2 research outputs found
Fermion Proca Stars: Vector Dark Matter Admixed Neutron Stars
Dark matter could accumulate around neutron stars in sufficient amounts to
affect their global properties. In this work, we study the effect of a specific
model for dark matter -- a massive and self-interacting vector (spin-1) field
-- on neutron stars. We describe the combined systems of neutron stars and
vector dark matter using Einstein-Proca theory coupled to a nuclear-matter
term, and find scaling relations between the field and metric components in the
equations of motion. We construct equilibrium solutions of the combined
systems, compute their masses and radii and also analyse their stability and
higher modes. The combined systems admit dark matter (DM) core and cloud
solutions. Core solutions compactify the neutron star component and tend to
decrease the total mass of the combined system. Cloud solutions have the
inverse effect. Electromagnetic observations of certain cloud-like
configurations would appear to violate the Buchdahl limit. This could make
Buchdahl-limit violating objects smoking gun signals for dark matter in neutron
stars. The self-interaction strength is found to significantly affect both mass
and radius. We also compare fermion Proca stars to objects where the dark
matter is modelled using a complex scalar field. We find that fermion Proca
stars tend to be more massive and geometrically larger than their scalar field
counterparts for equal boson masses and self-interaction strengths. Both
systems can produce degenerate masses and radii for different amounts of DM and
DM particle masses.Comment: 20 pages, 11 figures, superseeds arXiv:2308.1217
Tidal Deformability of Fermion-Boson Stars: Neutron Stars Admixed with Ultra-Light Dark Matter
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 compute the tidal deformability of the full
Einstein-Hilbert-Klein-Gordon system self-consistently, and probe the influence
of the scalar field mass and self-interaction strength on the total mass and
tidal properties of the combined system. We find that dark matter core-like
configurations lead to more compact objects with smaller tidal deformability,
and dark matter cloud-like configurations lead to larger tidal deformability.
Electromagnetic observations of certain cloud-like configurations would appear
to violate the Buchdahl limit. The self-interaction strength is found to have a
significant effect on both mass and tidal deformability. We discuss
observational constraints and the connection to anomalous detections. We also
investigate how this model compares to those with an effective bosonic equation
of state and find the interaction strength where they converge sufficiently.Comment: 14 pages, 7 figures; Accepted for publicatio