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nucl-th2006★ 38 cited
Spin polarized neutron matter within the Dirac-Brueckner-Hartree-Fock approach
F. Sammarruca, P. G. Krastev
The relation between energy and density (known as the nuclear equation of state) plays a major role in a variety of nuclear and astrophysical systems. Spin and isospin asymmetries…
nucl-th2006
Neutron star properties and the equation of state of neutron-rich matter
Plamen G. Krastev, Francesca Sammarruca
We calculate total masses and radii of neutron stars (NS) for pure neutron matter and nuclear matter in beta-equilibrium. We apply a relativistic nuclear matter equation of state (…