We review the physics of hyperons and Δ-resonances in dense matter in compact stars. The
covariant density functional approach to the equation of state and composition of dense …

Neutron stars are among the densest known objects in the universe and an ideal laboratory
for the strange physics of supercondensed matter. While the simultaneous measurements of …

We study rapidly rotating hybrid stars with the Dyson-Schwinger model for quark matter and
the Brueckner-Hartree-Fock many-body theory with realistic two-body and three-body forces …

Based on covariant density functional theory, we study the effects of rotation on the nucleon
direct URCA (N-DURCA) process for traditional and hyperonic neutron stars. The calculated …

In this theoretical study, we report an investigation of the equations of state (EoSs) of hyper-
nuclear matter and its composition as a function of density within the framework of effective …

With the inclusion of the isovector scalar channel in the meson-nucleon couplings, taking
DD-ME δ as an effective interaction, the moments of inertia of neutron stars possessing …

In the framework of the relativistic mean field theory including the hyperon-hyperon (YY)
interactions, protoneutron stars with a weakly interacting light U boson are studied. The U …

Based on the equations of state from the relativistic mean field theory without and with the
inclusion of strangeness-bearing hyperons, we study the dimensionless spin parameter j …

Neutron stars manifest one of the Universe's densest objects, where matter is compressed at
high densities, and nuclear physics combines with general relativity. The dense nuclear …

We investigate theoretical and observational constraints on the mass-radius relations for
neutron stars. For that purpose we consider the model of neutron stars taking into …