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Magnetically Induced Rotating Rayleigh-Taylor Instability
Published on: March 3, 2017
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A New Approach to the Rayleigh-Taylor Instability
Björn Gebhard1, József J Kolumbán1, László Székelyhidi1
1Mathematisches Institut, Universität Leipzig, Augustusplatz 10, 04109 Leipzig, Germany.
Summary
This study introduces a criterion for turbulent fluid mixing, proving infinite weak solutions for the Euler equations. This is demonstrated in Rayleigh-Taylor instability scenarios with ultra-high Atwood numbers.
Area of Science:
- Fluid dynamics
- Partial differential equations
- Mathematical physics
Background:
- The inhomogeneous incompressible Euler equations model fluid interfaces under gravity.
- Rayleigh-Taylor instability occurs when a heavier fluid is above a lighter fluid, leading to turbulent mixing.
- Understanding weak solutions is crucial for modeling complex fluid behaviors.
Purpose of the Study:
- To formulate a general criterion for the existence of infinitely many weak solutions for the Euler equations.
- To analyze turbulent mixing in two-fluid systems with different densities.
- To investigate the impact of relaxing constitutive laws on fluid behavior.
Main Methods:
- Modeling the Euler equations as a differential inclusion.
- Considering the relaxation of constitutive laws.
- Developing a criterion for existence of weak solutions.
- Analyzing the Rayleigh-Taylor instability configuration.
Main Results:
- A general criterion for infinitely many weak solutions is established.
- The criterion is verified for the Rayleigh-Taylor instability with a heavier fluid initially above a lighter fluid.
- Specific examples show mixing zones growing quadratically in time for ultra-high Atwood numbers.
Conclusions:
- The study provides a theoretical framework for understanding turbulent mixing in stratified fluids.
- The findings are particularly relevant for scenarios exhibiting strong density differences (ultra-high Atwood numbers).
- The relaxation of constitutive laws offers a pathway to model complex, turbulent phenomena.
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