Abstract
A hybrid equation of state (EoS) for dense matter is presented that satisfies phenomenological constraints from modern compact star (CS) observations which indicate high maximum masses ( M ∼ 2 M ⊙ ) and large radii ( R > 12 km ). The corresponding isospin symmetric EoS is consistent with flow data analyses of heavy-ion collisions. The transition from nuclear to two-flavor color superconducting quark matter at n crit ∼ 0.55 fm − 3 is almost a crossover.
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