Fig. 8

Mass M vs. radius R for non-rotating NS models
calculated using different assumptions concerning the structure of dense matter for
ρ > 2ρ0. Dotted
segments of M(R) curves: configurations unstable
with respect to small radial perturbations. N – nucleon matter, Argonne
V18+TBF nucleon interaction (Schulze
& Rijken 2011). B – baryon matter, EOS calculated using
hyperon-nucleon and hyperon-hyperon potentials Nijmegen ESC08 (Rijken et al. 2010a,b). Open
circles – configurations of maximum allowable mass, with central density given in
units of ρ0. BQ – hybrid stars with quark cores, when
reconfinement is not allowed. – hybrid
stars with stable quark cores, when the condition
is always satisfied and
the high-density reconfinement is allowed. Analytical EOS of quark matter in the CFL
state with ρ2 = 2.35ρ0,
aCFL = 0.5,
λCFL = 1.2. Enlarged rectangle: vicinity of
the high-density first-order phase transition Q→B (reconfinement). (This figure is
available in color in the electronic form.)
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