Microscopic Interaction versus Purely Gravitational Coupling in Strange Quark Stars Admixed with Dark Matter: A One-Fluid and Two-Fluid Comparison

arXiv:2608.12383 · astro-ph.HE, gr-qc, hep-ph, hep-th · Submitted 2026-07-30 · Read on arXiv

J. Sedaghat, G. H. Bordbar, M. Haghighat, S. M. Zebarjad

astro-ph.HE, gr-qc, hep-ph, hep-th

Submitted: 2026-07-30

Updated: 2026-08-14

Comments: 16 pages, 11 figures, 4 tables

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

Terminology

• Core — 4× in this paper · explained in 2 episodes
• Consistency — 3× in this paper · explained in 3 episodes
• Particle Data Group — 2× in this paper
• Adaptability — 1× in this paper · explained in 1 episode
• Alignment — 1× in this paper · explained in 1 episode
• Conservation Laws — 1× in this paper · explained in 3 episodes
• Degeneracy — 1× in this paper · explained in 3 episodes
• Equation of State (EoS) — 1× in this paper · explained in 4 episodes
• Gravitational Lensing — 1× in this paper · explained in 2 episodes
• Symmetry Breaking — 1× in this paper · explained in 3 episodes

Sources

• Observational Probes of the Neutron Star Equation of State with Hyperons, Bosonic Dark Matter, and Quark Matter

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