In general, achieving control of the nanoscale structure is of paramount importance for the design of novel materials with specific properties, leading to, for example, improved reaction rates and selectivity in catalysis (reduction of carbon dioxide), tailored magnetic behavior in electronics, and controlled growth of nanostructured materials (graphene). For binary alloys, the composition of the material in the surface region is of crucial importance in determining key properties, and is determined by complex self-diffusion and segregation mechanisms of the different atomic components. Close control of these processes would make tailoring of the material functionality possible by finely tuning the relative concentration of the alloy constituents. By means of a combined experimental and theoretical approach, we have studied this issue for the Ni-Cu system, where the above mechanisms were shown to be mostly defined by kinetic rather than energetic effects.
The processes taking place at the Ni/Cu(110) surface have been followed by high-energy-resolution X-ray photoelectron spectroscopy experiments performed at the SuperESCA beamline. Starting from a Ni coverage of 0.75 ML, XPS was used to monitor, at selected fixed temperatures, the real time evolution of the Cu and Ni core levels (Figure 1).
After preparation of the Ni ad-layer, the sample temperature was suddenly raised to the selected target value, following a step-like profile; a spectroscopic “movie” of the segregation process was then obtained. Due to the finite inelastic mean free path of the photoemitted electrons, upon diffusion of Ni atoms into the Cu bulk the Ni signal is screened by the atomic layers above. In parallel, as the Cu concentration at the surface increases, the Cu signal intensity raises. The Ni and Cu signal intensities are therefore related to the composition profile of the sample in the direction perpendicular to the surface. In order to obtain quantitative information, we modeled the diffusion process and optimized a set of parametric rate equations to fit the experimental intensities. Ni segregation energy barriers of increasing height were obtained when going deeper into the Cu(110) sample (from 1.2 to 2.0 eV, moving from the first layer to the bulk). In parallel, Density Functional Theory (DFT) ab-initio calculations modeled the most relevant processes, providing from the theory side diffusion and segregation energy barriers (Figure 2). multicols}
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Figure 1: Time evolution of the Cu and Ni 3p core level spectra at selected temperatures after Ni deposition at 170 K from the gas phase. The time decay of the Ni 3p XPS intensity and the parallel increase of the Cu 3p signal were reproduced by means of a simple kinetic model, which accounts for segregation energy barriers of Ni and Cu atoms, and for the inelastic mean free path of the photoelectrons that give rise to the experimental signal. Initial surface Ni coverage: 0.75 ML.
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