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Magnetically Induced Rotating Rayleigh-Taylor Instability
Published on: March 3, 2017
Rayleigh-Taylor instability in two-layer granular flows.
Umberto D'Ortona1, Denis Martinand1, Nathalie Thomas2
1M2P2, Aix Marseille University, CNRS, Centrale Méditérannée, Marseille, France.
This study reveals how granular materials with different densities exhibit Rayleigh-Taylor-like instability, forming organized bands and rolls. Particle size segregation and sedimentation influence mixing dynamics at the interface.
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Area of Science:
- Physics
- Geophysics
- Materials Science
Background:
- Granular materials exhibit complex behaviors under gravitational forces.
- Rayleigh-Taylor instability (RTI) is a known phenomenon in fluid dynamics.
- Understanding granular RTI is crucial for geophysical flows and industrial processes.
Purpose of the Study:
- To investigate the Rayleigh-Taylor-like instability in two-layer granular systems.
- To compare numerical simulations with experimental results.
- To analyze the role of particle properties and flow dynamics in granular RTI.
Main Methods:
- Numerical simulations using the discrete element method (DEM) with tilted gravity.
- Experimental setup involving an inclined channel with a confinement gate.
- Analysis of particle movement, plume formation, and band organization.
Main Results:
- Rapid onset of granular RTI with plumes of light particles emerging at the surface.
- Organization of plumes into alternated bands of dense and light particles due to flow and shear.
- Dense particles segregate to the surface, sustaining longitudinal rolls.
- Granular RTI exhibits characteristics similar to fluid RTI, including wavelength and growth rate dependencies.
Conclusions:
- Granular RTI shares similarities with fluid RTI but is modified by sedimentation and size segregation.
- Sedimentation promotes diffusion, while size segregation acts as an anti-diffusion process.
- These competing processes control the mixing zone at the interface between granular layers.