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Magnetically Induced Rotating Rayleigh-Taylor Instability
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Curvature-driven instabilities in thin active shells.

Andrea Giudici1, John S Biggins1

  • 1Department of Engineering, University of Cambridge, Trumpington Street, Cambridge CB21PZ, UK.

Royal Society Open Science
|October 17, 2022
PubMed
Summary
This summary is machine-generated.

Material shape changes trigger elastic instabilities in thin shells. These instabilities, driven by geometric incompatibility, lead to symmetry-breaking, inversion, and rotation phenomena with thickness-independent thresholds.

Keywords:
curvaturegeometryinstabilitymorphingshells

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Area of Science:

  • Physics
  • Materials Science
  • Mechanical Engineering

Background:

  • Spontaneous material shape changes (e.g., swelling, thermal expansion) can induce significant elastic instabilities in thin shells.
  • These instabilities arise from geometric incompatibility between a shell's preferred extrinsic and intrinsic curvatures.
  • Active deformations, through or in plane, can modify these curvatures.

Purpose of the Study:

  • To analyze the simplest model of elastic instabilities in shallow, thin shells.
  • To investigate instabilities under homogeneous preferred curvatures for zero, positive, and negative Gauss curvature cases.
  • To characterize symmetry-breaking, inversion, and rotation instabilities.

Main Methods:

  • Solving a simplified elastic instability model for shallow shells.
  • Analyzing shells that bend but do not stretch.
  • Considering shells with homogeneous preferred curvatures.

Main Results:

  • Identified two types of supercritical symmetry-breaking instabilities (discrete up/down and continuous planar isotropy).
  • Observed subcritical inversion instabilities and energy-free rotation instabilities.
  • Determined thickness-independent thresholds for preferred extrinsic curvature, proportional to the square root of Gauss curvature.

Conclusions:

  • The study provides a fundamental understanding of elastic instabilities in thin shells driven by material shape changes.
  • The identified instabilities and their thresholds offer insights into shell behavior under geometric constraints.
  • Results align with experimental data for deep spherical caps, validating the model.