Kaon Condensation in Baryonic Fermi Liquid at High Density
arXiv:1407.1611 · doi:10.1103/PhysRevC.91.015801
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 much greater than that of the pion -- are integrated out, then the resulting KN coupling Lagrangian consists of the leading chiral order () Weinberg-Tomozawa term and the next chiral order () term. In addressing kaon condensation in dense nuclear matter in chiral perturbation theory (ChPT), one makes an expansion in the "small" Fermi momentum . We argue that in the Wilsonian RG formalism with the Fermi-liquid fixed point, the expansion is on the contrary in with the "large" Fermi momentum . The kaon-quasinucleon interaction resulting from integrating out the massive mesons consists of a "relevant" term from the scalar exchange (analog to the term) and an "irrelevant" term from the vector-meson exchange (analog to the Weinberg-Tomozawa term). It is found that the critical density predicted by the latter approach, controlled by the relevant term, is three times less than that predicted by chiral perturbation theory.
arXiv comment26 pages and 6 figures, Revised for publication
References in corpus (30)
- Shapiro delay measurement of a two solar mass neutron star
- A Massive Pulsar in a Compact Relativistic Binary
- Renormalization Group Approach to Interacting Fermions
- Hidden Local Symmetry at Loop -- A New Perspective of Composite Gauge Boson and Chiral Phase Transition
- Maximal neutron star mass and the resolution of hyperon puzzle in modified gravity
- Effective Kbar N interaction based on chiral SU(3) dynamics
- An Effective Chiral Lagrangian Approach to Kaon-Nuclear Interactions: Kaonic atom and kaon condensation
- Formation of a topological non-Fermi liquid in MnSi
- Effective Lagrangian for Nonrelativistic Systems
- Non-Fermi liquid fixed point in a Wilsonian theory of quantum critical metals
- From Chiral Mean Field to Walecka Mean Field and Kaon Condensation
- Double Decimation and Sliding Vacua in the Nuclear Many-Body System
- Criterion for stability of Goldstone Modes and Fermi Liquid behavior in a metal with broken symmetry
- Interplay between ω-Nucleon Interaction and Nucleon Mass in Dense Baryonic Matter
- Dense Nuclear Matter: Landau Fermi-Liquid Theory and Chiral Lagrangian with Scaling
- Dispersion relations of Nambu-Goldstone modes at finite temperature and density
- Half-Skyrmions and the Equation of State for Compact-Star Matter
- Dense baryonic matter in conformally-compensated hidden local symmetry: Vector manifestation and chiral symmetry restoration
- Study of Strangeness Condensation by Expanding About the Fixed Point of the Harada-Yamawaki Vector Manifestation
- Recent Developments on Kaon Condensation and Its Astrophysical Implications
- Thermodynamic Properties of Effective Chiral Lagrangians with BR Scaling
- Anomalous Fermi liquid phase in metallic Skyrmion crystals
- Topology Change and Tensor Forces for the EoS of Dense Baryonic Matter
- Renormalization-Group Flow Analysis of Meson Condensations in Dense Matter
- Nucleon structure from lattice QCD - recent achievements and perspectives
- Hyperons and Condensed Kaons in Compact Stars
- A New Topological "Twist" to BR Scaling
- Effective Kbar N interaction and role of chiral symmetry
- Controlled non-Fermi liquids from spacetime dependent couplings
- Nuclear Symmetry Energy with Strangeness in Heavy Ion Collision
Cited by in corpus (8)
- Scale-Invariant Hidden Local Symmetry, Topology Change and Dense Baryonic Matter II
- Towards the Hadron-Quark Continuity Via a Topology Change in Compact Stars
- Cusp in the Symmetry Energy, Speed of Sound in Neutron Stars and Emergent Pseudo-Conformal Symmetry
- Scale-Invariant Hidden Local Symmetry, Topology Change and Dense Baryonic Matter
- Scalar Pseudo-Nambu-Goldstone Boson in Nuclei and Dense Nuclear Matter
- Topology change, emergent symmetries and compact star matter
- -matter: stable or unstable?
- Why {\em Explicit} Strangeness Is Not Relevant In Compact Stars