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nucl-th2001
Can weakly bound heavy nuclei with very large neutron excess exist?
M. Baldo, U. Lombardo, E. E. Saperstein +1
A realistic model is suggested based on the quasiparticle Lagrange version of the self-consistent Finite Fermi Systems theory supplemented with the microscopically calculated surfa…
nucl-th1996
Microscopic Nuclear Equation of State with Three-Body Forces and Neutron Star Structure
M. Baldo, G. F. Burgio, I. Bombaci
We calculate static properties of non-rotating neutron stars (NS's) using a microscopic equation of state (EOS) for asymmetric nuclear matter. The EOS is computed in the framework…