Probing of Casimir Wormholes Solutions in a Trace of the Energy Momentum Tensor Squared Gravity

Abstract

In this thesis, three different cases of Casimir wormholes have been studied in the framework of energy-momentum-tensor squared gravity. We have calculated b(r) using Casimir energy densities and found the integration constant using the flaring out condition. Analytical explanations and graphic illustrations are provided for the criteria of b(r). The active gravitational mass formula is used to calculate the WHs masses. We determined a Complexity factor for every scenario in order to evaluate the wormhole solution’s complexity.