We present a comprehensive study of compact stars admixed with nonself-annihilating self-
interacting fermionic dark matter, delineating the dependence on the nuclear equation of …

The effect of dark matter (DM) on f-mode oscillations in DM admixed neutron stars (NSs) is
investigated in a comprehensive analysis with particular attention to the role of the nuclear …

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 …

Over the last few years, researchers have become increasingly interested in understanding
how dark matter affects neutron stars, hel** them to better understand complex …

The tidal deformability and the radius of neutron stars are observables, which have been
used to constrain the neutron star equation of state and explore the composition in neutron …

A major science goal of gravitational-wave (GW) observations is to probe the nature of
gravity and constrain modifications to general relativity. An established class of modified …

We investigate the structure and the tidal deformability of the color-flavor locked strange
stars admixed with mirror dark matter. Assuming the stars in the GW170817 event have a …

Neutron stars (NSs) have generally been considered as cold, zero-temperature entities.
Recent progress in computational methods and theoretical modelling has opened up the …

In this work we investigate the properties of neutron stars admixed with selfinteracting scalar
bosonic dark matter. The dark matter interaction is described by a generalized $\phi^ n …

We present a superfluid dark star model consisting of relativistic dark bosons with two-body
self-interaction. The obtained masses, radii, and tidal deformability depend in a simple way …