Influence of charge on extended decoupled anisotropic solutions in $$f ({\mathcal {R,T}},{\mathcal {R}}_{\lambda \xi }{\mathcal {T}}^{\lambda \xi })$$ gravity

In this paper, we consider static self-gravitating spherical spacetime and determine various anisotropic solutions through the extended gravitational decoupling technique in $f(\mathcal{R},\mathcal{T},\mathcal{R}_{\lambda\xi}\mathcal{T}^{\lambda\xi})$ gravity to analyze influence of electromagnetic field on them. We construct two different sets modified equations by employing transformations both radial as well temporal metric potentials. The first set symbolizes isotropic fluid distribution, thus take Krori-Barua solution deal with it. indefinite second sector comprises anisotropy. regard, apply some constraints unknowns. Further, observe impact charge parameter $\zeta$ developed physical variables (such energy density,~radial tangential pressures) also other features compact geometry like mass, compactness redshift along conditions. Eventually, find that our show less stable behavior for higher values near boundary gravity.