Articles Citing

Constraints on the symmetry energy from PREX-II in the multimessenger era

Tong-Gang Yue¹, Lie-Wen Chen ^1,*, Zhen Zhang ², and Ying Zhou³

¹School of Physics and Astronomy, Shanghai Key Laboratory for Particle Physics and Cosmology, and Key Laboratory for Particle Astrophysics and Cosmology (MOE), Shanghai Jiao Tong University, Shanghai 200240, China
²Sino-French Institute of Nuclear Engineering and Technology, Sun Yat-sen University, Zhuhai 519082, China
³Quantum Machine Learning Laboratory, Shadow Creator Inc., Shanghai 201208, China

^*Corresponding author: lwchen@sjtu.edu.cn

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Novel scalings of neutron star properties from analyzing dimensionless Tolman–Oppenheimer–Volkoff equations

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Articles Citing

Constraints on the symmetry energy from PREX-II in the multimessenger era

Evidence for strong isovector nuclear spin–orbit interaction

Constraining the nuclear symmetry energy with PREX-II electroweak form factor data

A relativistic mechanism for the enhanced isovector spin-orbit interaction suggested by parity-violating electron scattering experiments

Toward a dedicated Skyrme interaction for α decay of superheavy nuclei

Constraining the nuclear symmetry energy with electric dipole polarizability and neutron skin characteristics in Pb208 within antisymmetrized molecular dynamics

Sensitivity of anisotropic flow in Pb+Pb collisions to the neutron skin of Pb208 at energies available at the CERN Large Hadron Collider

Anisotropic flows in Au+Au collisions at sNN=2.4 GeV with a Skyrme pseudopotential

Nuclear Signatures and Stellar Observables: Bridging Terrestrial Experiments and Neutron Star Structure

Beyond $$\rho ^{2/3}$$ scaling: microscopic origins and multimessengers of high-density nuclear symmetry energy

Nucleon short-range correlations and high-momentum dynamics: implications on the equation of state of dense matter

Constraining neutron star properties through parity-violating electron scattering experiments and relativistic point coupling interactions

Assessing the impact of incompressibility in the physics of nuclear matter and neutron star parameters

Reconciliation between Neutron Skin Thickness from PREX-2 Experiment and Neutron-Star Tidal Polarizability from GW170817 Event: The Key Role of Symmetry Energy Curvature

Phase transition and nuclear symmetry energy from neutron star observations: Constraints in light of PSR J0614-3329

Thermal properties of zero sound in asymmetrical nuclear matter

Extended Skyrme effective interactions with higher-order momentum dependence for transport models and neutron stars

Effects of symmetry energy on the properties of a hadron-quark mixed phase in hybrid stars

Novel scalings of neutron star properties from analyzing dimensionless Tolman–Oppenheimer–Volkoff equations

Constraining symmetry energy from pygmy dipole resonances in 68Ni and 132Sn*

Investigating Phase Transitions in Hybrid Stars Using the vMIT Bag Model and the QHD‐II Model

Equation of State Independent Determination on the Radius of a 1.4 M⊙ Neutron Star Using Mass–Radius Measurements

High-density Symmetry Energy: A Key to the Solution of the Hyperon Puzzle

Nuclear Matter Properties and Neutron Star Phenomenology Using the Finite Range Simple Effective Interaction

Dense nuclear matter equation of state from heavy-ion collisions

Refined determination of the weak mixing angle at low energy

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