Charged anisotropic models for quark stars

被引：121

作者：

Sunzu, Jefta M. ^{[1
]}

Maharaj, Sunil D. ^{[1
]}

Ray, Subharthi ^{[1
]}

机构：

[1] Univ KwaZulu Natal, Astrophys & Cosmol Res Unit, Sch Math Stat & Comp Sci, ZA-4000 Durban, South Africa

来源：

ASTROPHYSICS AND SPACE SCIENCE | 2014年 / 352卷 / 02期

基金：

新加坡国家研究基金会;

关键词：

Quarks stars; Compact bodies; Einstein-Maxwell equations; EQUATION-OF-STATE; STRANGE STARS; RELATIVISTIC STARS; SPHERES; MASS;

D O I：

10.1007/s10509-014-1918-7

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We perform a detailed physical analysis for a class of exact solutions for the Einstein-Maxwell equations. The linear equation of state consistent with quark stars has been incorporated in the model. The physical analysis of the exact solutions is performed by considering the charged anisotropic stars for the particular nonsingular exact model obtained by Maharaj, Sunzu and Ray. In performing such an analysis we regain masses obtained by previous researchers for isotropic and anisotropic matter. It is also indicated that other masses and radii may be generated which are in acceptable ranges consistent with observed values of stellar objects. A study of the mass-radius relation indicates the effect of the electromagnetic field and anisotropy on the mass of the relativistic star.

引用

页码：719 / 727

页数：9

共 64 条

[1] Further stable neutron star models from f(R) gravity [J].