326 citations · 2.9k across the 58 of their papers we have counts for
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Transport coefficients in neutron star cores in BHF approach. Comparison of different nucleon potentials
P S Shternin, M Baldo, H-J Schulze
Thermal conductivity and shear viscosity of npe matter in non-superfluid neutron star cores are considered in the framework of Brueckner-Hartree-Fock many-body theory. We extend…
Thermal states of neutron stars with a consistent model of interior
M. Fortin, G. Taranto, G. F. Burgio +3
We model the thermal states of both isolated neutron stars and accreting neutron stars in X-ray transients in quiescence and confront them with observations. We use an equation of…
Two-flavor hybrid stars with the Dyson-Schwinger quark model
J. -B. Wei, H. Chen, H. -J Schulze
We study the properties of two-flavor quark matter in the Dyson-Schwinger model and investigate the possible consequences for hybrid neutron stars, with particular regard to the tw…
Rotating hybrid stars with the Dyson-Schwinger quark model
J. -B. Wei, H. Chen, G. F. Burgio +1
We study rapidly rotating hybrid stars with the Dyson-Schwinger model for quark matter and the Brueckner-Hartree-Fock many-body theory with realistic two-body and three-body forces…