Anisotropic magnetized holographic Ricci dark energy cosmological models

被引：31
|
作者：
Santhi, M. Vijaya [1 ]
Rao, V. U. M. [1 ]
Aditya, Y. [1 ]
机构：
[1] Andhra Univ, Dept Appl Math, Visakhapatnam 530003, Andhra Prades, India
来源：
CANADIAN JOURNAL OF PHYSICS | 2017年 / 95卷 / 04期
关键词：
Bianchi type-III metric; Ricci dark energy; cosmology; general relativity; holographic dark energy; BIANCHI TYPE-I; DYNAMICS; UNIVERSE; DECELERATION;
D O I：
10.1139/cjp-2016-0781
中图分类号：
O4 [物理学];
学科分类号：
0702 ;
摘要：
In this paper, we have considered spatially homogeneous and anisotropic Bianchi type-III space-time filled with matter and anisotropic modified holographic Ricci dark energy in general relativity. We have solved Einstein's field equations using the following possibilities: (i) hybrid expansion law proposed by Akarsu et al. (JCAP, 01, 022 (2014)); (ii) a varying deceleration parameter considered by Mishra et al. (Int. J. Theor. Phys. 52, 2546 (2013)); and (iii) a linearly varying deceleration parameter given by Akarsu and Dereli (Int. J. Theor. Phys. 51, 612 (2012)). We have presented the cosmological models in each of the preceding cases and studied their evolutions. We have also discussed physical and kinematical properties of the models.
引用
收藏
页码：381 / 392
页数：12
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