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Advances in High Energy Physics
Volume 2014, Article ID 859638, 9 pages
Research Article

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

1School of Mathematical Sciences, Swami Ramanand Teerth Marathwada University, Vishnupuri, Nanded 431 606, India
2Mungsaji Maharaj Mahavidyalay, Darwha,Yavatmal, India

Received 2 April 2014; Revised 14 July 2014; Accepted 23 July 2014; Published 24 August 2014

Academic Editor: George Siopsis

Copyright © 2014 D. D. Pawar and Y. S. Solanke. This is an open access article distributed under the Creative Commons Attribution License, which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited. The publication of this article was funded by SCOAP3.


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 and a uniform magnetic field of energy density . 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.