Kaon condensation in neutron star matter

被引:0
|
作者
Guo, H [1 ]
Liu, B
Li, XG
Chen, YJ
机构
[1] Natl Lab Heavy Ion Accelerator Lanzhou, Ctr Nucl Theoret Phys, Lanzhou 730000, Peoples R China
[2] Peking Univ, Dept Tech Phys, Beijing 100871, Peoples R China
[3] Peking Univ, MOE Key Lab Heavy Ion Phys, Beijing 100871, Peoples R China
[4] Chinese Acad Sci, Inst High Energy Phys, Beijing 100039, Peoples R China
[5] Chinese Acad Sci, Inst Modern Phys, Lanzhou 730000, Peoples R China
关键词
kaon condensation; density dependent relativistic mean-field theory; neutron star matter;
D O I
暂无
中图分类号
O57 [原子核物理学、高能物理学];
学科分类号
070202 ;
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.
引用
收藏
页码:113 / 117
页数:5
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