We put constraints on the secondary component of GW190814 by analyzing the
observational data of the event. The relativistic mean-field models are used to calculate the …

The speed of sound of the matter within neutron stars may contain nonsmooth structure
related to first-or higher-order phase transitions. Here we investigate what are the …

The impact of anisotropic pressure models in neutron stars (NSs) is increasing their
compactness. Therefore, for the relatively soft NS equation of state (EOS), we can still obtain …

We systematically study the properties of pure nucleonic and hyperonic magnetic stars using
a density-dependent relativistic mean-field (DD-RMF) equations of state. We explore several …

We investigate the peculiar nature of strange stars through an analysis of different quark
models, ie vBag model and CFL model equation of states at different parameter sets, and …

A viable model for the dense matter equation of state above the nuclear saturation density
includes a hadron-to-quark phase transition at densities relevant to compact objects. In this …

The effects of the ϕ meson on the properties of hyperon stars are studied systematically in
the framework of the density-dependent relativistic mean field (DDRMF) model. The ϕ …

We investigate the properties of stars participating in double compact star merger events
considering interacting model of stable strange quark matter. We model the matter making it …

We investigate the possible presence of dark matter (DM) in massive and rotating neutron
stars (NSs). For the purpose we extend our previous work [1] to introduce a light new physics …

We investigate the effect of Δ baryons on the radial oscillations of neutron and hyperon stars,
employing a density-dependent relativistic mean-field model. The spin-3/2 baryons are …