Microbial Range Expansions on Liquid Substrates

Despite the importance of fluid flow for transporting and organizing populations, few laboratory systems exist to systematically investigate the impact of advection on their spatial evolutionary dynamics. To address this problem, we study the morphology and genetic spatial structure of microbial col...

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Autores principales: Severine Atis, Bryan T. Weinstein, Andrew W. Murray, David R. Nelson
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Publicado: American Physical Society 2019
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spelling oai:doaj.org-article:980ce8b2de81442788746fc2be98fc302021-12-02T11:08:30ZMicrobial Range Expansions on Liquid Substrates10.1103/PhysRevX.9.0210582160-3308https://doaj.org/article/980ce8b2de81442788746fc2be98fc302019-06-01T00:00:00Zhttp://doi.org/10.1103/PhysRevX.9.021058http://doi.org/10.1103/PhysRevX.9.021058https://doaj.org/toc/2160-3308Despite the importance of fluid flow for transporting and organizing populations, few laboratory systems exist to systematically investigate the impact of advection on their spatial evolutionary dynamics. To address this problem, we study the morphology and genetic spatial structure of microbial colonies growing on the surface of a nutrient-laden fluid 10^{4} to 10^{5} times more viscous than water in Petri dishes; the extreme but finite viscosity inhibits undesired thermal convection and allows populations to effectively live at the air-liquid interface due to capillary forces. We discover that S. cerevisiae (baker’s yeast) growing on a viscous liquid behave like “active matter”: They metabolically generate fluid flows many times larger than their unperturbed colony expansion speed, and that flow, in turn, can dramatically impact their colony morphology and spatial population genetics. We show that yeast cells generate fluid flows by consuming surrounding nutrients and decreasing the local substrate density, leading to misaligned fluid pressure and density contours, which ultimately generates vorticity via a thresholdless baroclinic instability. Numerical simulations with experimentally measured parameters demonstrate that an intense vortex ring is produced below the colony’s edge. As the viscosity of the substrate is lowered and the self-induced flow intensifies, we observe three distinct morphologies: At the highest viscosity, cell proliferation and movement produces compact circular colonies with, however, a stretched regime of exponential expansion; intermediate viscosities give rise to compact colonies with “fingers” that are usually monoclonal and then break into smaller cell clusters; at the lowest viscosity, the expanding colony fractures into many genetically diverse, mutually repelling, islandlike fragments that can colonize an entire 94-mm-diameter Petri dish within 36 hours. We propose a simple phenomenological model that predicts the early colony dynamics. Our results provide rich opportunities to study the interplay between fluid flow and spatial population genetics for future investigations.Severine AtisBryan T. WeinsteinAndrew W. MurrayDavid R. NelsonAmerican Physical SocietyarticlePhysicsQC1-999ENPhysical Review X, Vol 9, Iss 2, p 021058 (2019)
institution DOAJ
collection DOAJ
language EN
topic Physics
QC1-999
spellingShingle Physics
QC1-999
Severine Atis
Bryan T. Weinstein
Andrew W. Murray
David R. Nelson
Microbial Range Expansions on Liquid Substrates
description Despite the importance of fluid flow for transporting and organizing populations, few laboratory systems exist to systematically investigate the impact of advection on their spatial evolutionary dynamics. To address this problem, we study the morphology and genetic spatial structure of microbial colonies growing on the surface of a nutrient-laden fluid 10^{4} to 10^{5} times more viscous than water in Petri dishes; the extreme but finite viscosity inhibits undesired thermal convection and allows populations to effectively live at the air-liquid interface due to capillary forces. We discover that S. cerevisiae (baker’s yeast) growing on a viscous liquid behave like “active matter”: They metabolically generate fluid flows many times larger than their unperturbed colony expansion speed, and that flow, in turn, can dramatically impact their colony morphology and spatial population genetics. We show that yeast cells generate fluid flows by consuming surrounding nutrients and decreasing the local substrate density, leading to misaligned fluid pressure and density contours, which ultimately generates vorticity via a thresholdless baroclinic instability. Numerical simulations with experimentally measured parameters demonstrate that an intense vortex ring is produced below the colony’s edge. As the viscosity of the substrate is lowered and the self-induced flow intensifies, we observe three distinct morphologies: At the highest viscosity, cell proliferation and movement produces compact circular colonies with, however, a stretched regime of exponential expansion; intermediate viscosities give rise to compact colonies with “fingers” that are usually monoclonal and then break into smaller cell clusters; at the lowest viscosity, the expanding colony fractures into many genetically diverse, mutually repelling, islandlike fragments that can colonize an entire 94-mm-diameter Petri dish within 36 hours. We propose a simple phenomenological model that predicts the early colony dynamics. Our results provide rich opportunities to study the interplay between fluid flow and spatial population genetics for future investigations.
format article
author Severine Atis
Bryan T. Weinstein
Andrew W. Murray
David R. Nelson
author_facet Severine Atis
Bryan T. Weinstein
Andrew W. Murray
David R. Nelson
author_sort Severine Atis
title Microbial Range Expansions on Liquid Substrates
title_short Microbial Range Expansions on Liquid Substrates
title_full Microbial Range Expansions on Liquid Substrates
title_fullStr Microbial Range Expansions on Liquid Substrates
title_full_unstemmed Microbial Range Expansions on Liquid Substrates
title_sort microbial range expansions on liquid substrates
publisher American Physical Society
publishDate 2019
url https://doaj.org/article/980ce8b2de81442788746fc2be98fc30
work_keys_str_mv AT severineatis microbialrangeexpansionsonliquidsubstrates
AT bryantweinstein microbialrangeexpansionsonliquidsubstrates
AT andrewwmurray microbialrangeexpansionsonliquidsubstrates
AT davidrnelson microbialrangeexpansionsonliquidsubstrates
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