2015Prespacetime journalRequires access

A Tilted Cosmological Model in Brans-Dicke Theory of Gravitation

V. U. M. Rao, Gunnam Suryanarayana

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Abstract

In this paper, we have constructed titled Bianchi type- I cosmological model in Brans-Dicke scalar tensor theory of gravitation. To obtain a solution, it is assumed that expansion scalar is proportional to shear scalar which leads to a relation between metric potentials. Some physical and geometrical properties of the model are also discussed.

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What this paper is about

In this paper, we have constructed titled Bianchi type- I cosmological model in Brans-Dicke scalar tensor theory of gravitation. To obtain a solution, it is assumed that expansion scalar is proportional to shear scalar which leads to a relation between metric potentials. Some physical and geometrical properties of the model are also discussed.

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Available abstract

In this paper, we have constructed titled Bianchi type- I cosmological model in Brans-Dicke scalar tensor theory of gravitation. To obtain a solution, it is assumed that expansion scalar is proportional to shear scalar which leads to a relation between metric potentials. Some physical and geometrical properties of the model are also discussed.

Key concepts: Brans–Dicke theory, Scalar–tensor theory, Physics, Gravitation, Scalar theories of gravitation, Scalar (mathematics), Cosmological model, Mathematical physics

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