Using hydrodynamical simulations for a large set of high-density matter equations of state
(EOSs), we systematically determine the threshold mass M thres for prompt black-hole …

This study addresses the collapse behavior of neutron star (NS) mergers expressed through
the binary threshold mass M thres for prompt black-hole (BH) formation, which we determine …

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 …

The stability and equation of state of quark matter are studied within both two-flavor and (2+
1)-flavor Nambu-Jona-Lasinio (NJL) models including the vector interactions. With a free …

The rotating neutron-star properties are studied to investigate a phase transition to quark
matter. The density-dependent relativistic mean-field model (DD-RMF) is employed to study …

In this work we study different variations of the MIT bag model. We start with the so called
non-ideal bag model and discuss it in detail. Then we implement a vector interaction in the …

In this work, we perform a comparative analysis between the density-dependent quark
model and the vector MIT bag model using Bayesian analysis. We use the equations of state …

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 …

The effects of strong magnetic fields on the deconfinement phase transition expected to take
place in the interior of massive neutron stars are studied in detail for the first time. For …

Several global parameters of compact stars are related via empirical relations, which are
(nearly) independent of the underlying equation of state (EoS) of dense matter and …