Hypersurface-homogeneous cosmological models with anisotropic dark energy in Saez-Ballester theory of gravitation

被引:4
|
作者
Verma, M. K. [1 ]
Chandel, S. [2 ]
Shri Ram [2 ]
机构
[1] Baba Banarasi Das Natl Inst Technol & Management, Dept Math, Lucknow 227105, Uttar Pradesh, India
[2] Indian Inst Technol BHU, Dept Math Sci, Varanasi 221005, Uttar Pradesh, India
来源
PRAMANA-JOURNAL OF PHYSICS | 2017年 / 88卷 / 01期
关键词
Hypersurface-homogeneous models; dark energy; accelerating Universe; Saez-Ballester theory; VISCOUS-FLUID; EQUATION; UNIVERSE; COMPONENT;
D O I
10.1007/s12043-016-1317-4
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
The present study deals with hypersurface-homogeneous cosmological models with anisotropic dark energy in Saez-Ballester theory of gravitation. Exact solutions of field equations are obtained by applying a special law of variation of Hubble's parameter that yields a constant negative value of the deceleration parameter. Three physically viable cosmological models of the Universe are presented for the values of parameter K occurring in the metric of the space-time. The model for K = 0 corresponds to an accelerating Universe with isotropic dark energy. The other two models for K = 1 and -1 represent accelerating Universe with anisotropic dark energy, which isotropize for large time. The physical and geometric behaviours of the models are also discussed.
引用
收藏
页数:6
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