The sound speed and core of massive compact stars: A manifestation of hadron-quark duality
Yong-Liang Ma, Mannque Rho

TL;DR
This paper proposes a topological approach to describe the cores of massive compact stars, revealing emergent symmetries and a pseudo-conformal sound velocity, suggesting a form of hadron-quark duality without explicit quark degrees of freedom.
Contribution
It introduces a topology change framework that captures hadron-quark duality and emergent symmetries in dense nuclear matter, linking nuclear correlations to QCD properties.
Findings
Pseudo-conformal sound velocity of about 1/3 at densities above 3n0.
Emergent hidden symmetries from nuclear correlations.
Potential link between g_A quenching and the onset of pseudo-conformal behavior.
Abstract
When baryon-quark continuity is formulated in terms of a topology change without invoking "explicit " QCD degrees of freedom at a density higher than twice the nuclear matter density the core of massive compact stars can be described in terms of fractionally charged particles, behaving neither like pure baryons nor deconfined quarks. Hidden symmetries, both local gauge and pseudo-conformal (or broken scale), lead to the pseudo-conformal (PC) sound velocity at in compact stars. We argue these symmetries are "emergent" from strong nuclear correlations and conjecture that they reflect hidden symmetries in QCD proper exposed by nuclear correlations. We establish a possible link between the quenching of in superallowed Gamow-Teller transitions in nuclei and the precocious onset at of the PC sound velocity predicted at the…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
Taxonomy
TopicsPulsars and Gravitational Waves Research · Cosmology and Gravitation Theories · High-pressure geophysics and materials
