Tilted Bianchi Type IX Dust Fluid Cosmological Model in General Relativity

Bagora, Anita

doi:10.5402/2012/954043

ISRN Astronomy and Astrophysics

2012

DOI: 10.5402/2012/954043

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Tilted Bianchi Type IX Dust Fluid Cosmological Model in General Relativity

Anita Bagora

Abstract: Some tilted Bianchi type IX dust fluid cosmological model is investigated. To get a deterministic model we assume that a = b 1/2 , where a and b are metric potentials and the fluid is pressureless, that is, p = 0. Some physical and geometric properties of the model are discussed. Also, we have discussed a special model in terms of t only.

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2015

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Cited by 1 publication

References 26 publications

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Bianchi Type-IX Anisotropic Dark Energy Cosmological Models with Time Dependent Deceleration Parameter

Ghate¹,

Sontakke²,

Patil³

2015

IJAA

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Bianchi type-IX cosmological models with variable equation of state (EoS) parameter have been investigated in general relativity when universe is filled with dark energy. The field equations have been solved by considering (i) q B = (variable); (ii) q kt m 1 = − + − , where k and m are constants; (iii) 2 1 = − +. This renders early decelerating and late time accelerating cosmological models. The physical and geometrical properties of the models are also discussed.

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Bianchi Type-IX Anisotropic Dark Energy Cosmological Models with Time Dependent Deceleration Parameter

Ghate¹,

Sontakke²,

Patil³

2015

IJAA

View full text Add to dashboard Cite

show abstract

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Tilted Bianchi Type IX Dust Fluid Cosmological Model in General Relativity

Cited by 1 publication

References 26 publications

Bianchi Type-IX Anisotropic Dark Energy Cosmological Models with Time Dependent Deceleration Parameter

Bianchi Type-IX Anisotropic Dark Energy Cosmological Models with Time Dependent Deceleration Parameter

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