NONUNIFORM PAIRING GAP OF THE SUPERFLUID NEUTRONS IN THE CRUST OF NEUTRON-STARS

被引：0

作者：

LAZZARI, G ^{[1
]}

DEBLASIO, FV ^{[1
]}

机构：

[1] UNIV MILAN,DIPARTIMENTO FIS,I-20133 MILAN,ITALY

来源：

ACTA PHYSICA POLONICA B | 1994年 / 25卷 / 10期

关键词：

D O I：

暂无

中图分类号：

O4 [物理学];

学科分类号：

0702 ;

摘要：

We study the neutron superfluidity in the inner crust of a neutron star where a gas of unbound nucleons coexists with a lattice of neutron rich nuclei, using a Wigner-Seitz approximation and a well tested nuclear force. We found a neutron pairing energy gap which is generally larger outside the nuclear region. In order to clarify the relevance of our results we evaluate the pinning energy of vortices to nuclei and compare it with previous calculations.

引用

页码：1467 / 1474

页数：8

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[1] SEMICLASSICAL DESCRIPTION OF THE NEUTRON SUPERFLUID IN THE INNER CRUST OF NEUTRON-STARS
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[9] Role of finite nuclei on the pairing gap of the inner crust of neutron stars
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