Kantowski-Sachs and Bianchi type models with a general non-canonical scalar field
- Authors: Singh T.1,2, Chaubey R.1, Singh A.1
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Affiliations:
- DST-Centre for Interdisciplinary Mathematical Sciences
- Indian Institute of Advanced Study
- Issue: Vol 23, No 2 (2017)
- Pages: 195-200
- Section: Article
- URL: https://journals.rcsi.science/0202-2893/article/view/176081
- DOI: https://doi.org/10.1134/S0202289317020104
- ID: 176081
Cite item
Abstract
The paper deals with spatially homogeneous and anisotropic Kantowski-Sachs and Bianchi universes with a general non-canonical scalar field with the Lagrangian L = F(X) − Ω(ϕ), where \(X = \frac{1}{2}{\phi _i}{\phi ^i}\). We discuss a general non-canonical scalar field in three different cosmologies: (i) cosmology with a constant potential, Ω(ϕ) = Ω0 = const, (ii) cosmology with a constant equation-of-state parameter, i.e., γϕ = const, and (iii) cosmology with a constant speed of sound, i.e., cs2 = const. For a constant potential, we have shown that the k-essence Lagrangian and the Lagrangian of the present model are equivalent. Dissipation of anisotropy, when the universe is filled with a general non-canonical scalar field, is investigated. The existence of an average bounce in Kantowski-Sachs and locally rotationally symmetric Bianchi-I and Bianchi-III models is discussed in detail.
About the authors
T. Singh
DST-Centre for Interdisciplinary Mathematical Sciences; Indian Institute of Advanced Study
Author for correspondence.
Email: drtrilokisingh@yahoo.co.in
India, Varanasi; Shimla, H.P.
R. Chaubey
DST-Centre for Interdisciplinary Mathematical Sciences
Email: drtrilokisingh@yahoo.co.in
India, Varanasi
Ashutosh Singh
DST-Centre for Interdisciplinary Mathematical Sciences
Email: drtrilokisingh@yahoo.co.in
India, Varanasi