报告人:Prof. Nguyen Van Giai (Institut de Physique Nucléaire, Université Paris-Sud/CNRS-IN2P3, F-91405 Orsay, France)
时间:
地点:东南大学物理系田家炳楼南楼203
摘要:
Neutron stars are very dense stellar objects whose mass is about 1.2 solar mass contained in a very limited volume of less than
简介:
1961 : Graduate of Ecole Polytechnique, Paris.
1963 : Graduate of Université Paris-Sud, Licencié en Sciences Physiques.
1972 : Graduate of Université Paris-Sud, Doctorat d’Etat en Physique.
September 2007 - present date: Directeur de Recherche Emérite, Centre National de
October 1, 1983-August 2007: Directeur de Recherche CNRS, Head of Groupe de Theoreque, Institut de Physique Nucléaire,
Prof.N.V. Giai is one of pioneers in developing the nuclear many-body theory. His well-quoted works include the relativistic Hartree-Fock approach for finite nuclei, relativistic random phase approximations for giant resonances, and non-relativistic approaches for various many-body systems as well. His current research activity covers mainly two fields where he is involved in theoretical studies: 1)Structure of unstable nuclei studied in a microscopic approach (non-relativistic and relativistic mean field, random phase approximation for particles and quasiparticles; 2)Effects of nuclear structure on the physics of neutron stars. He has authored and coauthored more than 250 publications. He is also an excellent organizer for many international collaborations and conferences. In recent years, he has pushed and operated a few Sino-French scientific collaboration programs.