21 citations · 25 across the 4 of their papers we have counts for
8 papers
The mass of odd-odd nuclei in microscopic mass models
W. Ryssens, G. Scamps, G. Grams +3
Accurate estimates of the binding energy of nuclei far from stability that cannot be produced in the laboratory are crucial to our understanding of nuclear processes in astrophysic…
Progress on Brussels-Skyrme atomic mass models on a grid: stiff neutron matter equation of state
Guilherme Grams, Wouter Ryssens, Guillaume Scamps +2
We report here the current developments on the Brussels-Skyrme-on-a-Grid (BSkG) atomic mass models. In comparison with our previous models, BSkG3 improves the infinite nuclear matt…
Confronting a set of Skyrme and predictions for the crust of neutron stars
Guilherme Grams, Jérôme Margueron, Rahul Somasundaram +1
With the improved accuracy of neutron star observational data, it is necessary to derive new equation of state where the crust and the core are consistently calculated within a uni…
Effects of modified dispersion relations on free Fermi gas: equations of state and applications in astrophysics
Luis C. N. Santos, Clésio E. Mota, Franciele M. da Silva +2
Deformed dispersion relations are considered in the study of equations of state of Fermi gas with applications to compact objects. Different choices of deformed energy relations ar…
Properties of neutron star crust with improved nuclear physics: Impact of chiral EFT interactions and experimental nuclear masses
Grams, G., Margueron +5
A compressible liquid-drop approach adjusted to uniform matter many-body calculations based on chiral EFT interactions and to the experimental nuclear masses is used to investigate…
Neutron star cooling and GW170817 constraint within quark-meson coupling models
Odilon Lourenço, César H. Lenzi, Mariana Dutra +6
In the present work we used five different versions of the quark-meson coupling (QMC) model to compute astrophysical quantities related to the GW170817 event and to neutron star co…