Dynamics of stellar filaments in f(G) gravity

被引：4
|
作者：
Sharif, M. [1 ]
Fatima, H. Ismat [1 ,2 ]
机构：
[1] Univ Punjab, Dept Math, Quaid E Azam Campus, Lahore 54590, Pakistan
[2] Queen Mary Coll, Dept Math, Lahore 54000, Pakistan
来源：
EUROPEAN PHYSICAL JOURNAL PLUS | 2017年 / 132卷 / 03期
关键词：
FRAGMENTATION; STABILITY;
D O I：
10.1140/epjp/i2017-11421-1
中图分类号：
O4 [物理学];
学科分类号：
0702 ;
摘要：
We discuss the dynamics of stellar filaments with cylindrical symmetry in the context of f(G) gravity. For this purpose, we consider the modified gravity coupled with a dissipative anisotropic fluid and construct scalar functions through orthogonal splitting of the Riemann tensor. We formulate the set of equations governing the evolution and structure of stellar filaments in terms of these scalars. Finally, we discuss all static solutions for cylindrical filaments with anisotropy as well as isotropy and conclude that stellar filaments are necessarily inhomogeneous in this gravity.
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收藏
页数：12
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