Bianchi Type-IX Magnetized Dark Energy Model in Saez-Ballester Theory of Gravitation - International Journal of Astronomy and Astrophysics

IJAA > Vol.4 No.1, March 2014

Bianchi Type-IX Magnetized Dark Energy Model in Saez-Ballester Theory of Gravitation ()

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Download as PDF (Size: 328KB) PP. 181-191

DOI: 10.4236/ijaa.2014.41017 4,767 Downloads 7,077 Views Citations

Author(s)

H. R. Ghate, Atish S. Sontakke

Affiliation(s)

Department of Mathematics, Jijamata Mahaidyalaya, Buldana, India.

ABSTRACT

The Bianchi type-IX cosmological model with variable ω has been studied in the scalar tensor theory of gravitation proposed by Saez and Ballester [Phys. Lett. A 113: 467, 1985] in the presence and absence of magnetic field of energy densityρ_b. A special law of variation of Hubble’s parameter proposed by Berman [Nuovo Cimento 74 B, 182, 1983] has been used to solve the field equations. The physical and kinematical properties of the model are also discussed.

KEYWORDS

Dark Energy; Magnetic Field; Bianchi Type-IX Universe; Scalar-Tensor Theory

Share and Cite:

Ghate, H. and Sontakke, A. (2014) Bianchi Type-IX Magnetized Dark Energy Model in Saez-Ballester Theory of Gravitation. International Journal of Astronomy and Astrophysics, 4, 181-191. doi: 10.4236/ijaa.2014.41017.

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