We present a solution of LRS Bianchi type-II space-time with string viscous fluid and magnetic field by solving the Barber’s field equations of self-creation theory of gravitation and it is seen that Barber scalar function affects the other physical parameters of the model and contributes a very high matter density, with high particle density at early stage of the universe and also it contributes the negative role of bulk viscous fluid in the evolution. Other geometrical and physical aspects of the model are also studied
The present study deals with locally rotationally symmetric (LRS) Bianchi type II string cosmologica...
Bianchi type-III string cosmological models are investigated in the presence of string fluid as a so...
The present study deals with locally rotationally symmetric (LRS) Bianchi type II string cosmologica...
In this paper, we present a class of solutions of Barber’s second self creation field equations desc...
In this paper, LRS Bianchi type I string fluid cosmological model with magnetic field in bimetric th...
A five-dimensional Bianchi type-I space-time is considered in the presence of a perfect fluid source...
In the presence of both magnetic field and bulk viscosity, Bianchi Type I bulk viscous fluid string ...
A five-dimensional Bianchi type-I space-time is considered in the presence of a perfect fluid source...
A five-dimensional Bianchi type-I space-time is considered in the presence of a perfect fluid source...
ABSTRACT: We have studied the Bianchi type-V string cosmological model filled with perfect fluid in ...
The present paper deals with Bianchi type IX cosmological model with magnetized anisotropic dark ene...
We study the Bianchi type-V cosmological model filled with perfect fluid in Barber\u27s second self-...
We study the Bianchi type-V cosmological model filled with perfect fluid in Barber\u27s second self-...
We study the Bianchi type-V cosmological model filled with perfect fluid in Barber\u27s second self-...
The present study deals with locally rotationally symmetric (LRS) Bianchi type II string cosmologica...
The present study deals with locally rotationally symmetric (LRS) Bianchi type II string cosmologica...
Bianchi type-III string cosmological models are investigated in the presence of string fluid as a so...
The present study deals with locally rotationally symmetric (LRS) Bianchi type II string cosmologica...
In this paper, we present a class of solutions of Barber’s second self creation field equations desc...
In this paper, LRS Bianchi type I string fluid cosmological model with magnetic field in bimetric th...
A five-dimensional Bianchi type-I space-time is considered in the presence of a perfect fluid source...
In the presence of both magnetic field and bulk viscosity, Bianchi Type I bulk viscous fluid string ...
A five-dimensional Bianchi type-I space-time is considered in the presence of a perfect fluid source...
A five-dimensional Bianchi type-I space-time is considered in the presence of a perfect fluid source...
ABSTRACT: We have studied the Bianchi type-V string cosmological model filled with perfect fluid in ...
The present paper deals with Bianchi type IX cosmological model with magnetized anisotropic dark ene...
We study the Bianchi type-V cosmological model filled with perfect fluid in Barber\u27s second self-...
We study the Bianchi type-V cosmological model filled with perfect fluid in Barber\u27s second self-...
We study the Bianchi type-V cosmological model filled with perfect fluid in Barber\u27s second self-...
The present study deals with locally rotationally symmetric (LRS) Bianchi type II string cosmologica...
The present study deals with locally rotationally symmetric (LRS) Bianchi type II string cosmologica...
Bianchi type-III string cosmological models are investigated in the presence of string fluid as a so...
The present study deals with locally rotationally symmetric (LRS) Bianchi type II string cosmologica...