Slowly rotating neutron stars and hadronic stars in the chiral SU(3) quark mean-field model

doi:10.1140/epja/i2010-10916-0

	Slowly rotating neutron stars and hadronic stars in the chiral SU(3) quark mean-field model
	Yin, Shaoyu 1; Zang, Jiadong 2; Su, Ru-Keng 1,2,3
刊名	EUROPEAN PHYSICAL JOURNAL A
	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
出版者	SPRINGER
WOS记录号	WOS:000275161800005
内容类型	期刊论文
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.