On the relativistic anisotropic configurations

被引:10
作者
Shojai, F. [1 ,2 ]
Kohandel, M. [3 ]
Stepanian, A. [1 ]
机构
[1] Univ Tehran, Dept Phys, Tehran, Iran
[2] Inst Res Fundamental Sci IPM, Sch Phys, Fdn Phys Grp, Tehran, Iran
[3] Alzahra Univ, Dept Chem & Phys, Tehran, Iran
来源
EUROPEAN PHYSICAL JOURNAL C | 2016年 / 76卷 / 06期
关键词
DYNAMICAL INSTABILITY; ENERGY DENSITY; SPHERES; MODELS; STARS; EQUATION; FLUIDS;
D O I
10.1140/epjc/s10052-016-4204-8
中图分类号
O412 [相对论、场论]; O572.2 [粒子物理学];
学科分类号
摘要
In this paper we study anisotropic spherical polytropes within the framework of general relativity. Using the anisotropic Tolman-Oppenheimer-Volkov equations, we explore the relativistic anisotropic Lane-Emden equations. We find how the anisotropic pressure affects the boundary conditions of these equations. Also we argue that the behavior of physical quantities near the center of star changes in the presence of anisotropy. For constant density, a class of exact solution is derived with the aid of a new ansatz and its physical properties are discussed.
引用
收藏
页数:8
相关论文
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