Extended decoupled anisotropic solutions in f(?,???? ,?????????) gravity

In this paper, we consider static spherical structure to develop some anisotropic solutions by employing the extended gravitational decoupling scheme in background of [Formula: see text] gravity, where and indicate Ricci scalar trace energy–momentum tensor, respectively. We transform both radial as well temporal metric functions apply them on field equations that produce two different sets corresponding parameter text]. The first set is associated with isotropic distribution, i.e. modified Krori–Barua solution. second influenced from factor contains unknowns which are determined taking constraints. impact then analyzed obtained physical variables anisotropy. also investigate energy conditions other parameters such mass, compactness redshift graphically. It found our solution pressure-like constraint shows stable behavior throughout gravity for considered range