From Nuclear Matter with Quenched $g_A$ to Compact-Star Matter with a Signal for Emergent Hidden Scale Symmetry
Mannque Rho

TL;DR
This paper proposes that the longstanding quenching of the axial coupling constant in nuclei can be explained by an emergent hidden scale symmetry in dense matter, with implications for understanding the physics of compact stars.
Contribution
It introduces a novel effective field theory framework incorporating hidden scale and local symmetries to connect nuclear quenching phenomena with emergent symmetries in dense matter.
Findings
Quenched $g_A$ linked to hidden scale symmetry in dense matter
Connection between sound speed in stars and pseudo-conformal symmetry
Framework extends beyond traditional nuclear effective field theories
Abstract
An ``unorthodox" idea is developed that the long-standing mystery in nuclear physics of the effective axial-current coupling constant in nuclei, , could be interpreted in terms of an emerging hidden scale symmetry in dense compact-star matter. Arguments are presented using an effective field theory anchored on a renormalization-group approach to interacting baryons on the Fermi surface coupled with hidden symmetric heavy mesonic degrees of freedom that enables one to go beyond Weinberg's nuclear effective field theory involving nucleon and pion fields only, referred hereon to as EFT. Both hidden local and scale symmetries, the former involving the vector mesons and and the latter the hidden scalar meson, a dilaton (i.e., ), play the crucial role. Going beyond the density regime applicable to normal nuclear…
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