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 …

We study scenarios where Dark Matter is a weakly interacting particle (WIMP) embedded in
an ElectroWeak multiplet. In particular, we consider real SU (2) representations with zero …

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 …

We present exoplanets as new targets to discover dark matter (DM). Throughout the Milky
Way, DM can scatter, become captured, deposit annihilation energy, and increase the heat …

Probing the existence of hypothetical particles beyond the Standard model often deals with
extreme parameters: large energies, tiny cross-sections, large time scales, etc. Sometimes …

Neutron stars close to the Galactic center are expected to swim in a dense background of
dark matter. For models in which the dark matter has efficient interactions with neutrons, they …

Indirect detection experiments typically measure the flux of annihilating dark matter (DM)
particles propagating freely through galactic halos. We consider a new scenario where …

We continue the study of weakly interacting massive particles (WIMP) started in Bottaro et
al.(Eur Phys JC 82: 31, 2022), focusing on a single complex electroweak n-plet with non …

Dark matter (DM) can be captured in celestial bodies after scattering and losing sufficient
energy to become gravitationally bound. We derive a general framework that describes the …