Dynamical aspects of anisotropic Bianchi type VI0 cosmological model with dark energy fluid and massive scalar field

被引：19

作者：

Aditya, Y. ^{[1
]}

Raju, K. D. ^{[2
,4
]}

Ravindranath, P. J. ^{[3
]}

Reddy, D. R. K. ^{[4
]}

机构：

[1] GMR Inst Technol, Dept Math, Rajam 532127, India

[2] ANITS A, Dept Math, Visakhapatnam 531162, Andhra Pradesh, India

[3] Rajiv Gandhi Mem Coll Engn & Technol, Dept Math, Nandyal, India

[4] Andhra Univ, Dept Appl Math, Visakhapatnam 530003, Andhra Pradesh, India

来源：

INDIAN JOURNAL OF PHYSICS | 2021年 / 95卷 / 02期

关键词：

Anisotropic cosmological model; Dark energy; Massive scalar field; Einstein's theory; MODIFIED GRAVITY; TIME; INFLATION;

D O I：

10.1007/s12648-020-01722-6

中图分类号：

O4 [物理学];

学科分类号：

0702 ;

摘要：

In this article, we investigate a spatially homogeneous and anisotropic Bianchi type VI0 cosmological model in the presence of dark energy fluid and an attractive massive scalar field in Einstein's theory of gravitation. The field equations are solved using the following conditions (1) scalar expansion is proportional to shear scalar of the space time and (2) a power law between the scalar field and the average scale factor of the universe. We have evaluated the cosmological parameters of the model and discussed their dynamical aspects with reference to the recent discovery of accelerated expansion of the universe.

引用

页码：383 / 389

页数：7

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