Charged anisotropic models with complexity-free condition

This paper uses the definition of complexity for a static spherically symmetric spacetime and extends it to case charged distribution. We formulate Einstein–Maxwell field equations corresponding anisotropic interior calculate two different mass functions. then take Reissner–Nordström metric as an exterior find matching conditions at spherical boundary. Some scalars are developed from orthogonal splitting curvature tensor, we call one them, i.e., YTF factor considered setup. Further, three independent not enough close system, therefore, adopt complexity-free condition. Along with this condition, consider constraints that lead models. also present graphical interpretation resulting solutions by choosing some particular values parameters. conclude models pr=0 polytropic equation state show viable stable behavior everywhere.