Density-dependent symmetry energy at subsaturation densities from nuclear mass differences
arXiv:1403.2055 · doi:10.1103/PhysRevC.89.017305
Abstract
We extract the mass-dependent symmetry energy coefficients with the nuclear mass differences reducing the uncertainties as far as possible. The estimated of is MeV, which is further used to analyze the density-dependent nuclear matter symmetry energy at subsaturation densities. The slope parameter of the symmetry energy at the saturation density is MeV. Furthermore, it is found that, at the density of fm, the symmetry energy MeV and the correspondingly slope parameter is MeV, which are consistent with other independent analysis.
arXiv comment4 pages, 1 figure
References in corpus (28)
- Neutron Star Observations: Prognosis for Equation of State Constraints
- Recent Progress and New Challenges in Isospin Physics with Heavy-Ion Reactions
- Isospin Asymmetry in Nuclei and Neutron Stars
- Neutron Star Structure and the Neutron Radius of 208Pb
- Constraints on the symmetry energy and neutron skins from experiments and theory
- Reaction Dynamics with Exotic Beams
- Neutron-Rich Nuclei in Heaven and Earth
- Nuclear symmetry energy probed by neutron skin thickness of nuclei
- Neutron Radii in Mean-Field Models
- Constraints on the symmetry energy and on neutron skins from the pygmy resonances in 68Ni and 132Sn
- Nuclear Matter and its Role in Supernovae, Neutron Stars and Compact Object Binary Mergers
- Symmetry Energy I: Semi-Infinite Matter
- Connecting Neutron Star Observations to Three-Body Forces in Neutron Matter and to the Nuclear Symmetry Energy
- Surface Symmetry Energy
- Further improvements on a global nuclear mass model
- Constraining the symmetry energy at subsaturation densities using isotope binding energy difference and neutron skin thickness
- Mirror nuclei constraint in mass formula
- Constraining the nuclear equation of state at subsaturation densities
- Giant Quadrupole Resonances in 208Pb, the nuclear symmetry energy and the neutron skin thickness
- Probing the Equation of State of Nuclear Matter via Neutron Star Asteroseismology
- Shell and isospin effects in nuclear charge radii
- Determining the density content of symmetry energy and neutron skin: an empirical approach
- Correlation between alpha-decay Energies of Superheavy Nuclei Involving Effect of Symmetry Energy
- Nuclear symmetry energy at subnormal densities from measured nuclear masses
- Density dependence of nuclear symmetry energy constrained by mean-field calculations
- Nuclear symmetry energy from the Fermi-energy difference in nuclei
- Origin of symmetry energy in finite nuclei and density dependence of nuclear matter symmetry energy from measured alpha-decay energies
- Constraining the density dependence of symmetry energy from nuclear masses
Cited by in corpus (15)
- Theoretical and Experimental Constraints for the Equation of State of Dense and Hot Matter
- Model dependence of the neutron-skin thickness on the symmetry energy
- Constraining nuclear symmetry energy with the charge radii of mirror-pair nuclei
- Equation of state of nuclear matter from empirical constraints
- H/He ratio as a probe of the nuclear symmetry energy at sub-saturation densities
- Constraints on neutron skin thickness in 208Pb and density-dependent symmetry energy
- Studies of the equation-of-state of nuclear matter by heavy-ion collisions at intermediate energy in the multi-messenger era
- Influence of differential elastic nucleon-nucleon cross section on stopping and collective flows in heavy-ion collisions at intermediate energies
- Modern nuclear and astrophysical constraints of dense matter in a renormalized chiral approach
- Symmetry energy at subsaturation densities and the neutron skin thickness of 208Pb
- Probing the density dependence of the symmetry energy by nucleon flow
- Equation of state of asymmetric nuclear matter and the tidal deformability of neutron star
- Symmetry energy effects on isovector properties of neutron rich nuclei with a Thomas-Fermi approach
- r-mode instability of neutron stars in low-mass X-ray binaries: effects of Fermi surface depletion and superfluidity of dense matter
- A new probe to study symmetry energy at low density by deuteron breakup reaction