1. A Solution to the Quenched ${g_A}$ Problem in Nuclei and Dense Baryonic Matter
- Author
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Rho, Mannque, Institut de Physique Théorique - UMR CNRS 3681 (IPHT), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay-Centre National de la Recherche Scientifique (CNRS), and HEP, INSPIRE
- Subjects
[PHYS.NUCL] Physics [physics]/Nuclear Theory [nucl-th] ,magnetic moment ,Nuclear Theory ,[PHYS.NUCL]Physics [physics]/Nuclear Theory [nucl-th] ,new physics ,High Energy Physics::Lattice ,High Energy Physics::Phenomenology ,Hilbert space ,coupling constant ,quenching ,FOS: Physical sciences ,renormalization ,Nuclear Theory (nucl-th) ,symmetry: chiral ,effective field theory ,fixed point ,double-beta decay: (0neutrino) ,Fermi liquid ,nuclear matter ,quantum chromodynamics: effect ,Nuclear Experiment ,pi: decay constant - Abstract
When scale symmetry is combined with chiral symmetry in a scale-chiral Lagrangian, it can be shown in Fermi-liquid fixed point theory that $g_A^{\rm eff}\approx 1$ in finite nuclei {\it as well as} in dense baryonic matter. This is suggested as a signal for emergence of hidden symmetries of QCD in baryonic matter from low to very high density. This calculation throws doubt on the "first principles" explanation of the quenching of $g_A$ in nuclei with two-body meson-exchange currents. It also has relevance to Gamow-Teller matrix elements in neutrinoless double $\beta$ decay., Comment: 9 pages, 2 figures; this version gives a firmer conclusion
- Published
- 2019