Bianchi Type-V Dark Energy Model in a Scalar-Tensor Theory of Gravitation

被引：37

作者：

Naidu, R. L. ^{[1
]}

Satyanarayana, B. ^{[1
]}

Reddy, D. R. K. ^{[2
]}

机构：

[1] GMR Inst Technol, Dept Basic Sci & Humanities, Rajam 532127, Andhra Pradesh, India

[2] MVGR Coll Engn, Dept Sci & Humanities, Vizianagaram, Andhra Pradesh, India

来源：

INTERNATIONAL JOURNAL OF THEORETICAL PHYSICS | 2012年 / 51卷 / 07期

关键词：

Bianchi type-V universe; Dark energy; Scalar- tensor theory; UNIVERSE;

D O I：

10.1007/s10773-012-1078-x

中图分类号：

O4 [物理学];

学科分类号：

0702 ;

摘要：

A spatially homogeneous and anisotropic Bianchi type-V universe with variable equation of state (EoS) parameter and constant deceleration parameter is obtained in a scalar-tensor theory of gravitation proposed by Saez and Ballester (Phys. Lett. A 113:467, 1986). The physical and kinematical properties of the universe have been discussed.

引用

页码：1997 / 2002

页数：6

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