EoS from terrestrial experiments: static and dynamic polarizations of nuclear density

Abstract

We critically examine nuclear matter and neutron matter equation of state (EoS) parameters by using best available terrestrial experimental results. The nuclear incompression modulus $K_{\infty }$ is re-examined in comparisons with RPA results of modern relativistic and non-relativistic EDF and up-to-date experimental data of isoscalar giant monopole resonance energy of ${}^{208}$Pb. The symmetry energy expansion coefficients $J$, $L$ and $K_{sym}$ are examined by recent FRDM mass model and the neutron skin of ${}^{48}$Ca extracted from $(p,p^{\prime })$ experiments.

13 pages, 6figures, To appear in the AIP Conference Proceedings of the Xiamen-CUSTIPEN Workshop on the EOS of Dense Neutron-Rich Matter in the Era of Gravitational Wave Astronomy (January 3 - 7, 2019, Xiamen, China

References in corpus (2)

• Neutron density distributions from antiprotonic 208Pb and 209Bi atoms
• Excitation of Giant Monopole Resonance in ${}^{208}$Pb and ${}^{116}$Sn Using Inelastic Deuteron Scattering

Cited by in corpus (3)

• Multi-messenger and multi-physics Bayesian inference for GW170817 binary neutron star merger
• Low-energy nuclear physics and global neutron star properties
• Nuclear incompressibility and sound speed in uniform matter and finite nuclei