Effects of Mirror Dark Matter on Neutron-Star Structure and Tidal Deformability

arXiv:2606.28934 · hep-ph, astro-ph.HE, nucl-th · Submitted 2026-06-27 · Read on arXiv

Jin-Cheng Jiao, Cheng-Ming Li

hep-ph, astro-ph.HE, nucl-th

Submitted: 2026-06-27

Comments: 12 pages, 8 figures

License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/

Terminology

• Core — 17× in this paper · explained in 2 episodes
• Regularization — 4× in this paper · explained in 3 episodes
• Equation of State (EoS) — 3× in this paper · explained in 4 episodes
• First-Order Transition — 1× in this paper · explained in 2 episodes
• Phase Transitions — 1× in this paper · explained in 2 episodes
• Symmetry Breaking — 1× in this paper · explained in 3 episodes
• Trace — 1× in this paper · explained in 2 episodes

Sources

• QCD vacuum pressure and its influence on the equation of state of non-strange quark stars

Related papers

• Classification of g-modes for neutron stars with a strong transition: Novel universal relation including slow stable hybrid stars
• Higgsino Dark Matter Interpretation of the LUX-ZEPLIN 248 keV Nuclear-Recoil Event
• A Unified Bogoliubov Approach to Primordial Gravitational Waves: From Inflation to Reheating
• Probing Memory-Burdened Primordial Black Holes with High-Energy Neutrinos
• Enhanced Dark Matter Quantum Sensing via Phase-Space Geometric Interferometry
• Axions as Dark Matter, Dark Energy, and Dark Radiation