“…All these parameters ( U; U'; J, J' , , , , ) are fitting parameters of the model, and they are determined by the requirement that the model charge densities, obtained self‐consistently, have to be as close as possible to the GGA ones. The model parameters can be found from minimization of the difference Δ = [ ρ GGA ( k,σ ) − ρ model ( k, σ ; U; U'; J, J' , )] 2 between the ab initio electron density ρ GGA ( k, σ ) and the model one ρ model ( k, σ ; U; U'; J, J' , ) with respect to interaction parameters . Since the Hartree–Fock equations have to be solved self‐consistently for each set of the model parameters, we simplified the problem further and instead of minimization of function Δ (i.e., the differences of the model and VASP electron spin densities in each point of space), we have chosen to fit the occupation numbers of d‐electrons, the magnetic moments of Mn‐atoms, and partial d‐densities of states for Mn atoms (see Equation in the study by Zhandun et al).…”