Testing the density matrix expansion against ab initio calculations of trapped neutron drops

被引:44
作者
Bogner, S. K. [1 ,2 ]
Furnstahl, R. J. [3 ]
Hergert, H. [1 ,2 ]
Kortelainen, M. [4 ,5 ]
Maris, P. [6 ]
Stoitsov, M. [4 ,5 ]
Vary, J. P. [6 ]
机构
[1] Michigan State Univ, Natl Superconducting Cyclotron Lab, E Lansing, MI 48824 USA
[2] Michigan State Univ, Dept Phys & Astron, E Lansing, MI 48824 USA
[3] Ohio State Univ, Dept Phys, Columbus, OH 43210 USA
[4] Univ Tennessee, Dept Phys & Astron, Knoxville, TN 37996 USA
[5] Oak Ridge Natl Lab, Div Phys, Oak Ridge, TN 37831 USA
[6] Iowa State Univ, Dept Phys & Astron, Ames, IA 50011 USA
来源
PHYSICAL REVIEW C | 2011年 / 84卷 / 04期
基金
美国国家科学基金会;
关键词
CORE SHELL-MODEL; FOCK-BOGOLYUBOV EQUATIONS; PION-NUCLEON DYNAMICS; LIGHT-NUCLEI; SURFACE; C-12;
D O I
10.1103/PhysRevC.84.044306
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
Microscopic input to a universal nuclear energy density functional can be provided through the density matrix expansion (DME), which has recently been revived and improved. Several DME implementation strategies are tested for neutron drop systems in harmonic traps by comparing to Hartree-Fock (HF) and ab initio no-core full configuration (NCFC) calculations with a model interaction (Minnesota potential). The new DME with exact treatment of Hartree contributions is found to best reproduce HF results and supplementing the functional with fit Skyrme-like contact terms shows systematic improvement toward the full NCFC results.
引用
收藏
页数:9
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