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arxiv: 2502.13444 · v1 · submitted 2025-02-19 · ⚛️ physics.flu-dyn

Impact of transverse strain on linear, transitional and self-similar turbulent mixing layers

Pith reviewed 2026-05-23 02:59 UTC · model grok-4.3

classification ⚛️ physics.flu-dyn
keywords transverse strainmixing layerRayleigh-Taylor instabilityRichtmyer-Meshkov instabilitybuoyancy-drag modelturbulent mixingimplicit large eddy simulation
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The pith

Transverse compression slows turbulent mixing layer growth, predicted by rescaling drag length in buoyancy-drag model.

A machine-rendered reading of the paper's core claim, the machinery that carries it, and where it could break.

The paper examines how transverse strain modifies mixing layer evolution from Rayleigh-Taylor and Richtmyer-Meshkov instabilities when applied in planar geometry as a proxy for convergent flows. A model for the linear regime predicts amplified growth under transverse compression and matches two-dimensional simulations. In the transitional-to-turbulent regime, implicit large-eddy simulations of a multi-mode case instead show reduced growth, increased mixing, and a shift of turbulent kinetic energy toward transverse components. These turbulent changes are captured by modifying an existing buoyancy-drag model so that its drag length scale scales with the transverse expansion.

Core claim

The mixing layer width is able to be predicted by adjusting the buoyancy-drag model to utilise a drag length scale that scales with the transverse expansion. This accounts for the opposite trend to the linear regime, where turbulent growth decreases under transverse compression while the layer becomes more mixed and turbulent kinetic energy is increasingly dominated by the transverse directions.

What carries the argument

Buoyancy-drag model with drag length rescaled to follow transverse expansion of the mixing layer.

If this is right

  • Linear instability growth is amplified by transverse compression, with solutions equivalent to those in convergent geometry.
  • Turbulent mixing layer width decreases under transverse compression while the mixedness fraction increases.
  • Turbulent kinetic energy anisotropy shifts away from the unstrained self-similar state toward transverse dominance.
  • The adjusted model reproduces the observed width evolution without additional production or dissipation mechanisms.

Where Pith is reading between the lines

These are editorial extensions of the paper, not claims the author makes directly.

  • The mean-strain-rate framework may allow direct use of planar strain data to inform models of spherical or cylindrical convergence without separate compression-rate parameters.
  • Increased mixing under compression could alter predicted fuel-shell mix in inertial confinement fusion implosions that experience transverse strain.
  • The same drag-length rescaling could be tested against other initial perturbation spectra or against direct numerical simulations at higher Reynolds numbers.

Load-bearing premise

The effects of transverse strain on the transitional-to-turbulent regime can be captured solely by rescaling the drag length without introducing new source or sink terms for turbulent kinetic energy or mixing.

What would settle it

A three-dimensional implicit large-eddy simulation of the quarter-scale multi-mode initial condition under a fixed transverse strain rate that produces a mixing layer width differing from the rescaled buoyancy-drag prediction at late times.

Figures

Figures reproduced from arXiv: 2502.13444 by Ben Thornber, Bradley Pascoe, David L. Youngs, Michael Groom.

