LRS Bianchi type-II minimally interacting holographic dark energy model in Saez-Ballester theory of gravitation

被引：12

作者：

Ramesh, G. ^{[1
]}

Umadevi, S. ^{[1
]}

机构：

[1] AU Coll Engn A, Dept Engn Math, Visakhapatnam, Andhra Pradesh, India

来源：

ASTROPHYSICS AND SPACE SCIENCE | 2016年 / 361卷 / 02期

关键词：

Bianchi type II universe; Holographic dark energy; Saez-Ballester theory; Scalar-tensor theory; VARYING DECELERATION PARAMETER; PROBE WMAP OBSERVATIONS; SCALAR-TENSOR THEORY; COSMOLOGICAL MODELS; UNIVERSE; DYNAMICS;

D O I：

10.1007/s10509-015-2645-4

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Field equations of Saez and Ballester (Phys. Lett. A 113:467, 1986) scalar-tensor theory are obtained in the presence of two minimally interacting fields; matter and holographic dark energy components in spatially homogeneous and anisotropic LRS Bianchi type-II space-time. An exact solution of the field equations is presented using linearly varying deceleration parameter proposed by Akarsu and Dereli (Int. J. Theor. Phys. 51:612, 2012) which represents a minimally interacting Bianchi type-II universe in Saez-Ballester theory of gravitation. Some physical and kinematical properties of the model are also studied.

引用

页码：1 / 5

页数：5

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