Impact of crust-core connection procedures on the tidal deformability of neutron stars
arXiv:2602.11809 · doi:10.1103/jlfv-mkbt
Abstract
We study the impact of crust-core connection procedures on various neutron-star properties, especially on the tidal deformability. We consider three types of connection procedures to treat the discontinuity in a nonunified equation of state around the crust-core transition: (1) the direct connection procedure, (2) the crossover connection procedure, and (3) the segmented method. Our results indicate that the mass-radius relations of neutron stars are almost unaffected by the details of the connection procedure. However, the tidal deformabilities of neutron stars are sensitive to the crust-core connection procedures. The tidal deformability is closely related to gravitational-wave measurements. For a canonical 1.4 neutron star, uncertainties in the tidal deformability from different connection procedures can exceed 20\%. We find that the direct connection procedure yields significantly larger uncertainties in the tidal deformability, while the segmented method and crossover connection procedure provide relatively stable results.
14 pages, 10 figures, 3 tables, has been accepted by Physical Review C
References in corpus (44)
- Observation of Gravitational Waves from a Binary Black Hole Merger
- GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral
- A Massive Pulsar in a Compact Relativistic Binary
- GW170817: Measurements of Neutron Star Radii and Equation of State
- 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
- A unified equation of state of dense matter and neutron star structure
- A NICER View of the Massive Pulsar PSR J0740+6620 Informed by Radio Timing and XMM-Newton Spectroscopy
- Equations of state for supernovae and compact stars
- Refined Mass and Geometric Measurements of the High-Mass PSR J0740+6620
- Strange Quark Matter and Compact Stars
- Physics of Neutron Star Crusts
- New constraints on radii and tidal deformabilities of neutron stars from GW170817
- Evidence for quark-matter cores in massive neutron stars
- The NANOGrav 11-year Data Set: High-precision timing of 45 Millisecond Pulsars
- The Equation of State of Hot, Dense Matter and Neutron Stars
- Relativistic Mean-Field Hadronic Models under Nuclear Matter Constraints
- Neutron skins and neutron stars in the multi-messenger era
- Tidal Love Numbers of Neutron and Self-Bound Quark Stars
- Relativistic effective interaction for nuclei, giant resonances, and neutron stars
- Nonparametric constraints on neutron star matter with existing and upcoming gravitational wave and pulsar observations
- Neutron star radii and crusts: uncertainties and unified equations of state
- Neutron star tidal deformability and equation of state constraints
- GW190814: Impact of a 2.6 solar mass neutron star on nucleonic equations of state
- Unified treatment of sub-saturation stellar matter at zero and finite temperature
- Tidal deformability with sharp phase transitions in (binary) neutron stars
- Complete relativistic equation of state for neutron stars
- A new equation of state for neutron star matter with nuclei in the crust and hyperons in the core
- Effects of symmetry energy on equation of state for simulations of core-collapse supernovae and neutron-star mergers
- Influence of the hadronic equation of state on the hadron-quark phase transition in neutron stars
- Effects of the symmetry energy on properties of neutron star crusts near the neutron drip density
- Influence of the symmetry energy on nuclear pasta in neutron star crusts
- Massive Neutron Stars with Antikaon Condensates in a Density Dependent Hadron Field Theory
- Nuclear symmetry energy and hadron-quark mixed phase in neutron stars
- Effects of nuclear symmetry energy and equation of state on neutron star properties
- Neutron stars and the dense matter equation of state: from microscopic theory to macroscopic observations
- On the stability of strange dwarf hybrid stars
- Effects of -meson on properties of hyperon stars in density dependent relativistic mean field model
- Possibility of s-wave pion condensates in neutron stars revisited
- Charged pion condensation in dense quark matter: Nambu--Jona-Lasinio model study
- Quark-meson coupling model for antikaon condensation in neutron star matter with strong magnetic fields
- The Hadron-Quark Crossover in Neutron Star within Gaussian Process Regression Method
- (Anti)kaon condensation in strongly magnetized dense matter