Abstract: Some locally rotationally symmetric (LRS) Bianchi type I cosmological model of universe filled with dark energy from a wet dark fluid in the presence and absence of magnetic field is in investigated in general theory of relativity . We assume F 23 is non vanishing component of F ij . We obtain exact solutions to the field equation, where a relation between metric potential = is considered. The geometrical and kinematical properties of the models and the behaviours of the anisotropy of the dark energy have been carried out. Keywords: Bianchi type-I space-time, Magnetic field Wet dark fluid, Dark energy. I.INTRODUCTION The nature of the dark energy component of the univers
In the current study, we studied a fQ-gravitational, anisotropic, locally rotationally symmetric (LR...
We have studied the interacting and non-interacting dark energy and dark matter in the spatially hom...
In this paper, we present a class of solutions of Barber’s second self creation field equations desc...
We study anisotropic universe in the presence of magnetized dark energy. Bianchi type-V cosmological...
We study anisotropic universe in the presence of magnetized dark energy. Bianchi type-V cosmological...
The present study deals with spatial homogeneous and anisotropic locally rotationally symmetric (LRS...
Abstract. The Bianchi Type-I Universe filled with dark energy from a wet dark fluid has been conside...
Locally rotationally symmetric Bianchi type I cosmological models are examined in the presence of dy...
Today dark energy cosmological models have become essential to explain the accelerated expansion of ...
In this study, locally rotationally symmetric Bianchi type IV universe is considered in Einstein's g...
Today dark energy cosmological models have become essential to explain the accelerated expansion of ...
We investigated Bianchi type-I magnetized dark energy cosmological model in bimetric theory of gravi...
The spatially homogeneous but totally anisotropic and non-flat Bianchi type-II cosmological model ha...
The spatially homogeneous but totally anisotropic and non-flat Bianchi type-II cosmological model ha...
The present paper deals with Bianchi type IX cosmological model with magnetized anisotropic dark ene...
In the current study, we studied a fQ-gravitational, anisotropic, locally rotationally symmetric (LR...
We have studied the interacting and non-interacting dark energy and dark matter in the spatially hom...
In this paper, we present a class of solutions of Barber’s second self creation field equations desc...
We study anisotropic universe in the presence of magnetized dark energy. Bianchi type-V cosmological...
We study anisotropic universe in the presence of magnetized dark energy. Bianchi type-V cosmological...
The present study deals with spatial homogeneous and anisotropic locally rotationally symmetric (LRS...
Abstract. The Bianchi Type-I Universe filled with dark energy from a wet dark fluid has been conside...
Locally rotationally symmetric Bianchi type I cosmological models are examined in the presence of dy...
Today dark energy cosmological models have become essential to explain the accelerated expansion of ...
In this study, locally rotationally symmetric Bianchi type IV universe is considered in Einstein's g...
Today dark energy cosmological models have become essential to explain the accelerated expansion of ...
We investigated Bianchi type-I magnetized dark energy cosmological model in bimetric theory of gravi...
The spatially homogeneous but totally anisotropic and non-flat Bianchi type-II cosmological model ha...
The spatially homogeneous but totally anisotropic and non-flat Bianchi type-II cosmological model ha...
The present paper deals with Bianchi type IX cosmological model with magnetized anisotropic dark ene...
In the current study, we studied a fQ-gravitational, anisotropic, locally rotationally symmetric (LR...
We have studied the interacting and non-interacting dark energy and dark matter in the spatially hom...
In this paper, we present a class of solutions of Barber’s second self creation field equations desc...