The nuclear symmetry energy and stability of matter in neutron star

Abstract

It is shown that behavior of the nuclear symmetry energy is the key quantity in the stability consideration in neutron star matter. The symmetry energy controls the position of crust-core transition and also may lead to new effects in the inner core of neutron star.

5 pages, 4 figures

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Cited by in corpus (68)

• Recent Progress and New Challenges in Isospin Physics with Heavy-Ion Reactions
• Symmetry Energy I: Semi-Infinite Matter
• Nuclear constraints on properties of neutron star crusts
• Towards Understanding Astrophysical Effects of Nuclear Symmetry Energy
• Nuclear symmetry energy and its density slope at normal density extracted from global nucleon optical potentials
• Combined Constraints on the Equation of State of Dense Neutron-Rich Matter from Terrestrial Experiments and Observations of Neutron Stars
• Locating the inner edge of neutron star crust using terrestrial nuclear laboratory data
• Bayesian Inference of High-density Nuclear Symmetry Energy from Radii of Canonical Neutron Stars
• On the Induced Gravitational Collapse of a Neutron Star to a Black Hole by a Type Ib/c Supernova
• Bayesian Inference of the Symmetry Energy of Super-Dense Neutron-Rich Matter from Future Radius Measurements of Massive Neutron Stars
• Neutron star equilibrium configurations within a fully relativistic theory with strong, weak, electromagnetic, and gravitational interactions
• Nuclear matter fourth-order symmetry energy in the relativistic mean field models
• Sensitivity of the transverse flow towards symmetry energy
• Implications of the mass $M=2.17_{-0.10}^{+0.11}$M${}_{\odot }$ of PSR~J0740+6620 on the Equation of State of Super-Dense Neutron-Rich Nuclear Matter
• Higher-order symmetry energy and neutron star core-crust transition with Gogny forces
• Single-nucleon potential decomposition of the nuclear symmetry energy
• In medium T-matrix for nuclear matter with three-body forces - binding energy and single particle properties
• Delineating Effects of Nuclear Symmetry Energy on the Radii and Tidal Polarizabilities of Neutron Stars
• Higher-order symmetry energy of nuclear matter and the inner edge of neutron star crusts
• Curvature-slope correlation of nuclear symmetry energy and its imprints on the crust-core transition, radius and tidal deformability of canonical neutron stars
• Constraints on the symmetry energy from observational probes of the neutron star crust
• Constraints on the inner edge of neutron star crusts from relativistic nuclear energy density functionals
• Probing isospin- and momentum-dependent nuclear effective interactions in neutron-rich matter
• Neutron star structure and collective excitations of finite nuclei
• Constraints on the phase transition and nuclear symmetry parameters from PSR $\mathrm{J}0740+6620$ and multimessenger data of other neutron stars
• Nuclear fourth-order symmetry energy and its effects on neutron star properties in the relativistic Hartree-Fock theory
• Study of the core-crust transition in neutron stars with finite-range interactions: the dynamical method
• Correlation of the neutron star crust-core properties with the slope of the symmetry energy and the lead skin thickness
• Bayesian refinement of covariant energy density functionals
• Prior probability distributions of neutron star crust models
• Exact versus Taylor-expanded energy density in the study of the neutron star crust-core transition
• Impact of Symmetry Energy on Sound Speed and Spinodal Decomposition in Dense Neutron-Rich Matter
• Effect of Inner Crust EoS on Neutron star properties
• Bayesian Inference of Fine-Features of Nuclear Equation of State from Future Neutron Star Radius Measurements to 0.1km Accuracy
• Influence of the interactions of scalar mesons on the behavior of the symmetry energy
• Impact of The Newly Revised Gravitational Redshift of X-ray Burster GS 1826-24 on The Equation of State of Supradense Neutron-Rich Matter
• Effects of the equation of state on the core-crust interface of slowly rotating neutron stars
• Imprints of Nuclear Symmetry Energy on Properties of Neutron Stars
• Role of density dependent symmetry energy in nuclear stopping
• Empirical radius formulas for canonical neutron stars from bidirectionally selecting EOS features in extended Bayesian analyses of observational data
• Stability of the $\beta$-equilibrated dense matter and core-crust transition in neutron stars
• Multilayer neutron stars with scalar mesons crossing term
• Effects of the U-boson on the inner edge of neutron star crusts
• Impact of the nuclear equation of state on the formation of twin stars
• Core-crust transition and crustal fraction of moment of inertia in neutron stars
• Transition density and pressure in hot neutron stars
• Phase transition and nuclear symmetry energy from neutron star observations: Constraints in light of PSR J0614--3329
• Crust-core interface and bulk neutron star properties
• Influence of the nuclear matter equation of state on the r-mode instability using the finite-range simple effective interaction
• The key factor to determine the relation between radius and tidal deformability of neutron stars: slope of symmetry energy
• Core-crust transition properties of neutron stars within systematically varied extended relativistic mean-field model
• Bayesian Quantification of Observability and Equation of State of Twin Stars
• Moments of inertia of neutron stars in relativistic mean field theory: the role of the isovector scalar channel
• Inner crust of neutron stars with mass-fitted Skyrme interaction
• N/Z and N/A dependence of balance energy as a probe of symmetry energy in heavy-ion collisions
• Bayesian Inference of Hybrid Star Properties from Future High-Precision Measurements of Their Radii
• Applicability of Relativistic Point-Coupling Models to Neutron Star Physics
• Novel features of asymmetric nuclear matter from terrestrial experiments and astrophysical observations of neutron stars
• Properties of the Object HESS J1731-347 as a Twin Compact Star
• Properties of glitching pulsars in the Skyrme-Hartree-Fock framework
• Strong correlation of the neutron star core-crust transition density with the $\sigma$-meson mass via vacuum polarization
• On the Cooling of Compact Stars in Light of the HESS J1731-347 Remnant
• Imprints of high-density nuclear symmetry energy on the crustal fraction of neutron star moment of inertia
• Effects of isoscalar- and isovector-scalar meson mixing on neutron star structure
• Neutron Star Equation of State with Nucleon Short-Range Correlations: A Concise Review and Open Issues
• Nuclear constraints on the inner edge of neutron star crusts
• Examining the possibility of a thick crust in the compact stellar object HESS J1731-347
• Bayesian Constraints on the Neutron Star Equation of State with a Smooth Hadron-Quark Crossover