A Scalar Field Cosmological Model in a Modified Theory of Gravitation
T. Kanakavalli, G. Ananda Rao, D. R. K. Reddy
Abstract
T. Kanakavalli, G. Ananda Rao, D. R. K. Reddy
Abstract
This paper is devoted to the discussion of Bianchi type-III cosmological model in the frame work of f (R,T) gravity in the presence of two non-interacting matter sources, scalar field (quintessence or phantom) with scalar potential and matter contribution due to f (R,T) action where R is the Ricci scalar and T is the trace of the energy tensor. We have solved the field equations using the fact that scalar expansion is proportional to shear scalar of the space-time and presented the scalar field model in this theory. Finally, we have also discussed some physical and kinematical properties of the model.
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This paper is devoted to the discussion of Bianchi type-III cosmological model in the frame work of f (R,T) gravity in the presence of two non-interacting matter sources, scalar field (quintessence or phantom) with scalar potential and matter contribution due to f (R,T) action where R is the Ricci scalar and T is the trace of the energy tensor. We have solved the field equations using the fact that scalar expansion is proportional to shear scalar of the space-time and presented the scalar field model in this theory. Finally, we have also discussed some physical and kinematical properties of the model.
Key concepts: Quintessence, Physics, Scalar theories of gravitation, Scalar–tensor theory, Scalar field, Scalar (mathematics), Mathematical physics, f(R) gravity