Ultra-compact twin stars with hybrid equations of state from bosonic dark matter
astro-ph.HE, hep-ph, nucl-th
Submitted: 2026-09-03
Updated: 2026-09-03
Terminology
Sources
- Generic conditions for stable hybrid stars
- Non-Identical Neutron Star Twins
- Quark phases in neutron stars and a "third family" of compact stars as a signature for phase transitions
- Evidence for quark-matter cores in massive neutron stars
- Constraining neutron star matter with QCD
- Searching for New Physics in Ultradense Environment: a Review on Dark Matter Admixed Neutron Stars
- Comprehensive study of compact stars with dark matter
- The Second Love Number of Dark Compact Planets and Neutron Stars with Dark Matter
- Dark Compact Planets
- Improved Treatment of Dark Matter Capture in Neutron Stars
- Capture of Dark Matter in Neutron Stars
- Dark Matter Interpretation of the Neutron Decay Anomaly
- Dark Matter Effects On Neutron Star Properties
- Constraints on the fermionic dark matter from observations of neutron stars
- R-modes as a New Probe of Dark Matter in Neutron Stars
- Generating ultra compact boson stars with modified scalar potentials
- Generating ultra-compact neutron stars with bosonic dark matter
- A NICER View of PSR J0030+0451: Millisecond Pulsar Parameter Estimation
- PSR J0030+0451 Mass and Radius from NICER Data and Implications for the Properties of Neutron Star Matter
- A NICER View of the Massive Pulsar PSR J0740+6620 Informed by Radio Timing and XMM-Newton Spectroscopy
Related papers
- Numerical Studies of Accretion Flows onto a Neutron Star Engulfed in a Massive Star
- Collisionless Accretion of Finite-Angular-Momentum Plasma onto a Spinning Black Hole
- Impact of Magnetic Field Topology on Electromagnetic and Gravitational Waves from Binary Neutron Star Merger Remnants
- XRISM Resolve Spectroscopy of GX 5-1: Constraints on Iron Spectral Features in a Luminous Neutron-Star Binary
- SN 1006: A Cosmic Laboratory for Investigating Shock Acceleration Physics
- Neutrino Spectral Pinching in 3D Core-Collapse Supernovae: Late-Time Convergence, Failed-Explosion Signatures, and Viewing-Angle Dispersion