Energetic Interaction between Einstein’s Universe and a Source like-Tolman IV Complexity Factor

The energetic interaction between Einstein’s universe and a generic gravitational source like-Tolman IV complexity factor is studied. In this regard, we use the framework of Gravitational Decoupling by Extended Minimal Geometric Deformation and the concept of complexity for spherically symmetric fluid distributions. As a result of this interaction, we obtain a new physically realistic stellar model in the regime of anisotropic fluid pressure with high stability against gravitational cracking and gravitational collapse, which has a direct relationship with the absence of energy exchange in the inner shells.