Abstract
This paper is devoted to the investigation of spatially homogeneous and anisotropic Bianchi type-III massive scalar field model in the presence of anisotropic dark energy. We have constructed a deterministic cosmological model using some relevant physical and mathematical conditions. We obtain analytical solution of average scale factor and determine various cosmological parameters. We have also obtained the massive scalar field in the model and the graphical description of all the dynamical parameters is presented. A detailed discussion of the above dynamical quantities is, also, included.
Full Text 
Sign-in/Register to access full text options
Sign-in/Register to access full text options 
Published version (
Free)
Free) 
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a call
