arXiv · hep-ph/9411416
Renormalization-Group Flow Analysis of Meson Condensations in Dense Matter
Abstract
We present a renormalization-group (RG) flow argument for s-wave kaon condensation in dense nuclear-star matter predicted in chiral perturbation theory. It is shown that it is the {\it relevant} mass term together with {\it any} attractive interaction for the kaon in medium that triggers the instability. We show that a saddle point of multi-dimensional RG flow can imply a phase transition. Pion condensation is also analyzed along the same line of reasoning.
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Hyun Kyu Lee, Mannque Rho, Sang-Jin Sin. 1994-11-29. Renormalization-Group Flow Analysis of Meson Condensations in Dense Matter. https://doi.org/10.1016/0370-2693(95)00171-g
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