Experimental determination of the propulsion matrix of the body of helical Magnetospirillum magneticum cells.


Journal

Physical review. E
ISSN: 2470-0053
Titre abrégé: Phys Rev E
Pays: United States
ID NLM: 101676019

Informations de publication

Date de publication:
Sep 2022
Historique:
received: 04 05 2021
accepted: 07 06 2022
entrez: 21 10 2022
pubmed: 22 10 2022
medline: 22 10 2022
Statut: ppublish

Résumé

Helical-shaped magnetotactic bacteria provide a rare opportunity to precisely measure both the translational and rotational friction coefficients of micron-sized chiral particles. The possibility to align these cells with a uniform magnetic field allows clearly separating diffusion along and perpendicular to their longitudinal axis. Meanwhile, their corkscrew shape allows detecting rotations around their longitudinal axis, after which orientation correlation analysis can be used to retrieve rotational diffusion coefficients in the two principal directions. Using light microscopy, we measured the four principal friction coefficients of deflagellated Magnetospirillum magneticum cells, and compared our results to that expected for cylinders of comparable size. We show that for rotational motions, the overall dimensions of the cell body are what matters most, while the exact body shape has a larger influence on translational motions. To obtain a full characterization of the friction matrix of these elongated chiral particles, we also quantified the coupling between the rotation around and translation along the longitudinal axis of the cell. Our results suggest that for this bacterial species cell body rotation could significantly contribute to cellular propulsion.

Identifiants

pubmed: 36266829
doi: 10.1103/PhysRevE.106.034407
doi:

Types de publication

Journal Article

Langues

eng

Sous-ensembles de citation

IM

Pagination

034407

Auteurs

Liu Yu (L)

Department of Physics and Astronomy, McMaster University, 1280 Main Street W, Hamilton, Ontario L8S4M1, Canada.

Lucas Le Nagard (L)

Department of Physics and Astronomy, McMaster University, 1280 Main Street W, Hamilton, Ontario L8S4M1, Canada.

Solomon Barkley (S)

Department of Physics and Astronomy, McMaster University, 1280 Main Street W, Hamilton, Ontario L8S4M1, Canada.

Lauren Smith (L)

Department of Physics and Astronomy, McMaster University, 1280 Main Street W, Hamilton, Ontario L8S4M1, Canada.

Cécile Fradin (C)

Department of Physics and Astronomy, McMaster University, 1280 Main Street W, Hamilton, Ontario L8S4M1, Canada.

Classifications MeSH