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The Nucleon Direct Urca Processes in a Cooling Neutron Star
Xu Y(许妍) ; Liu GZ(刘广洲) ; Liu CZ(刘承志) ; Fan CB(范存波) ; Wang HY(王红岩) ; Zhu MF(朱明枫) ; Zhao EG(赵恩广)
刊名Chinese physics letters
2013
期号12
合作状况国内
中文摘要In the relativistic mean field approximation, the relativistic energy losses of the nucleon direct Urca processes
are studied in the degenerate baryon matter of neutron stars. We investigate the effects of hyperon degrees of
freedom and the isovector scalar interaction which is considered by exchanging meson on the nucleon direct Urca
processes in neutron star matter. The results indicate that the existence of hyperons decreases the abundance of
protons and leptons and can sharply suppress the neutrino emissivity of the nucleon direct Urca processes, while
it has only a little influence on the neutrino luminosity for a fixed neutron star whether mesons appear in a
neutron star or not. However, the presence of mesons can result in obvious growth in the neutrino emissivity
and luminosity which will speed up the cooling rate for the nonsuperfluid neutron star.
收录类别SCI
公开日期2014-01-08
内容类型期刊论文
源URL[http://210.72.87.206/handle/60510005-5/79]  
专题长春人造卫星观测站_卫星轨道理论研究室_期刊论文
推荐引用方式
GB/T 7714
Xu Y,Liu GZ,Liu CZ,et al. The Nucleon Direct Urca Processes in a Cooling Neutron Star[J]. Chinese physics letters,2013(12).
APA Xu Y.,Liu GZ.,Liu CZ.,Fan CB.,Wang HY.,...&Zhao EG.(2013).The Nucleon Direct Urca Processes in a Cooling Neutron Star.Chinese physics letters(12).
MLA Xu Y,et al."The Nucleon Direct Urca Processes in a Cooling Neutron Star".Chinese physics letters .12(2013).
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