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Stokesian dynamics simulations of a magnetotactic bacterium
ABSTRACT: The swimming of bacteria provides insight into propulsion and steering under the conditions of low-Reynolds number hydrodynamics. Here we address the magnetically steered swimming of magnetotactic bacteria. We use Stokesian dynamics simulations to study the swimming of single-flagellated m...
Autores principales: | , , |
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Formato: | Online Artículo Texto |
Lenguaje: | English |
Publicado: |
Springer Berlin Heidelberg
2021
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Materias: | |
Acceso en línea: | https://www.ncbi.nlm.nih.gov/pmc/articles/PMC7987682/ https://www.ncbi.nlm.nih.gov/pubmed/33759003 http://dx.doi.org/10.1140/epje/s10189-021-00038-5 |
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author | Mohammadinejad, Sarah Faivre, Damien Klumpp, Stefan |
author_facet | Mohammadinejad, Sarah Faivre, Damien Klumpp, Stefan |
author_sort | Mohammadinejad, Sarah |
collection | PubMed |
description | ABSTRACT: The swimming of bacteria provides insight into propulsion and steering under the conditions of low-Reynolds number hydrodynamics. Here we address the magnetically steered swimming of magnetotactic bacteria. We use Stokesian dynamics simulations to study the swimming of single-flagellated magnetotactic bacteria (MTB) in an external magnetic field. Our model MTB consists of a spherical cell body equipped with a magnetic dipole moment and a helical flagellum rotated by a rotary motor. The elasticity of the flagellum as well as magnetic and hydrodynamic interactions is taken into account in this model. We characterized how the swimming velocity is dependent on parameters of the model. We then studied the U-turn motion after a field reversal and found two regimes for weak and strong fields and, correspondingly, two characteristic time scales. In the two regimes, the U-turn time is dominated by the turning of the cell body and its magnetic moment or the turning of the flagellum, respectively. In the regime for weak fields, where turning is dominated by the magnetic relaxation, the U-turn time is approximately in agreement with a theoretical model based on torque balance. In the strong-field regime, strong deformations of the flagellum are observed. We further simulated the swimming of a bacterium with a magnetic moment that is inclined relative to the flagellar axis. This scenario leads to intriguing double helical trajectories that we characterize as functions of the magnetic moment inclination and the magnetic field. For small inclination angles ([Formula: see text] ) and typical field strengths, the inclination of the magnetic moment has only a minor effect on the swimming of MTB in an external magnetic field. Large inclination angles result in a strong reduction in the velocity in direction of the magnetic field, consistent with recent observations that bacteria with large inclination angles use a different propulsion mechanism. GRAPHIC ABSTRACT: [Image: see text] SUPPLEMENTARY INFORMATION: The online version supplementary material available at 10.1140/epje/s10189-021-00038-5. |
format | Online Article Text |
id | pubmed-7987682 |
institution | National Center for Biotechnology Information |
language | English |
publishDate | 2021 |
publisher | Springer Berlin Heidelberg |
record_format | MEDLINE/PubMed |
spelling | pubmed-79876822021-04-27 Stokesian dynamics simulations of a magnetotactic bacterium Mohammadinejad, Sarah Faivre, Damien Klumpp, Stefan Eur Phys J E Soft Matter Regular Article - Living Systems ABSTRACT: The swimming of bacteria provides insight into propulsion and steering under the conditions of low-Reynolds number hydrodynamics. Here we address the magnetically steered swimming of magnetotactic bacteria. We use Stokesian dynamics simulations to study the swimming of single-flagellated magnetotactic bacteria (MTB) in an external magnetic field. Our model MTB consists of a spherical cell body equipped with a magnetic dipole moment and a helical flagellum rotated by a rotary motor. The elasticity of the flagellum as well as magnetic and hydrodynamic interactions is taken into account in this model. We characterized how the swimming velocity is dependent on parameters of the model. We then studied the U-turn motion after a field reversal and found two regimes for weak and strong fields and, correspondingly, two characteristic time scales. In the two regimes, the U-turn time is dominated by the turning of the cell body and its magnetic moment or the turning of the flagellum, respectively. In the regime for weak fields, where turning is dominated by the magnetic relaxation, the U-turn time is approximately in agreement with a theoretical model based on torque balance. In the strong-field regime, strong deformations of the flagellum are observed. We further simulated the swimming of a bacterium with a magnetic moment that is inclined relative to the flagellar axis. This scenario leads to intriguing double helical trajectories that we characterize as functions of the magnetic moment inclination and the magnetic field. For small inclination angles ([Formula: see text] ) and typical field strengths, the inclination of the magnetic moment has only a minor effect on the swimming of MTB in an external magnetic field. Large inclination angles result in a strong reduction in the velocity in direction of the magnetic field, consistent with recent observations that bacteria with large inclination angles use a different propulsion mechanism. GRAPHIC ABSTRACT: [Image: see text] SUPPLEMENTARY INFORMATION: The online version supplementary material available at 10.1140/epje/s10189-021-00038-5. Springer Berlin Heidelberg 2021-03-23 2021 /pmc/articles/PMC7987682/ /pubmed/33759003 http://dx.doi.org/10.1140/epje/s10189-021-00038-5 Text en © The Author(s) 2021 https://creativecommons.org/licenses/by/4.0/Open AccessThis article is licensed under a Creative Commons Attribution 4.0 International License, which permits use, sharing, adaptation, distribution and reproduction in any medium or format, as long as you give appropriate credit to the original author(s) and the source, provide a link to the Creative Commons licence, and indicate if changes were made. The images or other third party material in this article are included in the article’s Creative Commons licence, unless indicated otherwise in a credit line to the material. If material is not included in the article’s Creative Commons licence and your intended use is not permitted by statutory regulation or exceeds the permitted use, you will need to obtain permission directly from the copyright holder. To view a copy of this licence, visit http://creativecommons.org/licenses/by/4.0/ (https://creativecommons.org/licenses/by/4.0/) . |
spellingShingle | Regular Article - Living Systems Mohammadinejad, Sarah Faivre, Damien Klumpp, Stefan Stokesian dynamics simulations of a magnetotactic bacterium |
title | Stokesian dynamics simulations of a magnetotactic bacterium |
title_full | Stokesian dynamics simulations of a magnetotactic bacterium |
title_fullStr | Stokesian dynamics simulations of a magnetotactic bacterium |
title_full_unstemmed | Stokesian dynamics simulations of a magnetotactic bacterium |
title_short | Stokesian dynamics simulations of a magnetotactic bacterium |
title_sort | stokesian dynamics simulations of a magnetotactic bacterium |
topic | Regular Article - Living Systems |
url | https://www.ncbi.nlm.nih.gov/pmc/articles/PMC7987682/ https://www.ncbi.nlm.nih.gov/pubmed/33759003 http://dx.doi.org/10.1140/epje/s10189-021-00038-5 |
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