Stability analysis of some reconstructed cosmological models in f (G, T) gravity

被引:59
作者
Sharif, M. [1 ]
Ikram, Ayesha [1 ]
机构
[1] Univ Punjab, Dept Math, Quaid E Azam Campus, Lahore 54590, Pakistan
关键词
Reconstruction; Stability analysis; Modified gravity; GAUSS-BONNET THEORY; SINGULARITY; ENERGY;
D O I
10.1016/j.dark.2017.05.001
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The aim of this paper is to reconstruct and analyze the stability of some cosmological models against linear perturbations in f (G, T) gravity (G and T represent the Gauss-Bonnet invariant and trace of the energy-momentum tensor, respectively). We formulate the field equations for both general as well as particular cases in the context of isotropic and homogeneous universe model. We reproduce the cosmic evolution corresponding to de Sitter universe, power-law solutions and phantom/non-phantom eras in this theory using reconstruction technique. Finally, we study stability analysis of de Sitter as well as power-law solutions through linear perturbations. (C) 2017 Elsevier B.V. All rights reserved.
引用
收藏
页码:1 / 9
页数:9
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