceted observations, combined with advances in theoretical modeling, pave the way toward a comprehensive description of the properties and phases of dense matter from the crust to the core of neutron stars. Under development by an international Consortium led by the Institute of High Energy Physics of the Chinese Academy of Sciences, the eXTP mission is planned to be launched in early 2030.
accepted for publication in the SCIENCE CHINA Physics, Mechanics & Astronomy
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- Oblate Schwarzschild approximation for polarized radiation from rapidly rotating neutron stars
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- Role of the symmetry energy slope in neutron stars: exploring the model-dependency
- The Regulated NiCu Cycles with the new Cu(p,)Zn reaction rate and the Influence on Type-I X-Ray Bursts: GS 182624 Clocked Burster
- What can PSR J1640-4631 tell us about the internal physics of this neutron star?
- Evolution of accretion disc reflection spectra due to a Type I X-ray burst
- Measuring the Lense-Thirring Orbital Precession and the Neutron Star Moment of Inertia with Pulsars
- Pulse Profile Modeling of Thermonuclear Burst Oscillations I: The Effect of Neglecting Variability
- Nambu-Jona-Lasinio description of hadronic matter from a Bayesian approach
- Broad iron emission line and kilohertz quasi-periodic oscillations in the neutron star system 4U 1636-53
- Constraints on the Equation of State of Neutron Star Matter From Observations of Kilohertz QPOs
- Polarized radiation from an accretion shock in accreting millisecond pulsars using exact Compton scattering formalism
- Revisiting the post-glitch relaxation of the 2000 Vela glitch with the neutron star equation of states in the Brueckner and relativistic Brueckner theories
- Gapless neutron superfluidity can explain the late time cooling of transiently accreting neutron stars
- NinjaSat monitoring of Type-I X-ray bursts from the clocked burster SRGA J144459.2604207
- Scale symmetry and composition of compact star matter
- Detection of millihertz quasi-periodic oscillations in the low-mass X-ray binary 4U 1730--22 with NICER
- Pulse Profile Modelling of Thermonuclear Burst Oscillations II: Handling variability
- Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis
- Effects from Dark Matter Halos on X-ray Pulsar Pulse Profiles
- Quasi-simultaneous Integral, Swift, And Nustar Observations Of The New X-ray Clocked Burster 1rxsj180408.9-342058
- Pasta phases in neutron stars under strong magnetic fields
- Unexpected late-time temperature increase observed in two neutron star crust cooling sources -- XTE~J1701-462 and EXO~0748-676
- The Orbit and Companion of PSR J1622-0315: Variable Asymmetry and a Massive Neutron Star
- New insights into the quasi-periodic X-ray burster GS 0836-429
- Neutron star matter as a dilute solution of protons in neutrons
- Spectral analysis of the quiescent low-mass X-ray binary in the globular cluster M30
- The outer crust of a cold, non-accreting neutron star within the Quark-Meson Coupling (QMC) model
- The distance and internal composition of the neutron star in EXO 0748-676 with XMM-Newton
- A comprehensive study of type I (thermonuclear) bursts in the new transient SRGA J144459.2604207
- Evolution of Urca Pairs in the Crusts of Highly Magnetized Neutron Stars
- Exploring Waveform Variations among Neutron Star Ray-tracing Codes for Complex Emission Geometries
- A NICER View of Spectral and Profile Evolution for Three X-ray Emitting Millisecond Pulsars
- Detecting Hyperons in neutron stars -- a machine learning approach
- Exploring nuclear force with pulsar glitch observation
- Modelling polarized X-ray pulses from accreting millisecond pulsars with X-PSI, using different hot spot locations and shapes
- Investigating the neutron star physics through observations of several young pulsars in the dipole-field re-emergence scenario
- Constraints on the internal physics of neutron stars from the observational data of several young pulsars: the role of a power-law decaying dipole magnetic field
- Scaling relations for the uncertainty in neutron star radius inferred from pulse profile modelling: the effect of spin rate
- Neutron stars from crust to core within the Quark-meson coupling model
- Dark Matter Seeding in Neutron Stars
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- Equation-of-state-informed pulse profile modeling
- Bayesian Inference of Hybrid Star Properties from Future High-Precision Measurements of Their Radii
- Gravitational Redshift for Rapidly Rotating Neutron Stars
- How Neutron Star Observations Point Towards Exotic Matter: Existing Explanations and a Prospective Proposal
- Is The Trace Anomaly at its Minimum Value at Neutron Star Centers?
- Tracing the Trace Anomaly of Dense Matter inside Neutron Stars
- Quantifying the Information Gain from Future High-Precision Radius Measurements for Identifying Twin Neutron Stars
- Bayesian Inference of fine-features of dense matter EOS from future high-precision data of neutron star radii
- Multiwavelength Analysis of PSR J0437-4715 with Pulse Profile Modeling
- -mode Oscillations for Hyperons and H-dibaryons in Neutron Stars