Bayesian Constraints on Bosonic Dark Matter in Neutron Stars within a Covariant Density-Functional Equation-of-State Ensemble
nucl-th, astro-ph.HE
Submitted: 2026-09-29
Updated: 2026-09-29
Terminology
Sources
- Dark Matter
- Dark matter in compact stars
- Searching for New Physics in Ultradense Environment: a Review on Dark Matter Admixed Neutron Stars
- Illuminating the dark universe in the multi-messenger era
- Dark Matter Effects On Neutron Star Properties
- Asymmetric Dark Stars and Neutron Star Stability
- Constraining Asymmetric Dark Matter through observations of compact stars
- Have neutron stars a dark matter core?
- Bosonic Dark Matter in Neutron Stars and its Effect on Gravitational Wave Signal
- Neutron stars: new constraints on asymmetric dark matter
- Amplified capture rate of dark matter in compact binaries and constraints on bosonic dark matter from GW170817
- Improved bounds on the bosonic dark matter with pulsars in the Milky Way
- Nucleon Structure and Strong Interactions in Dark Matter Capture in Neutron Stars
- On the change of old neutron star masses with galactocentric distance
- Dark Matter Capture in Supernovae Modifies Dark Photon Cooling Bounds
- Heavy dark matter in rapidly evolving massive stars
- Gravothermal Pile-Up of Collisional Dark Matter Around Compact Objects
- Constraining dark matter self-interaction from kinetic heating in neutron stars
- Triggering Electron Capture Supernovae: Dark Matter Effects in Degenerate White-Dwarf-like Cores of Super-Asymptotic Giant Branch Stars
- Dark halos around neutron stars and gravitational waves
Related papers
- BRST quantization for the restoration of broken symmetries: a pedagogical example
- FUSION: a skill-based research agent for publicly obtainable nuclear-physics codes
- Sensitivity of Neutron Star Observables to Transition Density in Hybrid Equation-of-State Models
- Exterior complex scaling enables physics-informed neural networks for quantum scattering
- Microscopic Insights into the Quarkyonic Hadron--Quark Crossover: Lessons from Ultracold Fermi Gases
- An Effective Upper Bound on the Pressure-to-Energy Density Ratio in Neutron Stars