Slowly rotating neutron stars and hadronic stars in the chiral SU(3) quark mean-field model
文献类型：期刊论文
| 作者 | Yin, Shaoyu1; Zang, Jiadong2; Su, Ru-Keng1,2,3 |
| 刊名 | EUROPEAN PHYSICAL JOURNAL A
 |
| 出版日期 | 2010-03 |
| 卷号 | 43页码:295-301 |
| ISSN号 | 1434-6001 |
| DOI | 10.1140/epja/i2010-10916-0 |
| 英文摘要 | The equations of state for neutron matter, strange and non-strange hadronic matter in the chiral SU(3) quark mean-field model are applied in the study of slowly rotating neutron stars and hadronic stars. The radius, mass, moment of inertia, and other physical quantities are carefully examined. The effect of the nucleon crust for the strange hadronic star is exhibited. Our results show that the rotation can increase the maximum mass of compact stars significantly. For a big enough mass of pulsars which cannot be explained as strange hadronic stars, theoretical approaches to increase the maximum mass are addressed. |
| WOS关键词 | MAXIMUM MASS ; DIFFERENTIAL ROTATION ; GENERAL-RELATIVITY ; STRANGE STARS ; HYBRID STARS ; MATTER ; STATE ; EQUATION ; DENSITIES ; PHASES |
| WOS研究方向 | Physics |
| 语种 | 英语 |
| WOS记录号 | WOS:000275161800005 |
| 出版者 | SPRINGER |
| 源URL | [http://119.78.100.186/handle/113462/56898]  |
| 专题 | 中国科学院近代物理研究所 |
| 通讯作者 | Yin, Shaoyu |
| 作者单位 | 1.Fudan Univ, Dept Phys, Shanghai 200433, Peoples R China 2.China Ctr Adv Sci & Technol, World Lab, Beijing 100080, Peoples R China 3.Natl Lab Heavy Ion Collis, Ctr Theoret Nucl Phys, Lanzhou 730000, Peoples R China |
| 推荐引用方式 GB/T 7714 | Yin, Shaoyu,Zang, Jiadong,Su, Ru-Keng. Slowly rotating neutron stars and hadronic stars in the chiral SU(3) quark mean-field model[J]. EUROPEAN PHYSICAL JOURNAL A,2010,43:295-301. |
| APA | Yin, Shaoyu,Zang, Jiadong,&Su, Ru-Keng.(2010).Slowly rotating neutron stars and hadronic stars in the chiral SU(3) quark mean-field model.EUROPEAN PHYSICAL JOURNAL A,43,295-301. |
| MLA | Yin, Shaoyu,et al."Slowly rotating neutron stars and hadronic stars in the chiral SU(3) quark mean-field model".EUROPEAN PHYSICAL JOURNAL A 43(2010):295-301. |
入库方式： OAI收割
来源：近代物理研究所
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