Gravitational waves emitted from the coalescence of neutron star binaries open a new
window to probe matter and fundamental physics in unexplored, extreme regimes. To extract …

Because of the development of many-body theories of nuclear matter, the long-standing,
open problem of the equation of state (EOS) of dense matter may be understood in the near …

In the present work, we investigate the effects of dark matter (DM) on hybrid star properties.
We assume that dark matter is mixed with both hadronic and quark matter and interacts with …

We address the question of the role of low-energy nuclear physics data in constraining
neutron star global properties, eg, masses, radii, angular momentum, and tidal deformability …

A relativistic mean-field hadronic model with a dark matter (DM) particle coupled to nucleons
including short-range correlations (SRC) is applied to study neutron stars (NS). The lightest …

A neutron star was first detected as a pulsar in 1967. It is one of the most mysterious
compact objects in the universe, with a radius of the order of 10 km and masses that can …

In this work we investigate neutron stars (NS) in f (Script R, T) gravity for the case R+ 2λ
Script T, Script R is the Ricci scalar and Script T the trace of the energy-momentum tensor …

In this work we study a relativistic mean-field (RMF) hadronic model, with nucleonic short-
range correlations (SRC) included, coupled to dark matter (DM) through the Higgs boson …

In this work we consider strange stars formed by quark matter in the color-flavor-locked
(CFL) phase of color superconductivity. The CFL phase is described by a Nambu-Jona …

We perform a Bayesian analysis of neutrons star moment of inertia by utilizing the available
gravitational-wave data from LIGO/Virgo (GW170817 and GW190425) and mass-radius …