Power-law spectral decay as a general feature of spiral turbulence

Spiral waves emitted by topological defects and their instabilities are a fundamental and ubiquitous process in nature. We study this phenomenon using data from recent experiments and different prototype models ranging from coupled oscillators, reaction-diffusion, and nonlinear optics. Statistically...

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Main Authors: Y. Soupart, M. G. Clerc, M. Tlidi
Format: Article
Language:English
Published: American Physical Society 2025-05-01
Series:Physical Review Research
Online Access:http://doi.org/10.1103/PhysRevResearch.7.023136
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author Y. Soupart
M. G. Clerc
M. Tlidi
author_facet Y. Soupart
M. G. Clerc
M. Tlidi
author_sort Y. Soupart
collection DOAJ
description Spiral waves emitted by topological defects and their instabilities are a fundamental and ubiquitous process in nature. We study this phenomenon using data from recent experiments and different prototype models ranging from coupled oscillators, reaction-diffusion, and nonlinear optics. Statistically we show that, for all systems considered, the spectral density exhibits a power-law decay on spatial scales shorter than the intrinsic wavelength. This reflects a common type of self-organization through a stationary turbulentlike dynamics. The role of short-range interactions due to high defects density is discussed. Using a generalized Hilbert transform in two dimensions, we show that local phase and amplitude field present similar power-law decays in their spectral density.
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series Physical Review Research
spelling doaj-art-67789fd3602a4a6eb80bad5e4e7d0c452025-08-20T01:50:31ZengAmerican Physical SocietyPhysical Review Research2643-15642025-05-017202313610.1103/PhysRevResearch.7.023136Power-law spectral decay as a general feature of spiral turbulenceY. SoupartM. G. ClercM. TlidiSpiral waves emitted by topological defects and their instabilities are a fundamental and ubiquitous process in nature. We study this phenomenon using data from recent experiments and different prototype models ranging from coupled oscillators, reaction-diffusion, and nonlinear optics. Statistically we show that, for all systems considered, the spectral density exhibits a power-law decay on spatial scales shorter than the intrinsic wavelength. This reflects a common type of self-organization through a stationary turbulentlike dynamics. The role of short-range interactions due to high defects density is discussed. Using a generalized Hilbert transform in two dimensions, we show that local phase and amplitude field present similar power-law decays in their spectral density.http://doi.org/10.1103/PhysRevResearch.7.023136
spellingShingle Y. Soupart
M. G. Clerc
M. Tlidi
Power-law spectral decay as a general feature of spiral turbulence
Physical Review Research
title Power-law spectral decay as a general feature of spiral turbulence
title_full Power-law spectral decay as a general feature of spiral turbulence
title_fullStr Power-law spectral decay as a general feature of spiral turbulence
title_full_unstemmed Power-law spectral decay as a general feature of spiral turbulence
title_short Power-law spectral decay as a general feature of spiral turbulence
title_sort power law spectral decay as a general feature of spiral turbulence
url http://doi.org/10.1103/PhysRevResearch.7.023136
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