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 7 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 4 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

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