2 papers
nucl-th2025
Neutron Star Core-Crust Transition and Crustal Moment of Inertia: Systematic Implications of Higher-Order Symmetry Energy in the Nuclear Equation of State
W. M. Seif, A. S. Hashem
We investigate how higher-order symmetry-energy coefficients of the equation of state (EOS) describing core matter impact key neutron star (NS) properties at its crust inner…
nucl-th2025
Tidal deformability and compactness of neutron stars and massive pulsars from semi-microscopic equations of state
W. M. Seif, A. S. Hashem
Tidal deformability measures how NS can comfortably deform as a response to an applied tidal field. We use updated constraints on the mass, radius, and tidal deformability of neutr…