14 0 50 100 150 APR SLY4 BSR10 TM1 NL3 2SC CFL APR BSR10 NL3 2SC CFL 350 400 450  (MeV) 0 50 100 150 0.5 1 $_{B}$ (fm$^{-3}$) G$_{D}$=1.1G$_{S}$ G$_{V}$=0 G$_{D}$=1.2G$_{S}$ G$_{V}$=0 p (MeV/fm 3 ) G$_{D}$=1.1G$_{S}$ G$_{V}$=0 G$_{D}$=1.2G$_{S}$ G$_{V}$=0 FIG. 2: (Color online) The pressure as a function of the quark chemical potential (left panel) and the baryon density (right panel) for the nuclear and quark matter. The EOSs for the quark matter in the 2SC and CFL phases are obtained within the NJL model using G$_{V}$ = 0 with G$_{D}$ = 1 . 1 G$_{S}$ and 1 . 2 G$_{S}$ . The solid circles on the various EOSs for the nuclear matter indicate the pressure at the center of the neutron star with the canonical mass (1 . 4 $^{M}$⊙ ).