The surface gravitational redshift of the neutron star PSR B2303+46
文献类型：期刊论文
| 作者 | Zhao, Xian-Feng1; Jia, Huan-Yu2 |
| 刊名 | BULLETIN OF THE ASTRONOMICAL SOCIETY OF INDIA
 |
| 出版日期 | 2013-12-01 |
| 卷号 | 41页码:291-298 |
| ISSN号 | 0304-9523 |
| 关键词 | Gravitation Stars: Neutron Pulsars: Individual: Psr b2303+46 |
| 文献子类 | Article |
| 英文摘要 | The surface gravitational redshift of the neutron star PSR B2303+ 46 is investigated within the framework of relativistic mean field theory for the baryon octet system through adjusting the hyperon coupling constants. We obtain any models for the neutron star B2303+ 46 by choosing suitable hyperon coupling constants chi(sigma h) and chi(omega h) with chi(rho h) being determined by SU(6) symmetry and the nucleon coupling constant being chosen as CZ11. Our calculations show that the radius and the surface gravitational redshift of the neutron star PSR B2303+ 46 are determined as R = 12: 477 similar to 12: 493 km and z = 0: 2184 similar to 0: 2187, respectively. Our results are not consistent with the recent discovery of the massive neutron star PSR J1614 2230 and PSR J0348+0432. |
| WOS关键词 | SIGMA(-) ATOMS ; HYPERNUCLEI ; PULSARS ; SPECTRUM ; PI(-) |
| 语种 | 英语 |
| 出版者 | INDIAN INST ASTROPHYSICS |
| WOS记录号 | WOS:000342398700004 |
| 源URL | [http://119.78.100.186/handle/113462/48215]  |
| 专题 | 中国科学院近代物理研究所 |
| 通讯作者 | Zhao, Xian-Feng |
| 作者单位 | 1.Chuzhou Univ, Coll Mech & Elect Engn, Chuzhou 239000, Peoples R China 2.Southwest Jiaotong Univ, Inst Modern Phys, Chengdu 610031, Peoples R China |
| 推荐引用方式 GB/T 7714 | Zhao, Xian-Feng,Jia, Huan-Yu. The surface gravitational redshift of the neutron star PSR B2303+46[J]. BULLETIN OF THE ASTRONOMICAL SOCIETY OF INDIA,2013,41:291-298. |
| APA | Zhao, Xian-Feng,&Jia, Huan-Yu.(2013).The surface gravitational redshift of the neutron star PSR B2303+46.BULLETIN OF THE ASTRONOMICAL SOCIETY OF INDIA,41,291-298. |
| MLA | Zhao, Xian-Feng,et al."The surface gravitational redshift of the neutron star PSR B2303+46".BULLETIN OF THE ASTRONOMICAL SOCIETY OF INDIA 41(2013):291-298. |
入库方式： OAI收割
来源：近代物理研究所
浏览0
下载0
收藏0
其他版本
除非特别说明，本系统中所有内容都受版权保护，并保留所有权利。