“…The phase diagram of quantum chromodynamics (QCD) is expected to contain color-superconducting regimes at sufficiently high densities and low temperatures [1,2,3,4,5,6,7]. Considering three (degenerate) quark flavors, the color-flavor locked (CFL) phase [8] is the ground-state for vanishing temperatures and asymptotically large densities [9,10]. At densities of potential relevance for compact stellar objects it is, however, not obvious how the splitting of Fermi surfaces due to finite quark masses and neutrality constraints is influencing the ground-state [11,12,13].…”