Magnetized Anisotropic Dark Energy Models in Barber’s Second Self-Creation Theory

The present paper deals with Bianchi type IX cosmological model with magnetized anisotropic dark energy by using Barber’s self-creation theory. The energy momentum tensor consists of anisotropic fluid with EoS parameter ω and a uniform magnetic field of energy density ρB. In order to obtain the exac...

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Main Authors: D. D. Pawar, Y. S. Solanke
Format: Article
Language:English
Published: Wiley 2014-01-01
Series:Advances in High Energy Physics
Online Access:http://dx.doi.org/10.1155/2014/859638
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author D. D. Pawar
Y. S. Solanke
author_facet D. D. Pawar
Y. S. Solanke
author_sort D. D. Pawar
collection DOAJ
description The present paper deals with Bianchi type IX cosmological model with magnetized anisotropic dark energy by using Barber’s self-creation theory. The energy momentum tensor consists of anisotropic fluid with EoS parameter ω and a uniform magnetic field of energy density ρB. In order to obtain the exact solution we have assumed that dark energy components and the components of magnetic field interact minimally and obey the law of conservation of energy momentum tensors. We have also used the special law of variation for the mean generalized Hubble parameter and power law relation between scalar field and scale factor. Some physical and kinematical properties of the models have been discussed.
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spelling doaj-art-09ed29f751cd4aec832b2a2d57f8af422025-08-20T03:55:27ZengWileyAdvances in High Energy Physics1687-73571687-73652014-01-01201410.1155/2014/859638859638Magnetized Anisotropic Dark Energy Models in Barber’s Second Self-Creation TheoryD. D. Pawar0Y. S. Solanke1School of Mathematical Sciences, Swami Ramanand Teerth Marathwada University, Vishnupuri, Nanded 431 606, IndiaMungsaji Maharaj Mahavidyalay, Darwha,Yavatmal, IndiaThe present paper deals with Bianchi type IX cosmological model with magnetized anisotropic dark energy by using Barber’s self-creation theory. The energy momentum tensor consists of anisotropic fluid with EoS parameter ω and a uniform magnetic field of energy density ρB. In order to obtain the exact solution we have assumed that dark energy components and the components of magnetic field interact minimally and obey the law of conservation of energy momentum tensors. We have also used the special law of variation for the mean generalized Hubble parameter and power law relation between scalar field and scale factor. Some physical and kinematical properties of the models have been discussed.http://dx.doi.org/10.1155/2014/859638
spellingShingle D. D. Pawar
Y. S. Solanke
Magnetized Anisotropic Dark Energy Models in Barber’s Second Self-Creation Theory
Advances in High Energy Physics
title Magnetized Anisotropic Dark Energy Models in Barber’s Second Self-Creation Theory
title_full Magnetized Anisotropic Dark Energy Models in Barber’s Second Self-Creation Theory
title_fullStr Magnetized Anisotropic Dark Energy Models in Barber’s Second Self-Creation Theory
title_full_unstemmed Magnetized Anisotropic Dark Energy Models in Barber’s Second Self-Creation Theory
title_short Magnetized Anisotropic Dark Energy Models in Barber’s Second Self-Creation Theory
title_sort magnetized anisotropic dark energy models in barber s second self creation theory
url http://dx.doi.org/10.1155/2014/859638
work_keys_str_mv AT ddpawar magnetizedanisotropicdarkenergymodelsinbarberssecondselfcreationtheory
AT yssolanke magnetizedanisotropicdarkenergymodelsinbarberssecondselfcreationtheory