We have constructed a Lagrangian model (SIG-OM) with coupling of sigma and omega mesons in the relativistic mean-field theory. Properties of finite nuclei and nuclear matter have been explored with the new Lagrangian model. The study shows that with SIG-OM an excellent description of binding energies and charge radii of nuclei over a large range of isospin is achieved. With an incompressibility of nuclear matter K=265 MeV, it is also able to describe the breathing-mode isoscalar giant mopole resonance energies successfully. It is shown that the high-density behaviour of the equation of state of nuclear and neutron matter with the sigma-omega coupling is significantly softer than the non-linear scalar coupling model
Properties of nuclear matter are calculated in the Dirac-Hartree-Fock approximation within the Ziman...
Recent works on the relativistic description of exotic nuclei and nuclear matter at extreme conditio...
We analyze the results for infinite nuclear and neutron matter using the standard relativistic mean ...
The sigma-omega coupling is introduced phenomenologically in the linear sigma-omega model to study t...
New parameter sets for the Lagrangian density in the relativistic mean field (RMF) theory, PK1 with ...
The parameters of the sigma-omega-rho model in the relativistic mean-field theory with nonlinear a-m...
The parameters of the $\sigma$-$\omega$-$\rho$ model in the relativistic mean-field theory with non...
The effects of $\omega$ meson self-coupling (OMSC) on the properties of finite nuclei and neutron st...
Starting from many quark interactions, we construct a nonlinear sigma-omega model at finite temperat...
AbstractA new Lagrangian model without nonlinear scalar self-interactions in the relativistic mean-f...
The equation of state (EOS) for highly compressed dense matter is one of the main concerns of nuclea...
The equation of state (EOS) for highly compressed dense matter is one of the main concerns of nuclea...
The equation of state (EOS) for highly compressed dense matter is one of the main concerns of nuclea...
Microscopic structure models based on the relativistic mean-field approximation have been extended t...
Properties of nuclear matter are calculated in the Dirac-Hartree-Fock approximation within the Ziman...
Properties of nuclear matter are calculated in the Dirac-Hartree-Fock approximation within the Ziman...
Recent works on the relativistic description of exotic nuclei and nuclear matter at extreme conditio...
We analyze the results for infinite nuclear and neutron matter using the standard relativistic mean ...
The sigma-omega coupling is introduced phenomenologically in the linear sigma-omega model to study t...
New parameter sets for the Lagrangian density in the relativistic mean field (RMF) theory, PK1 with ...
The parameters of the sigma-omega-rho model in the relativistic mean-field theory with nonlinear a-m...
The parameters of the $\sigma$-$\omega$-$\rho$ model in the relativistic mean-field theory with non...
The effects of $\omega$ meson self-coupling (OMSC) on the properties of finite nuclei and neutron st...
Starting from many quark interactions, we construct a nonlinear sigma-omega model at finite temperat...
AbstractA new Lagrangian model without nonlinear scalar self-interactions in the relativistic mean-f...
The equation of state (EOS) for highly compressed dense matter is one of the main concerns of nuclea...
The equation of state (EOS) for highly compressed dense matter is one of the main concerns of nuclea...
The equation of state (EOS) for highly compressed dense matter is one of the main concerns of nuclea...
Microscopic structure models based on the relativistic mean-field approximation have been extended t...
Properties of nuclear matter are calculated in the Dirac-Hartree-Fock approximation within the Ziman...
Properties of nuclear matter are calculated in the Dirac-Hartree-Fock approximation within the Ziman...
Recent works on the relativistic description of exotic nuclei and nuclear matter at extreme conditio...
We analyze the results for infinite nuclear and neutron matter using the standard relativistic mean ...