Kaon condensation in neutron star matter
Guo, H; 刘波(理); Liu, B; Li, XG; Chen, YJ
刊名HIGH ENERGY PHYSICS AND NUCLEAR PHYSICS-CHINESE EDITION
2003
卷号27期号:2页码:#REF!
关键词kaon condensation density dependent relativistic mean-field theory neutron star matter
其他题名中子星物质中的K介子凝聚
通讯作者Guo, H (reprint author), Natl Lab Heavy Ion Accelerator Lanzhou, Ctr Nucl Theoret Phys, Lanzhou 730000, Peoples R China.
英文摘要The Kaon condensation in neutron star matter is calculated in the framework of the density dependent relativistic mean-field theory. The present results show that the critical density for the Kaon condensation is similar to 2.75rho(0), while the critical densities for the URCA process in neutron star matter are rho/rho(0) approximate to 3.16 for the parameter set fitted to the DB nucleon self-energies of nuclear mater with the momentum-dependent correction, and rho/rho(0) approximate to 2.25 for the parameter set without the momentum-dependent correction. Then, influences of the two different model parameter sets on the equation of state of neutron star matter are discussed.
学科主题Physics
类目[WOS]Physics, Nuclear ; Physics, Particles & Fields
收录类别SCI
WOS记录号WOS:000181047100006
公开日期2016-05-03
内容类型期刊论文
源URL[http://ir.ihep.ac.cn/handle/311005/226249]  
专题高能物理研究所_理论物理室
推荐引用方式
GB/T 7714
Guo, H,Liu B,Liu, B,et al. Kaon condensation in neutron star matter[J]. HIGH ENERGY PHYSICS AND NUCLEAR PHYSICS-CHINESE EDITION,2003,27(2):#REF!.
APA Guo, H,刘波,Liu, B,Li, XG,&Chen, YJ.(2003).Kaon condensation in neutron star matter.HIGH ENERGY PHYSICS AND NUCLEAR PHYSICS-CHINESE EDITION,27(2),#REF!.
MLA Guo, H,et al."Kaon condensation in neutron star matter".HIGH ENERGY PHYSICS AND NUCLEAR PHYSICS-CHINESE EDITION 27.2(2003):#REF!.
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