Speaker
Prof.
hesham mansour
(Physics department,faculty of science,Cairo university,Egypt)
Description
Static properties of nuclear matter e.g., binding energy, symmetry energy, etc.; can be determined by the (EOS), the (EOS) of nuclear matter has been of great interest in nuclear physics and astrophysics. The interest in the equation of state (EOS) of nuclear matter stems from different motivations and prospects. First, it appears as a theoretical challenge to the possibility of predicting, based on the meson theory of nucleon-nucleon interaction, the EOS of nuclear matter in the density range of up to a few times the saturation density (central density of heavy nuclei). Three-body effects are studied for both asymmetric nuclear matter and pure neutron matter. The Brueckner-Hartree-Fock (BHF) approximation + two- body density dependent Skyrme potential are used using CD-BonnB and Argonne V18 potential. Good agreement is obtained with other theoretical calculation.
Primary author
Prof.
hesham mansour
(Physics department,faculty of science,Cairo university,Egypt)