Dynamical Aspects of Bianchi Type VI0 Cosmological Model with Cosmic String and Dark Energy in f(T) Gravity

This paper deals with the investigations of a spatially homogeneous and anisotropic Bianchi-type VI0 dark energy coupled string cosmological model within the context of gravity, where T denotes the torsion scalar. We have obtained the exact solutions of highly non-linear field equations considering some physically plausible conditions. Some physical and kinematical properties of the constructed model have been discussed and presented graphically. Additionally, we have calculated a jerk parameter that fits the model and discussed the physical stability and acceptability of constructed modelsThis paper deals with the investigations of a spatially homogeneous and anisotropic Bianchi-type VI0 dark energy coupled string cosmological model within the context of gravity, where T denotes the torsion scalar. We have obtained the exact solutions of highly non-linear field equations considering some physically plausible conditions. Some physical and kinematical properties of the constructed model have been discussed and presented graphically. Additionally, we have calculated a jerk parameter that fits the model and discussed the physical stability and acceptability of constructed models