Figure 1
Figure 1. Figure 1: Interface at 𝜏 = 0.1 for the 2-D single-mode simulations. Heavy fluid ( 𝑓1 = 1) is red, light fluid ( 𝑓1 = 0) is blue. Major ticks indicate a distance of 𝜆(𝑡)/4, with the final wavelength marked below the plot. (a) Constant velocity, 𝑆ˆ 0 = −7.5; (b) Unstrained case; (c) Constant velocity, 𝑆ˆ 0 = 30; (d) Constant strain rate, 𝑆ˆ = −14; (e) Constant strain rate, 𝑆ˆ = 14. A second-order interpolation scheme … view at source ↗
Figure 2
Figure 2. Figure 2: Amplitude of the single mode linear regime, non-dimensionalised for the initial [PITH_FULL_IMAGE:figures/full_fig_p018_2.png] view at source ↗
Figure 3
Figure 3. Figure 3: Amplitude of the single mode linear regime, non-dimensionalised by the [PITH_FULL_IMAGE:figures/full_fig_p019_3.png] view at source ↗
Figure 4
Figure 4. Figure 4: Error in the amplitude for the linear regime under ( [PITH_FULL_IMAGE:figures/full_fig_p019_4.png] view at source ↗
Figure 5
Figure 5. Figure 5: Contours of the volume fraction for the constant velocity ILES cases at the [PITH_FULL_IMAGE:figures/full_fig_p023_5.png] view at source ↗
Figure 6
Figure 6. Figure 6: Contour of volume fraction 𝑓1 for the expansion mixing layers at Λ ≈ 1.82, bounded by 𝑓1 = 0.99 (red) and 𝑓1 = 0.01 (blue). (a) 𝑆ˆ 0 = 0.102, 𝜏 = 9.05, (b) 𝑆ˆ = 0.081, 𝜏 = 8.37, (c) 𝑆ˆ 0 = 0.025, 𝜏 = 33.5, (d) 𝑆ˆ 0 = 0.020, 𝜏 = 30.5 (a) 𝑥 𝑦 𝑧 (b) (c) (d) [PITH_FULL_IMAGE:figures/full_fig_p024_6.png] view at source ↗
Figure 7
Figure 7. Figure 7: Contour of volume fraction 𝑓1 for the expansion mixing layers at Λ ≈ 0.57, bounded by 𝑓1 = 0.99 (red) and 𝑓1 = 0.01 (blue). (a) 𝑆ˆ 0 = −0.051, 𝜏 = 9.45, (b) 𝑆ˆ = −0.081, 𝜏 = 7.88, (c) 𝑆ˆ 0 = −0.013, 𝜏 = 34.9, (d) 𝑆ˆ 0 = −0.020, 𝜏 = 28.5 much closer to the unstrained simulation than was observed for cases with axial strain rates in Pascoe et al. (2024), where the strain rate causes the mixing layer to stret… view at source ↗
Figure 8
Figure 8. Figure 8: Integral width for (a) constant velocity, and (b) constant strain rate. (Zhou et al. 2016): M = ∫ 4𝜌𝑌1𝑌2𝑑𝑉 (4.4) The profiles of the mixed mass are plotted in figure 9, and show a different trend compared to the integral width. For the mixed mass, the compression cases achieve slightly higher growth and the expansion cases achieve less growth. As the name mixed mass suggests, it is not purely a measure of … view at source ↗
Figure 9
Figure 9. Figure 9: Mixed mass for (a) constant velocity and (b) constant strain rate. To reduce the impact of statistical fluctuations, the bubble and spike heights used are based off the integral measure proposed by Youngs & Thornber (2020a): ℎ¯ (𝑚) 𝑏 =       (𝑚 + 1) (𝑚 + 2) 2 ∫ 0 −∞ |𝑥 ′ | 𝑚(1 − ¯𝑓1)𝑑𝑥′ ∫ 0 −∞ (1 − ¯𝑓1)𝑑𝑥′       1/𝑚 , (4.6a) ℎ¯ (𝑚) 𝑠 = " (𝑚 + 1) (𝑚 + 2) 2 ∫ ∞ 0 |𝑥 ′ | 𝑚 ¯𝑓1𝑑𝑥′ ∫ ∞ 0 ¯𝑓1𝑑𝑥′ #1/𝑚… view at source ↗
Figure 10
Figure 10. Figure 10: Bubble and spike heights for (a) constant velocity and (b) constant strain rate. Solid lines indicate bubble height, dashed lines indicate spike height. 0 0 0 0 τ 0  0   ̂ 0  00 ̂ 0  00 ̂ 0  0000 ̂ 0   00 ̂ 0   00 (a) 0 0 0 0 τ 0  0   ̂ 00 ̂ 000 ̂ 0000 ̂  000 ̂  00 (b) [PITH_FULL_IMAGE:figures/full_fig_p027_10.png] view at source ↗
Figure 11
Figure 11. Figure 11: Ratio of spike-to-bubble height for (a) constant velocity and (b) constant strain rate. molecular mixing fraction measures how well the species in the mixing layer are mixed, as measured by the volume fraction. A value of Θ = 0 suggests complete segregation, whilst Θ = 1 suggests perfect homogeneity in the plane. The molecular mixing fraction is calculated by Θ(𝑡) = ∫ 𝑓1 𝑓2𝑑𝑥 ∫ ¯𝑓1 ¯𝑓2𝑑𝑥 . (4.7) At late-t… view at source ↗
Figure 12
Figure 12. Figure 12: Mixing measures for the (a) constant velocity and (b) constant strain rate. Solid lines indicate Θ, dashed lines indicate Ψ, dotted line is FLAMENCO’s final Θ value at 𝜏 = 246 (Thornber et al. 2017). This is the same trend as observed when axial strain rates are applied to the mixing layer, such that a decrease in turbulent growth of the mixing layer corresponds to an increase in the mixedness. The differ… view at source ↗
Figure 13
Figure 13. Figure 13: Planar-averaged volume-fraction profiles for the constant velocity cases: ( [PITH_FULL_IMAGE:figures/full_fig_p030_13.png] view at source ↗
Figure 14
Figure 14. Figure 14: Planar-averaged volume-fraction profiles for the constant strain rate cases: ( [PITH_FULL_IMAGE:figures/full_fig_p030_14.png] view at source ↗
Figure 15
Figure 15. Figure 15: Total turbulent kinetic energy for (a) constant velocity and (b) constant strain rate. Solid lines indicate ILES, gray dashed lines indicate the turbulent kinetic energy model, and black dotted lines indicate the corrected turbulent kinetic energy model. 1 11 τ 1 11  ̂   1 ̂    ̂    ̂   1 ̂   1 (a) 1 11 τ 1 11  ̂  1 ̂   ̂   ̂   ̂  1 (b) [P… view at source ↗
Figure 16
Figure 16. Figure 16: Turbulent kinetic energy in the 𝑦-direction for (a) constant velocity and (b) constant strain rate. Solid lines indicate ILES, gray dashed lines indicate the turbulent kinetic energy model, and black dotted lines indicate the corrected turbulent kinetic energy model. the transverse energy and the shear production contribution whilst increasing the 𝑇𝐾 𝑋 component. By the same process, redistribution of ene… view at source ↗
Figure 17
Figure 17. Figure 17: Turbulent kinetic energy in the 𝑥-direction for (a) constant velocity and (b) constant strain rate. Solid lines indicate ILES, and black dotted lines indicate the corrected turbulent kinetic energy model. factors: 𝜀 = 𝐶𝜖 𝑇𝐾𝐸3/2 𝑊 √ 𝑀Λ2/3 (4.15) As the strain rates are only applied in two out of the three dimensions, the resulting scale is to the power of 2/3. The results for this corrected model are also … view at source ↗
Figure 18
Figure 18. Figure 18: Anisotropy of the turbulent kinetic energy for ( [PITH_FULL_IMAGE:figures/full_fig_p036_18.png] view at source ↗
Figure 19
Figure 19. Figure 19: Turbulent mass flux for (a) constant velocity, and (b) constant strain rate. Solid lines indicate results at 𝜏 = 9.843, dashed lines indicate results at 𝜏 = 34.451. 4.2.6. Enstrophy The modelling of the pressure-dilatation tensor can be avoided by analysing the vorticity or enstrophy of the flow. The vorticity is defined by the curl of the velocity field, 𝜔𝑖 = 𝜖𝑖 𝑗𝑘 𝜕𝑢𝑘 𝜕𝑥 𝑗 . (4.18) For a compressible, v… view at source ↗
Figure 20
Figure 20. Figure 20: Enstrophy in the 𝑦 − 𝑧 plane for (a) constant velocity and (b) constant strain rate. Solid lines indicate ILES, dashed lines indicate the enstrophy model. 1 11 τ 1 11 1 [PITH_FULL_IMAGE:figures/full_fig_p040_20.png] view at source ↗
Figure 21
Figure 21. Figure 21: Enstrophy in the 𝑥 − 𝑧 plane for (a) constant velocity and (b) constant strain rate. Solid lines indicate ILES, dashed lines indicate the enstrophy model. the K-L turbulence model (Dimonte & Tipton 2006) which collapses to the buoyancy-drag model under a self-similar analysis. The most relevant buoyancy-drag model to the cases investigated here are the models calibrated to the quarter-scale 𝜃-group case b… view at source ↗
Figure 22
Figure 22. Figure 22: Effective drag lengthscale as a function of non-dimensionalised integral width [PITH_FULL_IMAGE:figures/full_fig_p042_22.png] view at source ↗
Figure 23
Figure 23. Figure 23: Buoyancy-drag model for integral width: ( [PITH_FULL_IMAGE:figures/full_fig_p044_23.png] view at source ↗
Figure 24
Figure 24. Figure 24: Buoyancy-drag model for bubble height: ( [PITH_FULL_IMAGE:figures/full_fig_p044_24.png] view at source ↗
Figure 25
Figure 25. Figure 25: Buoyancy-drag model for spike height. (a) constant velocity and (b) constant strain rate. Solid lines indicate ILES results, dashed lines indicate the buoyancy-drag model [PITH_FULL_IMAGE:figures/full_fig_p044_25.png] view at source ↗
Figure 26
Figure 26. Figure 26: Convergence of constant strain rate simulations under transverse compression [PITH_FULL_IMAGE:figures/full_fig_p047_26.png] view at source ↗
read the original abstract

