2021•SIAM Journal on Applied MathematicsRequires access

Scale-Dependent and Self-Similar Rayleigh--Taylor and Richtmyer--Meshkov Dynamics Induced by Acceleration Varying with Length Scale

Arun Pandian, Jiahe Tony Li, Snezhana I. Abarzhi

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Abstract

Rayleigh--Taylor (RT) and Richtmyer--Meshkov (RM) instabilities and RT/RM interfacial mixing are omnipresent in nature and technology and are often driven by variable acceleration. This work presents the detailed study of RT/RM dynamics induced by the acceleration varying as power-law with the length scale. We consider RT/RM dynamics within the framework of group theory and momentum model and find solutions for the scale-dependent dynamics and for the self-similar mixing. The effect of fluctuations on the self-similar mixing is also investigated by augmenting the momentum model with stochastic process. We find that the scale-dependent dynamics and the self-similar mixing can be RT type and RM type depending on the exponent of the acceleration power-law. For the scale-dependent dynamics the exponent value separating RT and RM subregimes approaches negative infinity, whereas for the self-similar mixing it is a finite negative value depending on the drag. Based on these results, we elaborate new theory benchmarks for future research.

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What this paper is about

Rayleigh--Taylor (RT) and Richtmyer--Meshkov (RM) instabilities and RT/RM interfacial mixing are omnipresent in nature and technology and are often driven by variable acceleration. This work presents the detailed study of RT/RM dynamics induced by the acceleration varying as power-law with the length scale. We consider RT/RM dynamics within the framework of group theory and momentum model and find solutions for the scale-dependent dynamics and for the self-similar mixing. The effect of fluctuations on the self-similar mixing is also investigated by augmenting the momentum model with stochastic process. We find that the scale-dependent dynamics and the self-similar mixing can be RT type and RM type depending on the exponent of the acceleration power-law. For the scale-dependent dynamics the exponent value separating RT and RM subregimes approaches negative infinity, whereas for the self-similar mixing it is a finite negative value depending on the drag. Based on these results, we elaborate new theory benchmarks for future research.

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Available abstract

Rayleigh--Taylor (RT) and Richtmyer--Meshkov (RM) instabilities and RT/RM interfacial mixing are omnipresent in nature and technology and are often driven by variable acceleration. This work presents the detailed study of RT/RM dynamics induced by the acceleration varying as power-law with the length scale. We consider RT/RM dynamics within the framework of group theory and momentum model and find solutions for the scale-dependent dynamics and for the self-similar mixing. The effect of fluctuations on the self-similar mixing is also investigated by augmenting the momentum model with stochastic process. We find that the scale-dependent dynamics and the self-similar mixing can be RT type and RM type depending on the exponent of the acceleration power-law. For the scale-dependent dynamics the exponent value separating RT and RM subregimes approaches negative infinity, whereas for the self-similar mixing it is a finite negative value depending on the drag. Based on these results, we elaborate new theory benchmarks for future research.

Key concepts: Acceleration, Scale (ratio), Rayleigh–Taylor instability, Dynamics (music), Physics, Richtmyer–Meshkov instability, Rayleigh scattering, Length scale

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