3PF2 neutron superfluidity in neutron stars and three-body force effect

被引：0

作者：

Cui Chang-Xi ^{[1
]}

Zuo Wei ^{[1
]}

Schulze, H. J. ^{[2
]}

机构：

[1] Chinese Acad Sci, Inst Modern Phys, Lanzhou 730000, Peoples R China

[2] Ist Nazl Fis Nucl, Sez Catania, I-95123 Catania, Italy

来源：

CHINESE PHYSICS B | 2008年 / 17卷 / 09期

基金：

中国国家自然科学基金;

关键词：

(PF2)-P-3 superfluidity; neutron star; three-body force; Brueckner-Hartree-Fock approach;

D O I：

暂无

中图分类号：

O4 [物理学];

学科分类号：

0702 ;

摘要：

We investigate the (PF2)-P-3 neutron superfluidity in beta-stable neutron star matter and neutron stars by using the BCS theory and the Brueckner-Hartree-Fock approach. We adopt the Argonne V-18 potential supplemented with a microscopic three-body force as the realistic nucleon-nucleon interaction. We have concentrated on studying the three-body force effect on the (PF2)-P-3 neutron pairing gap. It is found that the three-body force effect is to enhance remarkably the (PF2)-P-3 neutron superfluidity in neutron star matter and neutron stars.

引用

页码：3289 / 3293

页数：5

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