Nuclear Symmetry Energy Extracted from Laboratory Experiments

Abstract

Some recent progress and open questions in extracting and understanding the new physics underlying the density dependence of nuclear symmetry energy from laboratory experiments are discussed.

A feature article to appear in Nuclear Physics News

References in corpus (3)

• Momentum sharing in imbalanced Fermi systems
• The Nuclear Symmetry Energy
• Fundamental quantum limits to waveform detection

Cited by in corpus (38)

• Progress in Constraining Nuclear Symmetry Energy Using Neutron Star Observables Since GW170817
• Towards Understanding Astrophysical Effects of Nuclear Symmetry Energy
• Nucleon Effective Masses in Neutron-Rich Matter
• Dense Nuclear Matter Equation of State from Heavy-Ion Collisions
• Combined Constraints on the Equation of State of Dense Neutron-Rich Matter from Terrestrial Experiments and Observations of Neutron Stars
• Extracting Nuclear Symmetry Energies at High Densities from Observations of Neutron Stars and Gravitational Waves
• Bayesian Inference of High-density Nuclear Symmetry Energy from Radii of Canonical Neutron Stars
• GW190814's secondary component with mass $(2.50-2.67)$ M${}_{\odot }$ as a super-fast pulsar
• Bayesian Inference of the Symmetry Energy of Super-Dense Neutron-Rich Matter from Future Radius Measurements of Massive Neutron Stars
• 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
• Bayesian inference of dense matter EOS encapsulating a first-order hadron-quark phase transition from observables of canonical neutron stars
• GW170817 implications on the frequency and damping time of f-mode oscillations of neutron stars
• Bayesian inference of nuclear symmetry energy from measured and imagined neutron skin thickness in ${}^{116,118,120,122,124,130,132}$Sn, ${}^{208}$Pb, and ${}^{48}$Ca
• Impact of NICER's Radius Measurement of PSR J0740+6620 on Nuclear Symmetry Energy at Suprasaturation Densities
• Translating neutron star observations to nuclear symmetry energy via artificial neural networks
• Neutron star matter with strange interactions in a relativistic quark model
• Constraining the nuclear symmetry energy and properties of neutron star from GW170817 by Bayesian analysis
• Probing high-density nuclear symmetry energy with ${\Xi }^{-}/{\Xi }^0$ ratio in heavy-ion collisions at $\sqrt{s_{NN}}\sim 3$ GeV
• Extended Skyrme interactions for transport model simulations of heavy-ion collisions
• Symmetry energy effects on the properties of hybrid stars
• Bayesian Inference of Fine-Features of Nuclear Equation of State from Future Neutron Star Radius Measurements to 0.1km Accuracy
• Nuclear collective dynamics in the lattice Hamiltonian Vlasov method
• Density-dependent van der Waals model under the GW170817 constraint
• Temperature dependence of the volume and surface contributions to the nuclear symmetry energy within the coherent density fluctuation model
• Intersections of ultracold atomic polarons and nuclear clusters: How is a chart of nuclides modified in dilute neutron matter?
• Astrophysics with heavy-ion beams
• Minimal Length, Nuclear Matter, and Neutron Stars
• Auxiliary Function Approach for Determining Symmetry Energy at Supra-saturation Densities
• Effects of retarded electrical fields on observables sensitive to the high-density behavior of nuclear symmetry energy in heavy-ion collisions at intermediate energies
• Probing dense QCD matter in the laboratory: The CBM experiment at FAIR
• Relativistic self-energy decomposition of nuclear symmetry energy and equation of state of neutron matter within QCD sum rules
• The key factor to determine the relation between radius and tidal deformability of neutron stars: slope of symmetry energy
• Astrophysics in the Laboratory: The CBM Experiment at FAIR
• Symmetry energy of super-dense neutron-rich matter from integrating barotropic pressures in neutron stars and heavy-ion reactions
• Revisiting the isospin relaxation time in intermediate-energy heavy-ion collisions
• From masses and radii of neutron stars to EOS of nuclear matter through neural network
• New Insights into Supradense Matter from Dissecting Scaled Stellar Structure Equations
• Aspects of approximation in modelling of the symmetry energy