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Kinematic Properties of a Twisted Double Planetary Chaotic Mixer: A Three-Dimensional Numerical Investigation

In this study, a numerical investigation based on the CFD method is carried out to study the unsteady laminar flow of Newtonian fluid with a high viscosity in a three-dimensional simulation of a twisted double planetary mixer, which is composed of two agitating rods inside a moving tank. The conside...

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Autores principales: Mostefa, Telha, Eddine, Aissaoui Djamel, Tayeb, Naas Toufik, Hossain, Shakhawat, Rahman, Arifur, Mohamed, Bachiri, Kim, Kwang-Yong
Formato: Online Artículo Texto
Lenguaje:English
Publicado: MDPI 2022
Materias:
Acceso en línea:https://www.ncbi.nlm.nih.gov/pmc/articles/PMC9502745/
https://www.ncbi.nlm.nih.gov/pubmed/36144168
http://dx.doi.org/10.3390/mi13091545
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author Mostefa, Telha
Eddine, Aissaoui Djamel
Tayeb, Naas Toufik
Hossain, Shakhawat
Rahman, Arifur
Mohamed, Bachiri
Kim, Kwang-Yong
author_facet Mostefa, Telha
Eddine, Aissaoui Djamel
Tayeb, Naas Toufik
Hossain, Shakhawat
Rahman, Arifur
Mohamed, Bachiri
Kim, Kwang-Yong
author_sort Mostefa, Telha
collection PubMed
description In this study, a numerical investigation based on the CFD method is carried out to study the unsteady laminar flow of Newtonian fluid with a high viscosity in a three-dimensional simulation of a twisted double planetary mixer, which is composed of two agitating rods inside a moving tank. The considered stirring protocol is a “Continuous sine squared motion” by using the dynamic mesh model and user-defined functions (UDFs)to define the velocity profiles. The chaotic advection is obtained in our active mixers by the temporal modulation of rotational velocities of the moving walls in order to enhance the mixing of the fluid for a low Reynolds number and a high Peclet number. For this goal, we applied the Poincaré section and Lyapunov exponent as reliable mathematic tools for checking mixing quality by tracking a number of massless particles inside the fluid domain. Additionally, we investigated the development of fluid kinematics proprieties, such as vorticity, helicity, strain rate and elongation rate, at various time periods in order to view the impact of temporal modulation on the flow properties. The results of the mentioned simulation showed that it is possible to obtain a chaotic advection after a relatively short time, which can deeply enhance mixing fluid efficiency.
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spelling pubmed-95027452022-09-24 Kinematic Properties of a Twisted Double Planetary Chaotic Mixer: A Three-Dimensional Numerical Investigation Mostefa, Telha Eddine, Aissaoui Djamel Tayeb, Naas Toufik Hossain, Shakhawat Rahman, Arifur Mohamed, Bachiri Kim, Kwang-Yong Micromachines (Basel) Article In this study, a numerical investigation based on the CFD method is carried out to study the unsteady laminar flow of Newtonian fluid with a high viscosity in a three-dimensional simulation of a twisted double planetary mixer, which is composed of two agitating rods inside a moving tank. The considered stirring protocol is a “Continuous sine squared motion” by using the dynamic mesh model and user-defined functions (UDFs)to define the velocity profiles. The chaotic advection is obtained in our active mixers by the temporal modulation of rotational velocities of the moving walls in order to enhance the mixing of the fluid for a low Reynolds number and a high Peclet number. For this goal, we applied the Poincaré section and Lyapunov exponent as reliable mathematic tools for checking mixing quality by tracking a number of massless particles inside the fluid domain. Additionally, we investigated the development of fluid kinematics proprieties, such as vorticity, helicity, strain rate and elongation rate, at various time periods in order to view the impact of temporal modulation on the flow properties. The results of the mentioned simulation showed that it is possible to obtain a chaotic advection after a relatively short time, which can deeply enhance mixing fluid efficiency. MDPI 2022-09-17 /pmc/articles/PMC9502745/ /pubmed/36144168 http://dx.doi.org/10.3390/mi13091545 Text en © 2022 by the authors. https://creativecommons.org/licenses/by/4.0/Licensee MDPI, Basel, Switzerland. This article is an open access article distributed under the terms and conditions of the Creative Commons Attribution (CC BY) license (https://creativecommons.org/licenses/by/4.0/).
spellingShingle Article
Mostefa, Telha
Eddine, Aissaoui Djamel
Tayeb, Naas Toufik
Hossain, Shakhawat
Rahman, Arifur
Mohamed, Bachiri
Kim, Kwang-Yong
Kinematic Properties of a Twisted Double Planetary Chaotic Mixer: A Three-Dimensional Numerical Investigation
title Kinematic Properties of a Twisted Double Planetary Chaotic Mixer: A Three-Dimensional Numerical Investigation
title_full Kinematic Properties of a Twisted Double Planetary Chaotic Mixer: A Three-Dimensional Numerical Investigation
title_fullStr Kinematic Properties of a Twisted Double Planetary Chaotic Mixer: A Three-Dimensional Numerical Investigation
title_full_unstemmed Kinematic Properties of a Twisted Double Planetary Chaotic Mixer: A Three-Dimensional Numerical Investigation
title_short Kinematic Properties of a Twisted Double Planetary Chaotic Mixer: A Three-Dimensional Numerical Investigation
title_sort kinematic properties of a twisted double planetary chaotic mixer: a three-dimensional numerical investigation
topic Article
url https://www.ncbi.nlm.nih.gov/pmc/articles/PMC9502745/
https://www.ncbi.nlm.nih.gov/pubmed/36144168
http://dx.doi.org/10.3390/mi13091545
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