The growth of interfacial instabilities such as the Rayleigh-Taylor (RTI) and Richtmyer-Meshkov instability (RMI) are modified when developing in convergent geometries. Whilst these modifications are usually quantified by the compression rate and convergence rate of the mixing layer, an alternative framework is proposed, describing the evolution of the mixing layer through the effects of the mean strain rates experienced by the mixing layer. An investigation into the effect of the transverse strain rate on the mixing layer development is conducted through application of transverse strain rates in planar geometry. A model for the linear regime in planar geometry with transverse strain rate is derived, with equivalent solutions to convergent geometry, and validated with two-dimensional simulations demonstrating the amplification of the instability growth under transverse compression. The effect of the transverse strain rate on the transitional-to-turbulent mixing layer is investigated with implicit large eddy simulation based on the multi-mode quarter-scale $\theta$-group case by Thornber et al. (Phys. Fluids, vol. 29, 2017, 105107). The mixing layer's growth exhibits the opposite trend to the linear regime model, with reduced growth under transverse compression. The effect of shear-production under transverse compression causes the mixing layer to become more mixed and the turbulent kinetic energy is increasingly dominated by the transverse directions, deviating from the unstrained self-similar state. The mixing layer width is able to be predicted by adjusting the buoyancy-drag model by Youngs & Thornber (Physica D, vol. 410, 2020, 132517) to utilise a drag length scale that scales with the transverse expansion.

