English

A Bottom-Up EFT Approach To Superdense Baryonic Matter

Nuclear Theory 2025-12-01 v2 High Energy Astrophysical Phenomena Solar and Stellar Astrophysics High Energy Physics - Phenomenology

Abstract

How to arrive at the densest matter in massive compact stars starting from Walecka's linear ω\omega-σ\sigma 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 vpcs2/c21/3v_{pcs}^2/c^2\approx 1/3 but the trace of the energy-momentum tensor is not equal to zero, hence the matter is non-conformal.

Keywords

Cite

@article{arxiv.2511.21141,
  title  = {A Bottom-Up EFT Approach To Superdense Baryonic Matter},
  author = {Mannque Rho},
  journal= {arXiv preprint arXiv:2511.21141},
  year   = {2025}
}

Comments

6 pages, 2 figures, typos corrected

R2 v1 2026-07-01T07:55:45.368Z