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We have recently developed a set of equations of state based on the nuclearenergy density functional theory providing a unified description of thedifferent regions constituting the interior of neutron stars and magnetars. Thenuclear functionals, which were constructed from generalized Skyrme effectivenucleon-nucleon interactions, yield not only an excellent fit to essentiallyall experimental atomic mass data but were also constrained to reproduce theneutron-matter equation of state as obtained from realistic many-bodycalculations.

Unified description of dense matter in neutron stars and magnetars