326 citations · 4.3k across the 75 of their papers we have counts for
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Neutron Star masses from the Field Correlator Method Equation of State
D. Zappala, G. F. Burgio, V. Greco +1
We analyse the hadron-quark phase transition in neutron stars by confronting the hadronic Equation of State (EoS) obtained according to the microscopic Brueckner-Hartree-Fock many…
The neutron star in Cassiopeia A: equation of state, superfluidity, and Joule heating
A. Bonanno, M. Baldo, G. F. Burgio +1
The thermomagnetic evolution of the young neutron star in Cassiopea A is studied by considering fast neutrino emission processes. In particular, we consider neutron star models obt…
From the crust to the core of Neutron Stars on a microscopic basis
M. Baldo, G. F. Burgio, M. Centelles +2
Within a microscopic approach the structure of Neutron Stars is usually studied by modelling the homogeneous nuclear matter of the core by a suitable Equation of State, based on a…
Quark matter in Neutron Stars within the Field Correlator Method
S. Plumari, G. F. Burgio, V. Greco +1
We discuss the appearance of quark matter in neutron star cores', focussing on the possibility that the recent observation of a very heavy neutron star could constrain free paramet…
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…
Structure of the hadron-quark mixed phase in protoneutron stars
H. Chen, G. F. Burgio, H. -J. Schulze +1
We study the hadron-quark phase transition in the interior of hot protoneutron stars, combining the Brueckner-Hartree-Fock approach for hadronic matter with the MIT bag model or th…