# Localization and dynamics of sulfur-oxidizing microbes in natural   sediment

**Authors:** Alexander Petroff, Frank Tejera, Albert Libchaber

arXiv: 1704.08212 · 2017-04-27

## TL;DR

This study investigates the behavior and organization of sulfur-oxidizing microbes in sediment, revealing stable microbial fronts and their dynamics influenced by metabolism, aerotaxis, and diffusion, with implications for understanding sedimentary carbon cycling.

## Contribution

It provides a detailed model of microbial front formation and dynamics in sediment, integrating biological and physical processes for the first time.

## Key findings

- Microbes form stable fronts at the oxic-anoxic interface.
- Fronts move steadily towards the surface and stabilize at a fixed depth.
- Transient parallel fronts and bioconvective plumes are observed.

## Abstract

Organic material in anoxic sediment represents a globally significant carbon reservoir that acts to stabilize Earth's atmospheric composition. The dynamics by which microbes organize to consume this material remain poorly understood. Here we observe the collective dynamics of a microbial community, collected from a salt marsh, as it comes to steady state in a two-dimensional ecosystem, covered by flowing water and under constant illumination. Microbes form a very thin front at the oxic-anoxic interface that moves towards the surface with constant velocity and comes to rest at a fixed depth. Fronts are stable to all perturbations while in the sediment, but develop bioconvective plumes in water. We observe the transient formation of parallel fronts. We model these dynamics to understand how they arise from the coupling between metabolism, aerotaxis, and diffusion. These results identify the typical timescale for the oxygen flux and penetration depth to reach steady state.

## Full text

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## Figures

4 figures with captions in the complete paper: https://tomesphere.com/paper/1704.08212/full.md

## References

40 references — full list in the complete paper: https://tomesphere.com/paper/1704.08212/full.md

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Source: https://tomesphere.com/paper/1704.08212