2007Journal of Dynamical Systems and Geometric TheoriesRequires access

A Bianchi Type -V Cosmological Model in Brans - Dicke Theory of Gravitation

D. R. K. Reddy, Atchuta Rao, N. Premeshwari Devi, R. L. Naidu

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Abstract

Bianchi type - V space time is considered in the presence of perfect fluid source in the scalar - tensor theory of gravitation proposed by Brans and Dicke [Phys. Rev.124, 925,1961]. With the help of special law of variation for Hubble’s parameter presented by Bermann [Nuovo Cimento B74, 182, 1983] a cosmological model with negative constant deceleration parameter is obtained in the presence of perfect fluid with disordered radiation. Some physical and kinematical properties of the model are also discussed.

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Bianchi type - V space time is considered in the presence of perfect fluid source in the scalar - tensor theory of gravitation proposed by Brans and Dicke [Phys. Rev.124, 925,1961]. With the help of special law of variation for Hubble’s parameter presented by Bermann [Nuovo Cimento B74, 182, 1983] a cosmological model with negative constant deceleration parameter is obtained in the presence of perfect fluid with disordered radiation. Some physical and kinematical properties of the model are also discussed.

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Available abstract

Bianchi type - V space time is considered in the presence of perfect fluid source in the scalar - tensor theory of gravitation proposed by Brans and Dicke [Phys. Rev.124, 925,1961]. With the help of special law of variation for Hubble’s parameter presented by Bermann [Nuovo Cimento B74, 182, 1983] a cosmological model with negative constant deceleration parameter is obtained in the presence of perfect fluid with disordered radiation. Some physical and kinematical properties of the model are also discussed.

Key concepts: Physics, Scalar–tensor theory, Perfect fluid, Brans–Dicke theory, Gravitation, Hubble's law, Mathematical physics, Deceleration parameter

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