Neutrino emission from neutron stars

被引：0
|
作者：
Yakovlev, D. G. [1 ,2 ]
Gusakov, M. E. [1 ]
Kaminker, A. D. [3 ]
Potekhin, A. Y. [4 ,5 ]
机构：
[1] Ioffe Phys Tech Inst, Politekhnicheskaya 26, St Petersburg 194021, Russia
[2] Univ Calif Santa Barbara, Inst Theoret Phys, Santa Barbara, CA 93106 USA
[3] Inst Astron, Cambridge CB3 0HA, England
[4] Copernicus Astron Ctr, PL-00716 Warsaw, Poland
[5] Observ Paris, CNRS, Dept Astrophys Relativiste & Cosmol, UMR 8629du, F-92195 Meudon, France
来源：
EXOTIC NUCLEI AND NUCLEAR/PARTICLE ASTROPHYSICS | 2006年
基金：
俄罗斯基础研究基金会;
关键词：
D O I：
10.1142/9789812772862_0024
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
The main mechanisms of neutrino emission from the matter of supranuclear density in superfluid cores of neutron stars are reviewed, with the emphasis on the cores composed of nucleons. The effects of neutrino emission on the thermal evolution of neutron stars are described. The prospects of exploring the fundamental (but still poorly known) properties of supranuclear matter by comparing simulations of neutron star thermal evolution with observations are outlined.
引用
收藏
页码：205 / +
页数：2
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