Viscous String Cosmological Model with Electromagnetic Field in Saez Ballester Theory
Abstract
The framework of Saez-Ballester formalism is employed to study Bianchi Type III metrics, which is homogeneous and anisotropic, wherein the energy-momentum tensor is derived from a bulk viscous fluid containing one-dimensional strings embedded within an electromagnetic field. To obtain exact solutions, we utilized the proportionality relation between the expansion and shear scalars, as well as the average scale factor of a special form. In addition to the energy conditions, several dynamical and physical parameters were calculated, and their physical implications on cosmology were examined.
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