“…The measurements performed by STAR Collaboration [5] demonstrate that, in the range √ −t < 0.2 GeV, the spin-flip events take place due to electromagnetic interaction only. In their turn, available data on the proton-proton EDS at lower energies [6][7][8] point to the fact that, in the interval 0.5 GeV < √ −t < 1.5 GeV, the spin-flip contributions affect the differential cross-section very slightly, and, thus, they could be considered negligible, in the leading approximation (detailed discussion of this matter can be found in a recent paper [9]). Therefore, in further, we assume their subdominance in the whole kinematic range relevant for the high-energy EDS of nucleons.…”