Insights into the equation of state of neutron-rich matter since GW170817
arXiv:2202.13191 · doi:10.1088/1742-6596/2340/1/012012
Abstract
The historical detection of gravitational waves emitted from the binary neutron star merger GW170817 has opened the new era of multi-messenger astronomy. Since then, many other significant discoveries -- both on heaven and earth -- are providing new clues into the behavior of neutron-rich matter. It is the goal of this article to illustrate how the remarkable progress made during the last few years is spearheading the field into the golden age of neutron-star physics.
9 pages, 5 figures, submitted to the proceedings of the XLIV Brazilian Workshop on Nuclear Physics
References in corpus (21)
- Shapiro delay measurement of a two solar mass neutron star
- PSR J0030+0451 Mass and Radius from NICER Data and Implications for the Properties of Neutron Star Matter
- A NICER View of PSR J0030+0451: Millisecond Pulsar Parameter Estimation
- Tidal Love numbers of neutron stars
- Constraining neutron star tidal Love numbers with gravitational wave detectors
- A NICER View of the Massive Pulsar PSR J0740+6620 Informed by Radio Timing and XMM-Newton Spectroscopy
- The Electromagnetic Counterpart of the Binary Neutron Star Merger LIGO/VIRGO GW170817. II. UV, Optical, and Near-IR Light Curves and Comparison to Kilonova Models
- Refined Mass and Geometric Measurements of the High-Mass PSR J0740+6620
- Light Curves of the Neutron Star Merger GW170817/SSS17a: Implications for R-Process Nucleosynthesis
- Relativistic theory of tidal Love numbers
- Accurate Determination of the Neutron Skin Thickness of Pb through Parity-Violation in Electron Scattering
- The Electromagnetic Counterpart of the Binary Neutron Star Merger LIGO/VIRGO GW170817. IV. Detection of Near-infrared Signatures of r-process Nucleosynthesis with Gemini-South
- Nuclear symmetry energy probed by neutron skin thickness of nuclei
- The Electromagnetic Counterpart of the Binary Neutron Star Merger LIGO/VIRGO GW170817. III. Optical and UV Spectra of a Blue Kilonova From Fast Polar Ejecta
- Neutron skin of 208Pb, nuclear symmetry energy, and the parity radius experiment
- Astrophysical Measurement of the Equation of State of Neutron Star Matter
- Neutron star mass and radius measurements from atmospheric model fits to X-ray burst cooling tail spectra
- Using Neutron Star Observations to Determine Crust Thicknesses, Moments of Inertia, and Tidal Deformabilities
- Constraining the High-Density Behavior of Nuclear Symmetry Energy with the Tidal Polarizability of Neutron Stars
- Covariant Density Functional Theory in Nuclear Physics and Astrophysics
- The Radius of PSR J0740+6620 from NICER and XMM-Newton Data