The Composition of Baryon in the Proto Neutron Star PSR J0348+0432

被引:14
|
作者
Zhao, Xian-Feng [1 ]
机构
[1] Southwest Petr Univ, Sch Sci, Chengdu 610500, Sichuan, Peoples R China
关键词
Hyperon; Relativistic mean field thoery; Neutron star; MATTER;
D O I
10.1007/s10773-018-03997-2
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
The effect of the mesons f(0)(975)(named as f ), phi(1020)(named as phi) and on the properties of the proto neutron star PSR J0348 + 0432 is studied in the framework of the relativistic mean field theory considering the baryon octet. We find the central particle number density will decrease considering the mesons but will increase as the mesons f, phi or mesons f, phi and all being considered. We also find that the mesons f, phi and have little effect on the field strengths of mesons sigma and but have a greater influence on those of mesons . For the chemical potential of neutrons, the influence of these mesons is relative small but for the chemical potential of electrons the meson effect is relatively large. It is also found that the relative particle number density of n will decrease while those of p and sigma(-) will increase considering the effect of the mesons , or f, phi, or f, phi and . The relative particle number density of , sigma(0), sigma(+), (-) and (0) will decrease considering the effect of the mesons but will increase as the mesons f, phi or the mesons f, phi and all being considered.
引用
收藏
页码:1060 / 1070
页数:11
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