Transitioning universe with hybrid scalar field in Bianchi I space-time

被引:34
|
作者
Yadav, Anil Kumar [1 ]
Alshehri, A. M. [2 ]
Ahmad, Nafis [2 ]
Goswami, G. K. [3 ]
Kumar, Mukesh [4 ]
机构
[1] United Coll Engn & Res, Dept Phys, Greater Noida 201310, India
[2] King Khalid Univ, Dept Phys, Coll Sci, POB 9004, Abha 61413, Saudi Arabia
[3] Netaji Subhas Univ Technol, Dept Math, Delhi, India
[4] GLA Univ, Dept Math, Mathura 281406, India
关键词
Brans-Dicke gravity; Scalar field; Cosmological parameters; Dark energy; Bianchi I space-time;
D O I
10.1016/j.dark.2020.100738
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
In this paper we investigate a Bianchi type I transitioning Universe in Brans-Dicke theory. To get an explicit solution of the field equations, we assume scalar field as phi = phi(0) [t(alpha)exp(beta t)](delta) with phi(0), alpha, beta and d as constants. The values of alpha and beta are obtained by probing the proposed model with recent observational Hubble data (OHD) points. The interacting and non-interacting scenarios between dark matter and dark energy of the derived Universe within the framework of Brans-Dicke gravity are investigated. The om(z) analysis of the Universe in derived model shows that the Universe is filled with dynamical dark energy with its equation of state parameter omega(de) > -1. Hence the Universe behaves like a quintessence model at present epoch. Some physical properties of the Universe are also discussed. (C) 2020 Elsevier B.V. All rights reserved.
引用
收藏
页数:9
相关论文
共 50 条