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
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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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