Finite-Temperature Axion-Admixed Neutron Stars in a Quarkyonic Crossover Framework

arXiv:2609.28555 · hep-ph, astro-ph.HE, astro-ph.SR, nucl-th · Submitted 2026-09-23 · Read on arXiv

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

Submitted: 2026-09-23

Updated: 2026-09-23

Terminology

• Core — 26× in this paper · explained in 2 episodes
• Consistency — 4× in this paper · explained in 3 episodes
• Symmetry Breaking — 3× in this paper · explained in 3 episodes
• Degeneracy — 2× in this paper · explained in 3 episodes
• Equation of State (EoS) — 2× in this paper · explained in 4 episodes
• Benchmark — 1× in this paper · explained in 2 episodes
• Fine-Tuning — 1× in this paper · explained in 5 episodes
• Momentum transfer — 1× in this paper · explained in 2 episodes
• Self-consistency — 1× in this paper · explained in 2 episodes

Sources

• Axion contribution to the mass-radius relation of neutron stars
• Measuring Nuclear Matter Parameters with NICER and LIGO/Virgo

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