Can a slow and strong phase transition in neutron stars relieve major compact-star observation tensions?

arXiv:2606.17231 · astro-ph.HE, gr-qc, hep-ph, nucl-th · Submitted 2026-06-15 · Read on arXiv

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

Submitted: 2026-06-15

Updated: 2026-10-10

Terminology

• Phase Transition — 2× in this paper · explained in 2 episodes
• Benchmark — 1× in this paper · explained in 2 episodes

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