“…A scaling function, hsR(ξ K /ζ K , Z 2 /137), given in Ref. [8], is employed to correct for the Dirac-Hartree-Slater nature of the K shell. In this case, the relativistic correction, R, of ECPSSR is not necessary, and the modified cross-sections, σ eECPSShsR K , are given by,…”