Topical issue on nuclear symmetry energy

By Bao-An Li, À. Ramos, G. Verde, Isaac Vidaña. 2014

224 citations recorded by the source corpus.

Subfields: Nuclear and High Energy Physics, Radiation

View Paper: https://www.semanticscholar.org/paper/13ee4e5cbe6ea320f5b98c0690099c231343f619

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

In Nuclear and High Energy Physics

1. G. Fiorella Burgio
2. Marc A. Baldo
3. Bao-An Li
4. Nai-Bo Zhang
5. Jun Xu
6. Lie-Wen Chen
7. Bao-Jun Cai
8. Wen-Jie Xie

In Radiation

1. Bao-An Li
2. Marc A. Baldo
3. Jun Xu
4. G. Fiorella Burgio
5. Lie-Wen Chen

Citations in the corpus

• Global performance of covariant energy density functionals: ground state observables of even-even nuclei and the estimate of theoretical uncertainties (2014, background): “[38]) from ab initio calculations and from isovector excitations such as the giant dipole resonance (GDR) indicate clearly that one needs a density dependence in the isovector channel [39], as we have it in the CEDF’s DD-ME2, DD-ME δ , or DD-PC1.”
• Combined Constraints on the Equation of State of Dense Neutron-rich Matter from Terrestrial Nuclear Experiments and Observations of Neutron Stars (2018, background): “(Li et al. 2014; Russotto et al. 2016; Xu et al. 2016; Tsang et al. 2017; Trautmann and Wolter 2017).”
• Results of the ASY-EOS experiment at GSI: The symmetry energy at suprasaturation density (2016, background): “A comprehensive list of pertinent articles has recently appeared in Topical Issue on Nuclear Symmetry Energy [42].”
• Nucleon Effective Masses in Neutron-Rich Matter (2018, methodology): “ng, in this subsection we very briefly summarize the current situation of constraining the density dependence of nuclear symmetry energy. More comprehensive reviews on this topic can be found in refs. [19, 134, 167, 168, 169, 170, 171, 172, 173, 174, 175, 176, 177, 178, 179]. Essentially all availabl”
• Progress in Constraining Nuclear Symmetry Energy Using Neutron Star Observables Since GW170817 (2021, background): “The symmetry energy Esym(ρ) at supra-saturation densities and the possible hadron-quark phase transition are among the most uncertain parts of the EOS of dense neutron-rich matter [11,12,14, 28].”
• The Nuclear Symmetry Energy (2016, background): “the symmetry energy as a function of density [1].”