THE SURFACE GRAVITATIONAL REDSHIFT OF THE NEUTRON STAR PSR J1614-2230

被引：2
|
作者：
Zhao, Xian-Feng [1 ]
机构：
[1] Chuzhou Univ, Coll Mech & Elect Engn, Chuzhou 239000, Peoples R China
来源：
ACTA PHYSICA POLONICA B | 2013年 / 44卷 / 02期
关键词：
D O I：
10.5506/APhysPolB.44.211
中图分类号：
O4 [物理学];
学科分类号：
0702 ;
摘要：
Based on the hadronic level, the value range of the surface gravitational redshift of the neutron star PSR J1614-2230 is tried to be determined in the framework of the relativistic mean field theory. It is found that for the neutron star PSR J1614-2230 the ratio of mass M and radius R is in the range of similar to 0.1692 to 0.1958 and the surface gravitational redshift is in the range of similar to 0.4138 to 0.5397. However, for a small mass neutron star, which is calculated with the hyperon coupling constant obtained by the constituent quark model [SU(6) symmetry], the ratio of mass M and radius R is 0.1221 and the surface gravitational redshift is 0.2507. The surface gravitational redshift of the neutron star PSR J1614-2230 is about one times larger than that of the small mass neutron star. DOI:10.5506/APhysPolB.44.211
引用
收藏
页码：211 / 219
页数：9
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