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Hot quark matter and (proto-) neutron stars
(American Physical Society, 2019-07)
In the first part of this paper, we use a nonlocal extension of the three-flavor Polyakov-Nambu-Jona-Lasinio model, which takes into account flavor-mixing, momentum dependent quark masses, and vector interactions among ...
Third family of compact stars within a nonlocal chiral quark model equation of state
(American Physical Society, 2019-03)
A class of hybrid compact star equations of state is investigated that joins by a Maxwell construction a low-density phase of hadronic matter, modeled by a relativistic mean-field approach with excluded nucleon volume, ...