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Self-similar Rayleigh–Taylor mixing with accelerations varying in time and space

As a ubiquitous paradigm of instabilities and mixing that occur in instances as diverse as supernovae, plasma fusion, oil recovery, and nanofabrication, the Rayleigh–Taylor (RT) problem is rightly regarded as important. The acceleration of the fluid medium in these instances often depends on time an...

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Autores principales: Abarzhi, Snezhana I., Sreenivasan, Katepalli R.
Formato: Online Artículo Texto
Lenguaje:English
Publicado: National Academy of Sciences 2022
Materias:
Acceso en línea:https://www.ncbi.nlm.nih.gov/pmc/articles/PMC9704740/
https://www.ncbi.nlm.nih.gov/pubmed/36375067
http://dx.doi.org/10.1073/pnas.2118589119
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author Abarzhi, Snezhana I.
Sreenivasan, Katepalli R.
author_facet Abarzhi, Snezhana I.
Sreenivasan, Katepalli R.
author_sort Abarzhi, Snezhana I.
collection PubMed
description As a ubiquitous paradigm of instabilities and mixing that occur in instances as diverse as supernovae, plasma fusion, oil recovery, and nanofabrication, the Rayleigh–Taylor (RT) problem is rightly regarded as important. The acceleration of the fluid medium in these instances often depends on time and space, whereas most past studies assume it to be constant or impulsive. Here, we analyze the symmetries of RT mixing for variable accelerations and obtain the scaling of correlations and spectra for classes of self-similar dynamics. RT mixing is shown to retain the memory of deterministic conditions for all accelerations, with the dynamics ranging from superballistic to subdiffusive. These results contribute to our understanding and control of the RT phenomena and reveal specific conditions under which Kolmogorov turbulence might be realized in RT mixing.
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spelling pubmed-97047402022-11-29 Self-similar Rayleigh–Taylor mixing with accelerations varying in time and space Abarzhi, Snezhana I. Sreenivasan, Katepalli R. Proc Natl Acad Sci U S A Physical Sciences As a ubiquitous paradigm of instabilities and mixing that occur in instances as diverse as supernovae, plasma fusion, oil recovery, and nanofabrication, the Rayleigh–Taylor (RT) problem is rightly regarded as important. The acceleration of the fluid medium in these instances often depends on time and space, whereas most past studies assume it to be constant or impulsive. Here, we analyze the symmetries of RT mixing for variable accelerations and obtain the scaling of correlations and spectra for classes of self-similar dynamics. RT mixing is shown to retain the memory of deterministic conditions for all accelerations, with the dynamics ranging from superballistic to subdiffusive. These results contribute to our understanding and control of the RT phenomena and reveal specific conditions under which Kolmogorov turbulence might be realized in RT mixing. National Academy of Sciences 2022-11-14 2022-11-22 /pmc/articles/PMC9704740/ /pubmed/36375067 http://dx.doi.org/10.1073/pnas.2118589119 Text en Copyright © 2022 the Author(s). Published by PNAS. https://creativecommons.org/licenses/by-nc-nd/4.0/This open access article is distributed under Creative Commons Attribution-NonCommercial-NoDerivatives License 4.0 (CC BY-NC-ND) (https://creativecommons.org/licenses/by-nc-nd/4.0/) .
spellingShingle Physical Sciences
Abarzhi, Snezhana I.
Sreenivasan, Katepalli R.
Self-similar Rayleigh–Taylor mixing with accelerations varying in time and space
title Self-similar Rayleigh–Taylor mixing with accelerations varying in time and space
title_full Self-similar Rayleigh–Taylor mixing with accelerations varying in time and space
title_fullStr Self-similar Rayleigh–Taylor mixing with accelerations varying in time and space
title_full_unstemmed Self-similar Rayleigh–Taylor mixing with accelerations varying in time and space
title_short Self-similar Rayleigh–Taylor mixing with accelerations varying in time and space
title_sort self-similar rayleigh–taylor mixing with accelerations varying in time and space
topic Physical Sciences
url https://www.ncbi.nlm.nih.gov/pmc/articles/PMC9704740/
https://www.ncbi.nlm.nih.gov/pubmed/36375067
http://dx.doi.org/10.1073/pnas.2118589119
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