Physical origin of density dependent forces of Skyrme type within the quark meson coupling model

被引:97
作者
Guichon, PAM [1 ]
Matevosyan, HH
Sandulescu, N
Thomas, AW
机构
[1] CEA Saclay, SPhN, DAPNIA, F-91191 Gif Sur Yvette, France
[2] Thomas Jefferson Natl Accelerator Facil, Newport News, VA 23606 USA
[3] Louisiana State Univ, Dept Phys & Astron, Baton Rouge, LA 70803 USA
[4] Inst Phys & Nucl Engn, R-76900 Bucharest, Romania
[5] CEA, DAM, Serv Phys Nucl, F-91680 Bruyeres Le Chatel, France
基金
美国国家科学基金会;
关键词
D O I
10.1016/j.nuclphysa.2006.04.002
中图分类号
O57 [原子核物理学、高能物理学];
学科分类号
070202 ;
摘要
A density dependent, effective nucleon-nucleon force of the Skyrme type is derived from the quark-meson coupling model-a self-consistent, relativistic quark level description of nuclear matter. This new formulation requires no assumption that the mean scalar field is small and hence constitutes a significant advance over earlier work. The similarity of the effective interaction to the widely used SkM* force encourages us to apply it to a wide range of nuclear problems, beginning with the binding energies and charge distributions of doubly magic nuclei. Finding acceptable results in this conventional arena, we apply the same effective interaction, within the Hanree-Fock-Bogoliubov approach, to the properties of nuclei far from stability. The resulting two neutron drip lines and shell quenching are quite satisfactory. Finally, we apply the relativistic formulation to the properties of dense nuclear matter in anticipation of future application to the properties of neutron stars. (c) 2006 Elsevier B.V. All rights reserved.
引用
收藏
页码:1 / 19
页数:19
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