Editorial analysis

A structured set of objections, weighed in public.

Desk editor's note, referee report, simulated authors' rebuttal, and a circularity audit. Tearing a paper down is the easy half of reading it; the pith above is the substance, this is the friction.

Referee Report

2 major / 2 minor

Summary. The manuscript investigates the effects of transverse strain on Rayleigh-Taylor and Richtmyer-Meshkov mixing layers in planar geometry as a proxy for convergent configurations. It derives a linear stability model showing growth amplification under transverse compression (with solutions equivalent to convergent geometry), validates this with 2D simulations, and then uses implicit LES of multi-mode cases to show the opposite trend in the transitional-to-turbulent regime: reduced growth, increased mixing fraction, and TKE anisotropy with transverse dominance. The central claim is that mixing-layer width can be predicted by modifying the Youngs & Thornber buoyancy-drag model to employ a drag length scale that scales with transverse expansion.

Significance. If the adjusted buoyancy-drag model proves robust, the work supplies a strain-rate framework that could simplify modeling of convergent RTI/RMI relative to compression-rate approaches, with relevance to inertial confinement fusion and astrophysical flows. The linear-regime derivation and its 2D validation constitute a clear strength; the turbulent-regime results highlight physically interesting deviations from self-similarity.

major comments (2)
  1. [Abstract (turbulent regime) and model-adjustment section] Abstract and turbulent-regime results: the claim that mixing-layer width is predicted by rescaling the drag length in the Youngs & Thornber (Physica D, 2020) buoyancy-drag model rests on a scaling chosen to match the ILES data rather than obtained from an independent derivation or external benchmark; this renders the central turbulent prediction circular and potentially case-specific.
  2. [ILES results and model adjustment] ILES analysis: the simulations show that transverse compression increases the mixing fraction and shifts TKE dominance to the transverse components, breaking the unstrained self-similar state; the model adjustment omits any new source/sink terms for this anisotropy or enhanced production, so the width match achieved solely by drag-length rescaling does not demonstrate that the underlying turbulent-state changes have been captured.
minor comments (2)
  1. The specific functional form adopted for the transverse-expansion drag-length scaling (including any fitted coefficient) should be stated explicitly with its numerical value and the fitting procedure used.
  2. Clarify whether the linear-model derivation assumes incompressible flow or includes any compressibility corrections that would be relevant when mapping to convergent geometries.

Simulated Author's Rebuttal

2 responses · 0 unresolved

We thank the referee for their constructive review highlighting important aspects of our turbulent-regime analysis. We respond point-by-point to the major comments below, clarifying the physical motivation for the model adjustment while acknowledging its phenomenological nature.

read point-by-point responses
  1. Referee: [Abstract (turbulent regime) and model-adjustment section] Abstract and turbulent-regime results: the claim that mixing-layer width is predicted by rescaling the drag length in the Youngs & Thornber (Physica D, 2020) buoyancy-drag model rests on a scaling chosen to match the ILES data rather than obtained from an independent derivation or external benchmark; this renders the central turbulent prediction circular and potentially case-specific.

