PSR J0740+ 6620 has a gravitational mass of 2.08±0.07 M⊙, which is the highest reliably
determined mass of any neutron star. As a result, a measurement of its radius will provide …

We present a systematic study of f-mode oscillations in neutron stars containing hyperons,
extending recent results obtained within the Cowling approximation to linearized general …

We introduce a family of equations of state (EoS) for hybrid neutron star (NS) matter that is
obtained by a two-zone parabolic interpolation between a soft hadronic EoS at low densities …

We investigate the possibility that GW170817 was not the merger of two conventional
neutron stars (NS), but involved at least one if not two hybrid stars with a quark matter core …

The possible presence of deconfined matter in the cores of massive neutron stars is the
subject of a large debate. In this context, it is important to set limits on the size and …

ABSTRACT A theoretical framework for calculating the mass–radius curve of compact stars
in the Kaluza–Klein space–time is introduced, with one additional compact spatial …

We present a Bayesian analysis on the equation of state of neutron stars based on a class of
relativistic mean field models. The priors on the equation of state are related to the …

Recent studies based on the relativistic mean field (RMF) model found certain nuclear
empirical parameters, in particular the nucleon effective mass, to be strongly correlated with …

In this paper, an investigation of the role of nuclear saturation parameters on f-mode
oscillations in neutron stars is performed within the Cowling approximation. It is found that …

We investigated recent observation data of pulsar masses of PSR J0740+ 6620, PSR
J0348+ 0432, and PSR J1614− 2230 based on the extended σ-ω model. We assumed that …