# Nucleated dewetting in supported ultra-thin liquid films with   hydrodynamic slip

**Authors:** Matthias Lessel, Joshua D. McGraw, Oliver B\"aumchen, Karin Jacobs

arXiv: 1705.00917 · 2017-05-03

## TL;DR

This paper investigates how surface energy and slip conditions affect the dewetting mechanisms of ultra-thin polymer films, showing a transition from spinodal to nucleation-driven breakup due to hydrophobic surfaces and slip.

## Contribution

It demonstrates the impact of hydrophobic surface treatments and slip conditions on dewetting morphology and introduces a free energy model for critical nucleus size in supported films.

## Key findings

- Transition from spinodal to nucleation-driven dewetting
- Dependence of hole density on film thickness and temperature
- Support for the free energy model with in situ AFM observations

## Abstract

This study reveals the influence of the surface energy and solid/liquid boundary condition on the breakup mechanism of dewetting ultra-thin polymer films. Using silane self-assembled monolayers, SiO$_2$ substrates are rendered hydrophobic and provide a strong slip rather than a no-slip solid/liquid boundary condition. On undergoing these changes, the thin-film breakup morphology changes dramatically -- from a spinodal mechanism to a breakup which is governed by nucleation and growth. The experiments reveal a dependence of the hole density on film thickness and temperature. The combination of lowered surface energy and hydrodynamic slip brings the studied system closer to the conditions encountered in bursting unsupported films. As for unsupported polymer films, a critical nucleus size is inferred from a free energy model. This critical nucleus size is supported by the film breakup observed in the experiments using high speed \emph{in situ} atomic force microscopy.

## Full text

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## Figures

14 figures with captions in the complete paper: https://tomesphere.com/paper/1705.00917/full.md

## References

52 references — full list in the complete paper: https://tomesphere.com/paper/1705.00917/full.md

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Source: https://tomesphere.com/paper/1705.00917