Direct Urca Processes with Hyperons in Cooling Neutron Stars
超子中子星的冷却直接URCA过程作者机构:Center for Theoretical PhysicsJilin UniversityChangchun 130012 College of ScienceNanjing Forestry UniversityNanjing 210037 Institute of Theoretical PhysicsChinese Academy of SciencesBeijing 100190
出 版 物:《Chinese Physics Letters》 (中国物理快报(英文版))
年 卷 期:2011年第28卷第7期
页 面:334-337页
核心收录:
学科分类:07[理学] 070202[理学-粒子物理与原子核物理] 0702[理学-物理学]
基 金:by the National Natural Science Foundation of China under Grant Nos 10675024 and 11075063 the National Fundamental Project for Subsidy Funds of Personnel Training J0730311
主 题:processes relativistic sharply
摘 要:In the relativistic mean field approximation,the relativistic energy losses of the direct Urca processes with nucleons(N-DURCA)and hyperons(Y-DURCA)are studied in the degenerate baryon matter of neutron *** investigate the effects of hyperon degrees of freedom and the Y-DURCA processes on the N-DURCA processes,and the total neutrino emissivity of neutron star *** results show that the existence of hyperons decreases the abundance of protons and leptons,and can sharply suppress the neutrino emissivity of the N-DURCA processes.