The extended nonlinear model has been applied to construct neutron star matter equation of state. In the case of neutron star matter with nonzero strangeness the extension of the vector meson sector by the inclusion of nonlinear mixed terms results in the stiffening of the equation of state and accordingly in the higher value of the maximum neutron star mass
I review the issues related to the appearance of hyperons in neutron star matter, focusing in partic...
We determine the structure of neutron stars within a Brueckner-Hartree-Fock approach based on realis...
I review the issues related to the appearance of hyperons in neutron star matter, focusing in partic...
This paper gives an overview of the model of a neutron star with non-zero strangeness constructed wi...
The comparative analysis of the impact of strangeness on the structure and evolution of a neutron st...
The true nature and the internal constitution of the compact stars known as neutron stars (NSs) is o...
The true nature and the internal constitution of the compact stars known as neutron stars (NSs) is o...
Context. A recent measurement of the mass of PSR J1614-2230 rules out most existing models of the eq...
Context. A recent measurement of the mass of PSR J1614-2230 rules out most existing models of the eq...
Context. A recent measurement of the mass of PSR J1614-2230 rules out most existing models of the eq...
Analysis of the density dependence of the symmetry energy in the case of strangeness-rich neutron s...
We investigate the equations of state for pure neutron matter and strange hadronic matter in $\beta$...
Recent progress in the understanding of the high density phase of neutron stars advances the view th...
The analysis of the density dependence of the nuclear symmetry Energy in strangeness-rich nuclear ma...
We present results from Brueckner-Hartree-Fock calculatons for beta stable neutron star matter with ...
I review the issues related to the appearance of hyperons in neutron star matter, focusing in partic...
We determine the structure of neutron stars within a Brueckner-Hartree-Fock approach based on realis...
I review the issues related to the appearance of hyperons in neutron star matter, focusing in partic...
This paper gives an overview of the model of a neutron star with non-zero strangeness constructed wi...
The comparative analysis of the impact of strangeness on the structure and evolution of a neutron st...
The true nature and the internal constitution of the compact stars known as neutron stars (NSs) is o...
The true nature and the internal constitution of the compact stars known as neutron stars (NSs) is o...
Context. A recent measurement of the mass of PSR J1614-2230 rules out most existing models of the eq...
Context. A recent measurement of the mass of PSR J1614-2230 rules out most existing models of the eq...
Context. A recent measurement of the mass of PSR J1614-2230 rules out most existing models of the eq...
Analysis of the density dependence of the symmetry energy in the case of strangeness-rich neutron s...
We investigate the equations of state for pure neutron matter and strange hadronic matter in $\beta$...
Recent progress in the understanding of the high density phase of neutron stars advances the view th...
The analysis of the density dependence of the nuclear symmetry Energy in strangeness-rich nuclear ma...
We present results from Brueckner-Hartree-Fock calculatons for beta stable neutron star matter with ...
I review the issues related to the appearance of hyperons in neutron star matter, focusing in partic...
We determine the structure of neutron stars within a Brueckner-Hartree-Fock approach based on realis...
I review the issues related to the appearance of hyperons in neutron star matter, focusing in partic...