Extended decoupled anisotropic solutions in f(R, T, Rγχ Tγχ) gravity

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

Automated summary

In this paper, anisotropic solutions in static spherical structures are developed by employing the extended gravitational decoupling scheme. The impact of the decoupling parameter on physical variables and anisotropy is analyzed, and it is found that the solution corresponding to the pressure-like constraint shows stable behavior within the considered range.