A Bottom-Up EFT Approach To Superdense Baryonic Matter
Mannque Rho

TL;DR
This paper develops a bottom-up theoretical framework combining symmetries and renormalization-group techniques to model superdense baryonic matter in compact stars, suggesting a topology change from hadrons to quarks without phase transition.
Contribution
It introduces a novel approach integrating hidden symmetries and topology change to describe dense matter, extending Walecka's model to higher densities with quark-hadron continuity.
Findings
Dense matter exhibits pseudo-conformal behavior with sound velocity around 1/3 of light speed.
Hadrons transform into quarks via topology change without a phase transition.
The model predicts non-conformal matter with a non-zero trace of the energy-momentum tensor.
Abstract
How to arrive at the densest matter in massive compact stars starting from Walecka's linear - mean-field model is described in a series of arguments anchored on hidden local symmetry, hidden scale symmetry and emergent parity-doublet symmetry. I follow the bottom-up approach from chiral symmetry with pions, coupled to hidden local and scale symmetry degrees of freedom. Exploiting the renormalization-group treatment \`a la Shankar and Polchinski of the fermionic interactions on the Fermi sphere, leading to Landau-Migdal Fermi-liquid, one obtains a sort of generalized ``Density Functional" that allows via a topology change hadrons transform to quarks without phase changes at the center of massive stars. The highly dense matter is ``pseudo-conformal" with the sound velocity but the trace of the energy-momentum tensor is not equal to zero, hence…
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Taxonomy
TopicsQuantum Chromodynamics and Particle Interactions · High-Energy Particle Collisions Research · Pulsars and Gravitational Waves Research
