We study an impact of self-interacting bosonic dark matter (DM) on various observable
properties of neutron stars (NSs). The analysis is performed for asymmetric DM with masses …

Strange stars ought to exist in the universe according to the strange quark matter hypothesis,
which states that matter made of roughly equal numbers of up, down, and strange quarks …

We study possible effects of a dark matter (DM) core on the maximum mass of a neutron star
(NS), on the mass-radius relation and on the NS tidal deformability parameter Λ. We show …

The mirror twin Higgs model is a candidate for (strongly-interacting) complex dark matter,
which mirrors SM interactions with heavier quark masses. A consequence of this model are …

We study the dark matter (DM) effects on the nuclear matter (NM) parameters characterizing
the equation of states of super dense neutron-rich nucleonic matter. The observables of the …

The distribution of the dark matter (DM) in DM-admixed neutron stars (DANSs) is supposed
to result in either a dense dark core or an extended dark halo, subject to the DM fraction of …

Motivated by the recent detection of the gravitational wave signal emitted by a binary
neutron star merger, we analyse the possible impact of dark matter on such signals. We …

Neutron stars could contain a mixture of ordinary nuclear matter and dark matter, such that
dark matter could influence observable properties of the star, such as its mass and radius …

In this work, we apply relativistic mean-field theory in neutron stars assuming that fermionic
dark matter is trapped inside the star and interacts directly with neutrons by exchanging …

A subfraction of dark matter or new particles trapped inside celestial objects can significantly
alter their macroscopic properties. We investigate the new physics imprint on celestial …