“…One of the most successful approaches is based on the Random Phase Approximation (RPA), which makes use of the relaxed-core Hartree Fock (RCHF) approximation (N 2 3,4,9,60,61,63,64,70,112-114 ; CO 76,112 ) in order to describe core-orbital relaxation effects that may play an important role, e.g., in K-shell photoionization. At higher energies the RCHF approximation has also been used (CO 43,44,50,52,54,67,[115][116][117][118][119][120] , N 2 3 ).…”