2014
DOI: 10.4236/ijaa.2014.41017
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Bianchi Type-IX Magnetized Dark Energy Model in Saez-Ballester Theory of Gravitation

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 density ρ 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.

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Cited by 7 publications
(6 citation statements)
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“…Katore et al [25] studied the Einstein-Rosen bulk viscous cosmological model and zero-mass scalar field in Lyra's geometry. Ghate and Sontakke [26], Asgar and Ansari [27], and Das and Sharma [28] studied the Bianchi type V cosmological models in Lyra's geometry with dark energy, in the presence of bulk viscous string; Sahu et al [29] studied the Bianchi type III cosmological model in Lyra's geometry, and Katore and Kapse [30] studied dynamics of Bianchi type VI 0 holographic dark energy models in general relativity and Lyra's geometry.…”
Section: Introductionmentioning
confidence: 99%
“…Katore et al [25] studied the Einstein-Rosen bulk viscous cosmological model and zero-mass scalar field in Lyra's geometry. Ghate and Sontakke [26], Asgar and Ansari [27], and Das and Sharma [28] studied the Bianchi type V cosmological models in Lyra's geometry with dark energy, in the presence of bulk viscous string; Sahu et al [29] studied the Bianchi type III cosmological model in Lyra's geometry, and Katore and Kapse [30] studied dynamics of Bianchi type VI 0 holographic dark energy models in general relativity and Lyra's geometry.…”
Section: Introductionmentioning
confidence: 99%
“…Many authors [16][17][18][19][20][21][22][23][24][25] have studied different aspects of Bianchi type-IX cosmological models in various theories of gravitation. Recently, Bianchi type-IX DE model in Brans-Dicke theory of gravitation has been studied [26].…”
Section:   Pmentioning
confidence: 99%
“…Anisotropic Bianchi Type-III dark energy model with time dependent deceleration parameter in Saez-Ballester theory have been investigated by Rahman and Ansari (2013). The Bianchi type-IX cosmological model with variable ω has been studied by Ghate and Sontakke (2014) in the scalar tensor theory of gravitation proposed by Saez and Ballester theory in the presence and absence of magnetic field of energy density ρ b .…”
Section: Introductionmentioning
confidence: 99%