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Employing the Vienna ab initio simulation package (VASP), a possible nonequilibrium intermediate state located near ${\mathrm{Ag}}_{3}\mathrm{Ni}$ in the immiscible Ag-Ni system is predicted through calculating the total energy of six possible structures of ${A}_{3}B$ type as a function of their lattice constants. The predicted state is confirmed by the fact that a metastable hcp ${\mathrm{Ag}}_{3}\mathrm{Ni}$ phase was indeed obtained in the properly designed Ag-Ni multilayers upon 200 keV xenon ion irradiation at 77 K and its lattice constants determined by diffraction analysis were in good agreement with the calculated values.
he spontaneous formation and subsequent aggregation of planar V 6O 12clusters on a Rh(111) surface after deposition of V atoms at submonolayer coveragesunder appropriate temperature and sufficiently oxidizing conditions is monitored bySTM. The stoichiometry and the geometry of the obtained starlike structures are char-acterized by ab initio DFT calculations