book of abstracts - IM2NP
book of abstracts - IM2NP
book of abstracts - IM2NP
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A B S T R A C T S THURSDAY, JULY 1 N A N O S E A 2 0 1 0<br />
deposition noise dominates deposition noise has been observed in computer simulations, but does not appear<br />
to have any experimental relevance.<br />
For an initially flat surface, the Villain-Lai-Das Sarma (VLDS) equation with nonconserved noise is obtained<br />
for all models with random deposition and nearest-neighbor hopping. This equation is not observed in any<br />
transient regime for typical MBE conditions. If, however, the initial surface is corrugated, the relative<br />
magnitudes <strong>of</strong> terms in the equation <strong>of</strong> motion can be altered to the point where the VLDS equation does<br />
indeed describe transient growth, albeit with conserved noise. This is consistent with the analysis <strong>of</strong> growth<br />
on patterned surfaces reported by the Maryland group. We will discuss the effect <strong>of</strong> various types <strong>of</strong> patterns<br />
on the governing growth equations and their experimental consequences.<br />
3 – Conclusion<br />
We have shown how our previously developed methodology for deriving regularized stochastic continuum<br />
equations can account for much <strong>of</strong> the transient behavior seen in deposition/diffusion systems. On such<br />
surfaces, under typical conditions, the governing equations are found to be linear. The extent to which this<br />
can be extended to the submonolayer regime is currently being investigated. We have seen that the<br />
patterning <strong>of</strong> a substrate can pre-empt the behavior seen on initially flat substrates. The application <strong>of</strong> RG<br />
methods to see the complete evolution <strong>of</strong> such systems remains to be carried out. But already the systematic<br />
derivation <strong>of</strong> growth equations for patterned substrates represents a substantial advance for these important<br />
systems.<br />
17H00-17H30<br />
Modeling Facet Nucleation and Growth <strong>of</strong> Hut Clusters on Ge/Si(001).<br />
J. A. Venables1,3, D.R. Bowler3, M.R. McKay2,4 and J. Drucker1,2 (1) Physics, 2)<br />
Materials, Arizona State University, Tempe, Arizona, USA, 3) LCN-UCL, London, UK; 4) Lawrence<br />
Semiconductor, Tempe, Arizona, USA).<br />
Recent STM observations <strong>of</strong> homogenous distributions <strong>of</strong> pyramid and hut clusters on Ge/Si(001) have<br />
shown that these clusters grow extremely slowly during annealing at intermediate temperatures, T ~ 450 oC,<br />
when there is a super-saturation <strong>of</strong> mobile ad-particles above and within the wetting layer. Data has been<br />
obtained on the absolute length <strong>of</strong> the clusters as a function <strong>of</strong> time L(t), and thereby the evolution <strong>of</strong> the<br />
growth rate, over periods <strong>of</strong> order 100 hours [1]. We model this slow growth as a layer by layer (2D) facet<br />
nucleation and growth problem, in the presence <strong>of</strong> strain-induced energies both on and around the facets.<br />
All <strong>of</strong> these energies can markedly influence the nucleation rate <strong>of</strong> new facets. First, they justify the<br />
observation that facet nucleation occurs from the apex <strong>of</strong> the hut, as has been observed in several other<br />
studies [2, 3]. Second, they indicate a substantial slowing down <strong>of</strong> the nucleation rate, by many orders <strong>of</strong><br />
magnitude, relative to the case when such energies are not present. Finally the need to undo the stable<br />
reconstruction on the {105} facets as each new layer is formed contributes an extra energy <strong>of</strong> order 0.5 eV<br />
[4] to the energy <strong>of</strong> the critical nucleus.<br />
Inclusion <strong>of</strong> these effects, with experimental values <strong>of</strong> the Ge diffusion coefficient, provides a quantitative fit<br />
to the L(t) data, and sets bounds on step and facet energies appropriate to hut clusters. Such energies are<br />
increasingly amenable to ab-initio calculation on reconstructed hut clusters to compare with experiment [5].<br />
1. M.R. McKay, J.A. Venables and J. Drucker, Phys. Rev. Lett. 101, 216104 (2008); Solid State Comm. 149, 1403-1409 (2009)<br />
2. F. Montalenti et al., Phys. Rev. Lett., 93, 216102 (2004)<br />
100