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This analysis demonstrates solutions to field equations in type III Bianchi Universes, highlighting domain wall behavior and metric potential relationships.
In this research we employ first model of f(R,T) gravitational theory f(R, T) = R + 2f(T) to explore the type III Bianchi Universe featuring domain wall. It was assumed that the expansion scalar is directly related to the shear scalar to find solution of the field equation. This results the metric potentials connection Z = kY n and the consideration of two scenarios for the integrating constant D. We observed that the domain wall existed early in the universe’s history and eventually vanished. A few of the model’s physical parameters are also covered.
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Junaid et al. (2025) studied this question.
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