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Updated: Oct 21, 2025

Magnetically Induced Rotating Rayleigh-Taylor Instability
Published on: March 3, 2017
Origin of the Sharkskin Instability: Nonlinear Dynamics
Stylianos Varchanis1,2, Dionisis Pettas1, Yannis Dimakopoulos1
1Laboratory of Fluid Mechanics & Rheology, Department of Chemical Engineering, University of Patras, Patras 26500, Greece.
Abstract:
The appearance of surface distortions on polymer melt extrudates, often referred to as sharkskin instability, is a long-standing problem. We report results of a simple physical model, which link the inception of surface defects with intense stretch of polymer chains and subsequent recoil at the region where the melt detaches from the solid wall of the die. The transition from smooth to wavy extrudate is attributed to a Hopf bifurcation, followed by a sequence of period doubling bifurcations, which eventually lead to elastic turbulence under creeping flow. The predicted flow profiles exhibit all the characteristics of the experimentally observed surface defects during polymer melt extrusion.
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