    Authors: The proposed scaling of the drag length with transverse expansion is guided by the strain-rate framework developed in the manuscript. The linear analysis and 2D simulations establish that transverse compression amplifies growth, while the ILES reveal the opposite trend in the turbulent regime due to strain-induced changes in mixing and anisotropy. The drag-length adjustment is therefore motivated as an effective representation of how transverse expansion alters the characteristic length in the drag term, reversing the linear trend. Although the precise functional dependence was identified to reproduce the simulated widths, it is not an arbitrary fit but a direct consequence of incorporating the transverse strain into the existing Youngs & Thornber model. We view the ILES as validation of this extension rather than the sole determinant of its form, and the approach remains testable on additional configurations. revision: no

  2. Referee: [ILES results and model adjustment] ILES analysis: the simulations show that transverse compression increases the mixing fraction and shifts TKE dominance to the transverse components, breaking the unstrained self-similar state; the model adjustment omits any new source/sink terms for this anisotropy or enhanced production, so the width match achieved solely by drag-length rescaling does not demonstrate that the underlying turbulent-state changes have been captured.

    Authors: The buoyancy-drag model is a reduced-order description whose purpose is to predict mixing-layer width, not the detailed evolution of the Reynolds-stress tensor or mixing fraction. The drag-length rescaling provides an effective means to incorporate the net influence of the observed anisotropy and altered production on the growth rate, without introducing additional transport equations. We do not claim that this adjustment resolves the internal turbulent state; it only reproduces the width evolution that results from those changes. This constitutes a limitation of the simple model, and more complete closures would be required to capture the TKE anisotropy explicitly. revision: partial

Circularity Check

2 steps flagged

Mixing layer width prediction reduces to fitted rescaling of drag length in self-cited buoyancy-drag model

specific steps
  1. fitted input called prediction [Abstract (final sentence); model-adjustment discussion]
    "The mixing layer width is able to be predicted by adjusting the buoyancy-drag model by Youngs & Thornber (Physica D, vol. 410, 2020, 132517) to utilise a drag length scale that scales with the transverse expansion."

    The scaling factor for the drag length is selected so that the model reproduces the simulated mixing-layer widths under transverse strain. The 'prediction' is therefore the output of a parameter fit to the same growth-rate data it is claimed to predict, with no independent derivation of the scaling provided.

  2. self citation load bearing [Abstract; model section]
    "adjusting the buoyancy-drag model by Youngs & Thornber (Physica D, vol. 410, 2020, 132517)"

    The load-bearing turbulent model is taken from prior work co-authored by Thornber; the only modification is the fitted drag-length rescaling. No external validation or machine-checked uniqueness result is cited to justify that this single change captures the observed TKE anisotropy and enhanced mixing.

full rationale

The linear-regime derivation is self-contained and independent. However, the central claim for the transitional-to-turbulent regime states that width is 'predicted' by adjusting the Youngs & Thornber buoyancy-drag model via a drag-length scaling chosen to match the ILES data. This adjustment is data-driven rather than derived from first principles or external benchmarks, and the base model is self-cited. The result is therefore partially forced by construction on the simulation inputs.

Axiom & Free-Parameter Ledger

1 free parameters · 2 axioms · 0 invented entities

The work relies on standard incompressible or weakly compressible Navier-Stokes assumptions plus the specific modeling choice that transverse strain enters only through a rescaled drag length. No new particles or forces are postulated.

free parameters (1)
  • transverse-expansion drag-length scaling coefficient
    The functional dependence of the drag length on transverse strain is introduced to match the observed turbulent growth; its coefficient is not derived from first principles.
axioms (2)
  • domain assumption The mean strain-rate tensor can be imposed independently of the instability growth in planar geometry.
    Invoked when the authors apply transverse strain rates to planar mixing layers to mimic convergent geometry.
  • domain assumption The buoyancy-drag model remains structurally valid once the drag length is rescaled.
    Central modeling step for the turbulent-regime prediction.

pith-pipeline@v0.9.0 · 5833 in / 1520 out tokens · 25405 ms · 2026-05-23T02:59:57.942131+00:00 · methodology

discussion (0)

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