WDs and neutron stars are far-reaching and multi-faceted laboratories in the hunt for dark
matter. We review detection prospects of wave-like, particulate, macroscopic and black hole …

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 …

Isolated ideal neutron stars (NS) of age> 10 9 yr exhaust thermal and rotational energies
and cool down to temperatures below O (100) K. Accretion of particle dark matter (DM) by …

In this work, we investigate the tidal deformability of a neutron star admixed with dark matter,
modeled as a massive, self-interacting, complex scalar field. We derive the equations to …

While astrophysical and cosmological probes provide a remarkably precise and consistent
picture of the quantity and general properties of dark matter, its fundamental nature remains …

The dense environment of neutron stars makes them an excellent target for probing dark
matter interactions with the Standard Model. We study neutron star heating from capture of …

We systematically study the observable properties of dark-matter admixed neutron stars with
arbitrary dark-matter fraction, employing a realistic nuclear equation of state in combination …

Dark matter (DM) from the galactic halo can accumulate in neutron stars and transmute them
into sub-2.5 M⊙ black holes if the dark matter particles are heavy, stable, and have …

In many cosmologies dark matter clusters on subkiloparsec scales and forms compact
subhalos, in which the majority of Galactic dark matter could reside. Null results in direct …

Neutron stars harbour matter under extreme conditions, providing a unique testing ground
for fundamental interactions. We recently developed an improved treatment of dark matter …