1996
DOI: 10.1007/978-3-642-61400-2
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Concepts in Surface Physics

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Cited by 262 publications
(179 citation statements)
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“…6). The resulting cohesive energy is found to be ß0.34 eV per interface atom which is higher than what is typically expected for weak physisorption interactions (Desjonquères & Spanjaard, 1996). This value is however consistent with other modelling works on 2D heterostacks (Zhong et al, 2016) and points towards the presence of a strong interaction at the interface between the two phases (Lefebvre et al, 1998), which leads to a distortion in the atomic structure of the β-SnS layer, leading to the formation of the new β' phase.…”
Section: Fig 6 Evolution Of the Interaction Energy Per Surface Atomsupporting
confidence: 82%
“…6). The resulting cohesive energy is found to be ß0.34 eV per interface atom which is higher than what is typically expected for weak physisorption interactions (Desjonquères & Spanjaard, 1996). This value is however consistent with other modelling works on 2D heterostacks (Zhong et al, 2016) and points towards the presence of a strong interaction at the interface between the two phases (Lefebvre et al, 1998), which leads to a distortion in the atomic structure of the β-SnS layer, leading to the formation of the new β' phase.…”
Section: Fig 6 Evolution Of the Interaction Energy Per Surface Atomsupporting
confidence: 82%
“…In thermodynamic equilibrium, the ratio between facet radius r and the distance h of the facet from the center of the crystal is equal to the ratio of step free energy b to surface free energy g of the facet [3,14]. With increasing temperature, steps lower their free energy by gaining configurational entropy due to kink formation [15] and by an excess vibrational free energy [5,16]. Since free energies for singular surfaces change much more slowly with temperature than step free energies [17], a temperature increase corresponds to shrinking (and decrease to expansion) of the equilibrium facet diameter.…”
mentioning
confidence: 99%
“…This common property of this class of potentials has a clear physical origin: the energy E i of an atom i should decrease more and more slowly when its coordination increases towards the bulk coordination [59,65]. This clearly implies that F ′′ (ρ) must be positive.…”
Section: N-body Semi-empirical Potentialsmentioning
confidence: 90%
“…The step vibrational free energy of a given vicinal surface is of the order of a few meV and decreases with temperature, reaching a linear regime for T larger than 100K when the entropy contribution becomes the leading term (see ref. [59]). More interestingly F vib step (T ) can be plotted for a given temperature, as a function of the terrace width as shown in Fig.…”
Section: Vibrational Free Energy Of Stepsmentioning
confidence: 99%