2007
DOI: 10.1016/j.msea.2007.01.040
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First-principles study of Sn adsorption on Ni(100), (110) and (111) surfaces

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Cited by 14 publications
(9 citation statements)
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“…For the Sn/Ni(110) surface, the atomic radius of Sn is about 20% larger than that of Ni, leading to compressive stress both in the [001] and [110] directions. The surface stress can be partly relieved by the outward relaxation of Sn, and 40±3 pm protrusion was reported by low-energy electron diffraction (LEED) and 33±6 pm by medium-energy ion scattering (MEIS) [16] as well as 47 pm by the first-principles calculation [17]. This stress can be further relieved by alternately locating Sn along the [001] direction to stabilize the c(2×2) configuration.…”
Section: Resultsmentioning
confidence: 99%
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“…For the Sn/Ni(110) surface, the atomic radius of Sn is about 20% larger than that of Ni, leading to compressive stress both in the [001] and [110] directions. The surface stress can be partly relieved by the outward relaxation of Sn, and 40±3 pm protrusion was reported by low-energy electron diffraction (LEED) and 33±6 pm by medium-energy ion scattering (MEIS) [16] as well as 47 pm by the first-principles calculation [17]. This stress can be further relieved by alternately locating Sn along the [001] direction to stabilize the c(2×2) configuration.…”
Section: Resultsmentioning
confidence: 99%
“…For a half monolayer of Si, alternating Si and Ni in closepacked [110] rows have lower energy than the separated configuration. A few metal-embedded superstructures, such as Sn/Ni(110) [16,17], Mn/Ni(110) [18,19], were previously reported on the Ni(110) surface, and only the c(2×2) superstructure was stabilized for both surfaces. This shows a marked contrast to the present Si/Ni(110) where p(1×2) coexists with c(2×2).…”
Section: Resultsmentioning
confidence: 99%
“…However, if one were to compute E Sn ad with respect to the atomic state of Sn (note that the cohesive energy of bulk α-Sn is calculated to be −3.18 eV), the calculated values for E Sn ad now span over a range of −4.11 to −2.29 eV. These values will ease our discussion when comparing the adsorption energies reported for other bimetallic adsorbate-substrate systems: from −3.8 to −2.7 eV for Co=Cuð001Þ [53], −4.1 to −2.9 eV for Sb=Cuð001Þ [54], −4.7 to −3.7 eV for Sn=Nið001Þ [55], and −4.5 to −3.4 eV for Sn=Auð111Þ [56].…”
Section: Surface Alloysmentioning
confidence: 72%
“…Here, E vac f is the formation energy of a surface vacancy, E vac is the total energy per unit cell of the surface with a vacancy, and E Ni bulk is the total energy per atom of bulk fcc Ni. The surface vacancy formation energy of Ni(110) c(2×2) model was calculated to be 0.48 eV, smaller than that of the Ni(100) c(2×2) phase, [16] The calculated adsorption energies of all the structural models considered were given in Table 1. In the case of the AFM coupling for the substitutional adsorption, only the AFM coupling between the Mn adatoms for the c(2×2) phase was presented here since it is the most stable configuration under the condition of AFM coupling as suggested by the following research of magnetic properties.…”
Section: Structural Propertiesmentioning
confidence: 99%
“…It seems that the adsorption behaviour of Mn on Ni(110) c(2×2) surface is somewhat different from that on the Sn-Ni(110) c(2×2) surface alloy, which has a much smoother surface and shorter NN distance than the bulk Ni 3 Sn. [16,21] Obviously the magnetic moments of Mn atoms have a considerable influence on surface geometrical structure. The interlayer distances are also presented in Table 1.…”
Section: Structural Propertiesmentioning
confidence: 99%