2001
DOI: 10.1103/physrevlett.87.016104
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Dewetting: Film Rupture by Nucleation in the Spinodal Regime

Abstract: Unstable thin liquid films on solid substrates dewet by hole nucleation on defects or by a linear surface instability (spinodal dewetting). A system with destabilizing short-range and stabilizing long-range molecular interactions is investigated. We show that, for a subrange within the linearly unstable film thickness range, nucleation determines the final structure, whereas spinodal dewetting is of negligible influence. The results are also applicable to the spinodal decomposition of binary mixtures.

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Cited by 187 publications
(198 citation statements)
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References 23 publications
(26 reference statements)
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“…This was confirmed by direct integration of the time evolution Eq. (7) for case (I) in [43], for case (II) in [42] and for case (III) in Section 5. Despite the restriction to a two-dimensional geometry we think that the difference of subranges (A) and (B) can also be seen in the more realistic three-dimensional geometry.…”
Section: Discussionmentioning
confidence: 99%
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“…This was confirmed by direct integration of the time evolution Eq. (7) for case (I) in [43], for case (II) in [42] and for case (III) in Section 5. Despite the restriction to a two-dimensional geometry we think that the difference of subranges (A) and (B) can also be seen in the more realistic three-dimensional geometry.…”
Section: Discussionmentioning
confidence: 99%
“…To clarify this issue, we discuss first in detail the linear stability of the periodic nucleation solutions in range (ii), and second the results of a direct integration in time performed in [42]. For a given h( we calculate the linear growth rates of disturbances to the solutions of the branch of nucleation solutions in the mixed range, (ii).…”
Section: (Ii))mentioning
confidence: 99%
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“…Several instability mechanisms exist that by means of different driving forces may destabilize an initially flat film. They are described, analysed and modelled in a large number of experimental 4,5,10,11,12,13,14 and theoretical 7,15,16,17,18,19,20,21,22,23,24,25,26,27,28,29,30,31 works. For film thicknesses d less than about 100 nm, effective molecular interactions between the film surface and the substrate dominate all the other forces, like thermo-and soluto-capillarity or gravity, and thus determine the film stability.…”
Section: Introductionmentioning
confidence: 99%