Superfluidity in beta-stable neutron star matter

被引：61

作者：

Elgaroy, O ^{[1
]}

Engvik, L ^{[1
]}

HjorthJensen, M ^{[1
]}

Osnes, E ^{[1
]}

机构：

[1] EUROPEAN CTR THEORET STUDIES NUCL PHYS & RELATED, TRENT, ITALY

来源：

PHYSICAL REVIEW LETTERS | 1996年 / 77卷 / 08期

关键词：

D O I：

10.1103/PhysRevLett.77.1428

中图分类号：

O4 [物理学];

学科分类号：

0702 ;

摘要：

In this work we present results for pairing gaps in beta-stable neutron star matter with electrons and muons using a Dirac-Brueckner-Hartree-Fock approach, starting with modern meson-exchange models for the nucleon-nucleon interaction. Results are given for superconducting S-1(0) protons and superfluid P-3(2) and D-1(2) neutrons. A comparison is made with recent nonrelativistic calculations, and the implications for neutron star cooling are discussed.

引用

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页码：1428 / 1431

页数：4

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