Although ab initio calculations of relativistic Brueckner theory lead to large scalar isovector
fields in nuclear matter, at present, successful versions of covariant density functional theory …

We study the effect of the isovector-scalar meson a 0 (980) on the properties of nuclear
matter and the neutron star (NS) matter by constructing a parity doublet model with including …

We present the covariance analysis of two successful nuclear energy density functionals
(EDFs),(i) a non-relativistic Skyrme functional built from a zero-range effective interaction …

The effect of δ-and ω-ρ-meson cross couplings on asymmetry nuclear systems are analyzed
in the framework of an effective field theory motivated relativistic mean field formalism. The …

In this review, we summarize recent studies on nuclear matter and finite nuclei based on
parity doublet models. We first construct a parity doublet model (PDM), which includes the …

The effect of temperature on the crust-core transition of a magnetar is studied. The
thermodynamical spinodals are used to calculate the transition region within a relativistic …

The equation of state of neutron matter is affected by the presence of a magnetic field due to
the intrinsic magnetic moment of the neutron. Here we study the equilibrium configuration of …

The thermodynamical instabilities of low densities in the np matter and npe matter are
studied within several relativistic nuclear models under some values of magnetic fields. The …

The effects of δ mesons on the dynamical instabilities of cold and warm nuclear and stellar
matter at subsaturation densities are studied in the framework of relativistic mean-field …

Equilibrium sequences were developed for rotating neutron stars in the relativistic mean-
field interaction framework using four density-dependent equations of state (EOSs) for the …