Bianchi type-VI0\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$\mathrm{VI}_{0}$\end{document} anisotropic dark energy model in Brans–Dicke theory of gravitation

被引：0

作者：

V. U. M. Rao

V. Jayasudha

机构：

[1] Andhra University,Department of Applied Mathematics

来源：

Astrophysics and Space Science | 2015年 / 358卷 / 2期

关键词：

Brans–Dicke theory; Dark energy; Bianchi type models;

D O I：

10.1007/s10509-015-2412-6

中图分类号：

学科分类号：

摘要：

In this paper, we have considered Bianchi type-VI0\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$\mathrm{VI}_{0}$\end{document} space-time in the presence of anisotropic dark energy in Brans–Dicke (Phys. Rev. 124:925, 1961). Scalar-tensor theory of gravitation. Three different time dependent skewness parameters along spatial directions are introduced to represent the deviations of pressure from isotropy. Special law of variation for the mean Hubble parameter and variable equation of state (EoS) parameter are used to obtain a determinate solution of the field equations. Some properties of the model are also discussed.

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