Bianchi type-V dark energy cosmological model in general relativity in the presence of massive scalar field

In this paper, we discuss spatially homogeneous and anisotropic Bianchi type-V dark energy cosmological model in the presence of an attractive massive scalar field in general relativity. We have solved the field equations using (i) the shear scalar of the metric is proportional to the expansion scal...

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Main Authors: R.L. Naidu, Y. Aditya, D.R.K. Reddy
Format: Article
Language:English
Published: Elsevier 2019-05-01
Series:Heliyon
Subjects:
Online Access:http://www.sciencedirect.com/science/article/pii/S2405844019315348
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author R.L. Naidu
Y. Aditya
D.R.K. Reddy
author_facet R.L. Naidu
Y. Aditya
D.R.K. Reddy
author_sort R.L. Naidu
collection DOAJ
description In this paper, we discuss spatially homogeneous and anisotropic Bianchi type-V dark energy cosmological model in the presence of an attractive massive scalar field in general relativity. We have solved the field equations using (i) the shear scalar of the metric is proportional to the expansion scalar which results a relationship between metric potentials and (ii) a power law between the massive scalar field and the average scale factor. We have computed the cosmological parameters like dark energy density, equation of state parameter, skewness parameters, deceleration parameter and statefinder parameters of our dark energy model with massive strings and discussed their physical significance in the light of the recent scenario of accelerated expansion of the universe and cosmological observations.
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spelling doaj.art-30cf26a1f12645f5be32901ad21c969e2022-12-22T01:16:02ZengElsevierHeliyon2405-84402019-05-0155e01645Bianchi type-V dark energy cosmological model in general relativity in the presence of massive scalar fieldR.L. Naidu0Y. Aditya1D.R.K. Reddy2Department Mathematics, GMR Institute of Technology, Rajam, 532 127, IndiaDepartment of Mathematics, ANITS (A), Visakhapatnam, 531162, India; Corresponding author.Department of Applied Mathematics, Andhra University, Visakhapatnam, 530003, IndiaIn this paper, we discuss spatially homogeneous and anisotropic Bianchi type-V dark energy cosmological model in the presence of an attractive massive scalar field in general relativity. We have solved the field equations using (i) the shear scalar of the metric is proportional to the expansion scalar which results a relationship between metric potentials and (ii) a power law between the massive scalar field and the average scale factor. We have computed the cosmological parameters like dark energy density, equation of state parameter, skewness parameters, deceleration parameter and statefinder parameters of our dark energy model with massive strings and discussed their physical significance in the light of the recent scenario of accelerated expansion of the universe and cosmological observations.http://www.sciencedirect.com/science/article/pii/S2405844019315348Cosmology
spellingShingle R.L. Naidu
Y. Aditya
D.R.K. Reddy
Bianchi type-V dark energy cosmological model in general relativity in the presence of massive scalar field
Heliyon
Cosmology
title Bianchi type-V dark energy cosmological model in general relativity in the presence of massive scalar field
title_full Bianchi type-V dark energy cosmological model in general relativity in the presence of massive scalar field
title_fullStr Bianchi type-V dark energy cosmological model in general relativity in the presence of massive scalar field
title_full_unstemmed Bianchi type-V dark energy cosmological model in general relativity in the presence of massive scalar field
title_short Bianchi type-V dark energy cosmological model in general relativity in the presence of massive scalar field
title_sort bianchi type v dark energy cosmological model in general relativity in the presence of massive scalar field
topic Cosmology
url http://www.sciencedirect.com/science/article/pii/S2405844019315348
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