High Density Quark Matter under Stress
P. F. Bedaque, T. Schaefer
TL;DR
This work analyzes how SU(3) flavor breaking, via a nonzero electron chemical potential $μ_e$ and finite strange quark mass $m_s$, affects high-density CFL quark matter. It builds a chiral EFT for CFL Goldstone modes, performs perturbative matching to QCD to fix $f_π$ and $O(M^4)$ operators, and uses linear response to show that $μ_e$ and $m_s^2/(2p_F)$ act as flavor gauge fields that induce kaon or pion condensation at scales well below the gap $Δ$. The main results are precise onset conditions $μ_e \sim \sqrt{m m_s}\,Δ/p_F$ and $m_s \sim m^{1/3}\,Δ^{2/3}$, with $f_π^2 = m_D^2$ and the $O(M^4)$ term fixed by matching; these findings illuminate the phase structure of dense quark matter and the role of Goldstone modes in neutron-star cores. Overall, the paper provides a coherent EFT framework linking microscopic QCD to the macroscopic behavior of stressed CFL matter and its potential astrophysical manifestations.
Abstract
We study the effect of SU(3) flavor breaking on high density quark matter. We discuss, in particular, the effect a non-zero electron chemical potential and a finite strange quark mass. We argue that these perturbations trigger pion or kaon condensation. The critical chemical potential behaves as $μ_e\sim\sqrt{m m_s} Δ/p_F$ and the critical strange quark mass as $m_s \sim m^{1/3} Δ^{2/3}$, where $m$ is the light quark mass, $Δ$ is the gap, and $p_F$ is the Fermi momentum. We note that parametrically, both the critical $μ_e$ and $m_s^2/(2p_F)$ are much smaller than the gap.
