Repository logo
Log in(current)
Repository logoMIT Open ScholarshipDSpace@MIT
  1. Home
  2. MIT Open Access Articles
  3. MIT Open Access Articles
  4. The nature of triad interactions in active turbulence

The nature of triad interactions in active turbulence

Thumbnail Image
Download
Name

1708.01394.pdf

Size

2.76 MB

Format

Adobe PDF

Checksum (MD5)

faf5feda1a9d0a8b79482bce4d0df5e0

Download all files submitted through automated deposit
sword-2018-05-18.original.zip (2.59 MB)
Author(s)
Slomka, Jonasz Jozef
•
Suwara, Piotr
•
Dunkel, Joern
Date Issued
April 2018
Journal
Journal of Fluid Mechanics
Publisher
Cambridge University Press
Citation
Słomka, Jonasz et al. “The Nature of Triad Interactions in Active Turbulence.” Journal of Fluid Mechanics 841 (February 2018): 702–731 © 2018 Cambridge University Press
Version
Original manuscript
Abstract
Generalised Navier-Stokes (GNS) equations describing three-dimensional active fluids with flow-dependent narrow spectral forcing have been shown to possess numerical solutions that can sustain significant energy transfer to larger scales by realising chiral Beltrami-type chaotic flows. To rationalise these findings, we study here the triad truncations of polynomial and Gaussian GNS models focusing on modes lying in the energy injection range. Identifying a previously unknown cubic invariant for the triads, we show that their asymptotic dynamics reduces to that of a forced rigid body coupled to a particle moving in a magnetic field. This analogy allows us to classify triadic interactions by their asymptotic stability: unstable triads correspond to rigid-body forcing along the largest and smallest principal axes, whereas stable triads arise from forcing along the middle axis. Analysis of the polynomial GNS model reveals that unstable triads induce exponential growth of energy and helicity, whereas stable triads develop a limit cycle of bounded energy and helicity. This suggests that the unstable triads dominate the initial relaxation stage of the full hydrodynamic equations, whereas the stable triads determine the statistically stationary state. To test whether this hypothesis extends beyond polynomial dispersion relations, we introduce and investigate an alternative Gaussian active turbulence model. Similar to the polynomial case, the steady-state chaotic flows in the Gaussian model spontaneously accumulate non-zero mean helicity while exhibiting Beltrami statistics and upward energy transport. Our results suggest that self-sustained Beltrami-type flows and an inverse energy cascade may arise generically in the presence of flow-dependent narrow spectral forcing.
MIT Department
Massachusetts Institute of Technology. Department of Mathematics
Terms of Use
Creative Commons Attribution-Noncommercial-Share Alike
http://creativecommons.org/licenses/by-nc-sa/4.0/
Persistent DSpace Link
http://hdl.handle.net/1721.1/115497
DOI of Published Version
https://doi.org/10.1017/jfm.2018.108
Repository logo
PrivacyPermissionsAccessibilityContact us
Repository logo
Notify us about copyright concerns.