4.4 Article

Rayleigh-Taylor instability of viscous liquid films under a temperature-controlled inclined substrate

Journal

PHYSICAL REVIEW FLUIDS
Volume 6, Issue 6, Pages -

Publisher

AMER PHYSICAL SOC
DOI: 10.1103/PhysRevFluids.6.064001

Keywords

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Funding

  1. National University of Singapore [R-265-000-696-133]

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The study investigates the Rayleigh-Taylor instability of gravity-driven viscous liquid films flowing under a uniformly heated or cooled inclined substrate. It finds that the thermocapillary stress can significantly affect the stability of the liquid film, enhancing or suppressing instability. Specific critical values can completely inhibit instability or trigger absolute instability.
We study the Rayleigh-Taylor instability of gravity-driven viscous liquid films flowing under a uniformly heated or cooled inclined substrate. The long-wave assumption is adopted to derive the evolution equation of the film, which is characterized by five dimensionless parameters including Marangoni number Ma, Biot number Bi, Reynolds number Re, Weber number We, and the inclination angle alpha of the substrate. Based on the long-wave equation, we systematically examine the temporal and spatiotemporal stability of the system. Temporal stability analysis shows that the thermocapillary stress reinforces the Rayleigh-Taylor instability of a heated film but counteracts the instability of a cooled film, as verified by the numerical solutions of linearized Navier-Stokes equation. In particular, this instability can be completely inhibited if a composite Marangoni number Ma* is below a critical value Ma(1)*. We further perform a spatiotemporal stability analysis to delineate the absolute and convective nature of the temporally unstable system. We find that the thermocapillary stress in the heated film enhances the absolute instability and suppresses the convective instability. The trend reverses for a cooled film that is featured by suppressed absolute instability and enhanced convective instability. More importantly, the transition between the absolute and convective instability can be characterized by another critical value, Ma(2*), beyond which the flow stability will be triggered from the convectively into the absolutely unstable. The predictions from linear stability analysis are confirmed by numerical solutions of the full long-wave evolution equation.

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