Shock trapping and inertial escape: Dust-particle clustering in compressible turbulence

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Main Authors: Kankaria, Anikat, Ray, Samriddhi Sankar
Format: Preprint
Published: 2025
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author Kankaria, Anikat
Ray, Samriddhi Sankar
author_facet Kankaria, Anikat
Ray, Samriddhi Sankar
contents We study the dynamics and clustering of dust particles with inertia in shock-dominated compressible turbulence using the two-dimensional, stochastically forced Burgers equation. At small Stokes numbers, shock trapping leads to extreme density inhomogeneities and nearly singular aggregation, with correlation dimensions approaching zero. With increasing inertia, particles undergo inertial escape and intermittently cross shock fronts, producing a sharp crossover from shock-dominated trapping to quasi-ballistic dynamics. This crossover is accompanied by a pronounced reduction in density fluctuations, a continuous increase of the correlation dimension from zero to the embedding dimension, and a power-law dependence of density fluctuations on the Stokes number over an extended intermediate regime. In this regime, particle distributions show scale-free coarse-grained density statistics arising from repeated trap--escape dynamics. This behaviour is qualitatively distinct from inertial-particle clustering in incompressible turbulence and is directly relevant to dust concentration in shock-rich regions of protoplanetary discs and other compressible astrophysical environments.
format Preprint
id arxiv_https___arxiv_org_abs_2512_07164
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle Shock trapping and inertial escape: Dust-particle clustering in compressible turbulence
Kankaria, Anikat
Ray, Samriddhi Sankar
Fluid Dynamics
Earth and Planetary Astrophysics
Astrophysics of Galaxies
Chaotic Dynamics
We study the dynamics and clustering of dust particles with inertia in shock-dominated compressible turbulence using the two-dimensional, stochastically forced Burgers equation. At small Stokes numbers, shock trapping leads to extreme density inhomogeneities and nearly singular aggregation, with correlation dimensions approaching zero. With increasing inertia, particles undergo inertial escape and intermittently cross shock fronts, producing a sharp crossover from shock-dominated trapping to quasi-ballistic dynamics. This crossover is accompanied by a pronounced reduction in density fluctuations, a continuous increase of the correlation dimension from zero to the embedding dimension, and a power-law dependence of density fluctuations on the Stokes number over an extended intermediate regime. In this regime, particle distributions show scale-free coarse-grained density statistics arising from repeated trap--escape dynamics. This behaviour is qualitatively distinct from inertial-particle clustering in incompressible turbulence and is directly relevant to dust concentration in shock-rich regions of protoplanetary discs and other compressible astrophysical environments.
title Shock trapping and inertial escape: Dust-particle clustering in compressible turbulence
topic Fluid Dynamics
Earth and Planetary Astrophysics
Astrophysics of Galaxies
Chaotic Dynamics
url https://arxiv.org/abs/2512.07164