posted on 2018-12-07, 14:37authored byTyler Shendruk, Kristian Thijssen, Julia M. Yeomans, Amin Doostmohammadi
While studies of active nematics in two dimensions have shed light on various aspects of the flow regimes
and topology of active matter, three-dimensional properties of topological defects and chaotic flows remain
unexplored. By confining a film of active nematics between two parallel plates, we use continuum simulations
and analytical arguments to demonstrate that the crossover from quasi-two-dimensional (quasi-2D) to threedimensional
(3D) chaotic flows is controlled by the morphology of the disclination lines. For small plate
separations, the active nematic behaves as a quasi-2D material, with straight topological disclination lines spanning
the height of the channel and exhibiting effectively 2D active turbulence. Upon increasing channel height, we
find a crossover to 3D chaotic flows due to the contortion of disclinations above a critical activity. Above this
critical activity highly contorted disclination lines and disclination loops are formed. We further show that these
contortions are engendered by twist perturbations producing a sharp change in the curvature of disclinations.
Funding
. K.T. was funded by the European Union’s Horizon
2020 research and innovation programme under the Marie
Skłodowska-Curie Grant Agreement No. 722497. A.D. was
supported by a Royal Commission for the Exhibition of 1851
Research Fellowship
History
School
Science
Department
Mathematical Sciences
Published in
Physical Review E
Volume
98
Issue
1
Citation
SHENDRUK, T.N., 2018. Twist-induced crossover from two-dimensional to three-dimensional turbulence in active nematics. Physical Review E, 98: 010601(R).
This work is made available according to the conditions of the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International (CC BY-NC-ND 4.0) licence. Full details of this licence are available at: https://creativecommons.org/licenses/by-nc-nd/4.0/
Acceptance date
2018-06-01
Publication date
2018-07-13
Notes
This paper was accepted for publication in the journal Physical Review E and the definitive published version is available at https://doi.org/10.1103/PhysRevE.98.010601