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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Detalles Bibliográficos
Autores principales: Naidu, R.L., Aditya, Y., Reddy, D.R.K.
Formato: Online Artículo Texto
Lenguaje:English
Publicado: Elsevier 2019
Materias:
Article
Acceso en línea:https://www.ncbi.nlm.nih.gov/pmc/articles/PMC6512874/
https://www.ncbi.nlm.nih.gov/pubmed/31192992
http://dx.doi.org/10.1016/j.heliyon.2019.e01645

Internet

https://www.ncbi.nlm.nih.gov/pmc/articles/PMC6512874/
https://www.ncbi.nlm.nih.gov/pubmed/31192992
http://dx.doi.org/10.1016/j.heliyon.2019.e01645

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