Kaon Condensation in Baryonic Fermi Liquid at High Density
Won-Gi Paeng, Mannque Rho

TL;DR
This paper formulates kaon condensation in dense baryonic matter using a Wilsonian RG approach, revealing that the critical density for condensation is significantly lower than previous chiral perturbation theory predictions.
Contribution
It introduces a Wilsonian RG framework for kaon condensation, contrasting with traditional chiral perturbation theory, and identifies the dominant interactions influencing the critical density.
Findings
Critical density is three times lower with the RG approach.
Scalar exchange dominates the relevant interaction.
Vector meson exchange contributes an irrelevant term.
Abstract
We formulate kaon condensation in dense baryonic matter with anti-kaons fluctuating from the Fermi-liquid fixed point. This entails that in the Wilsonian RG approach, the decimation is effectuated in the baryonic sector to the Fermi surface while in the meson sector to the origin. In writing the kaon-baryon (KN) coupling, we will take a generalized hidden local symmetry Lagrangian for the meson sector endowed with a "mended symmetry" that has the unbroken symmetry limit at high density in which the Goldstone , scalar , and vectors (and ) and become massless. The vector mesons (and ) and can be identified as emergent (hidden) local gauge fields and the scalar as the dilaton field of the spontaneously broken scale invariance at chiral restoration. In matter-free space, when the vector mesons and the scalar meson -- whose masses are…
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