activity
19962026
most citedMicroscopic Nuclear Equation of State with Three-Body Forces and Neutron Star Structure

147 citations · 167 across the 5 of their papers we have counts for

collaborators

5 papers

nucl-th2026

Microscopic Optical Potential from Brueckner-Hartree-Fock Theory

Miao Qi, Li-Li Chen, Li-Gang Cao +4

Modern Brueckner-Hartree-Fock (BHF) calculations are very successful in describing various properties of symmetric and asymmetric nuclear matter. Within BHF theory a microscopic op…

nucl-th2018★ 10 cited

Proton-proton 1S0 pairing in neutron star

Wenmei Guo, J. M. Dong, X. Shang +4

The onset of 1S0 proton spin-singlet pairing in neutron-star matter is studied in the framework of the BCS theory including medium polarization effects. The strong three-body coupl…

nucl-th2002★ 10 cited

Short-range Effects on Nuclear Pairing

W. Zuo, U. Lombardo, H. -J. Schulze +1

We determine the influence of the three-body force and the medium modification of meson masses on pairing in nuclear and neutron matter. A reduction of the pairing gap is found and…

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★ 147 cited

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…