126 citations · 349 across the 6 of their papers we have counts for
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Cassiopeia A and direct URCA cooling
G. Taranto, G. F. Burgio, H. -J. Schulze
We model neutron star cooling, in particular the current rapid cooldown of the neutron star Cas A, with a microscopic nuclear equation of state featuring strong direct Urca process…
Constraining and applying a generic high-density equation of state
Mark G. Alford, G. F. Burgio, Sophia Han +2
We discuss the "constant speed of sound" (CSS) parametrization of the equation of state of high-density matter and its application to the field correlator method (FCM) model of qua…
Nucleon effective masses within the Brueckner-Hartree-Fock theory: Impact on stellar neutrino emission
M. Baldo, G. F. Burgio, H. -J. Schulze +1
We calculate the effective masses of neutrons and protons in dense nuclear matter within the microscopic Brueckner-Hartree-Fock many-body theory and study the impact on the neutrin…
Selecting microscopic Equations of State
G. Taranto, M. Baldo, G. F. Burgio
We compare a set of equations of state derived within microscopic many-body approaches, and study their predictions as far as phenomenological data on nuclei from heavy ion collisi…
Constraints on the quark matter equation of state from astrophysical observations
G. F. Burgio, H. Chen, H. -J. Schulze +1
We calculate the structure of neutron star interiors comprising both the hadronic and the quark phases. For the hadronic sector we employ a microscopic equation of state involving…