The Non-Quenching of $g_A$ in Nuclei and Emergent Scale Symmetry in Dense Baryonic Matter
Yan-Ling Li, Yong-Liang Ma, Mannque Rho

TL;DR
This paper explains the non-quenching of the axial coupling constant $g_A$ in nuclei through nuclear correlations and emergent scale symmetry in dense matter, challenging the idea of fundamental quenching due to QCD condensates.
Contribution
It introduces a scale-symmetric chiral Lagrangian framework to explain $g_A$ behavior and describes the emergence of scale symmetry and pseudo-conformal sound velocity in dense baryonic matter.
Findings
$g_A$ remains unaffected by QCD condensates for densities below $n_{1/2}$.
At densities above $n_{1/2}$, matter exhibits pseudo-conformal behavior with a sound velocity approaching that of a conformal fluid.
The mechanism impacts gravitational wave signals from neutron star mergers.
Abstract
How the axial coupling constant in nuclear Gamow-Teller transitions described in shell model gets "quenched" to a universal constant close to 1 can be explained by nuclear correlations in Fermi-liquid fixed point theory using a scale-symmetric chiral Lagrangian supplemented with hidden local symmetric vector mesons. Contrary to what one might naively suspect -- and has been discussed in some circles, there is no fundamental quenching at nuclear matter density due to QCD condensates. When the density of many-body systems treated with the same Lagrangian increases beyond the density (where is the normal nuclear matter density) at which skyrmions representing baryons fractionize to half-skyrmions, with the meson driven toward the vector manifestation fixed point and a scalar meson driven to the dilaton-limit fixed point with the nucleons…
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