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pith:QQR5GZWK

pith:2026:QQR5GZWKAEKLVBTO5GGJNFU4CJ
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Solutocapillary instability in slipping falling films

Asim Mukhopadhyay, Bastien Di Pierro, Sanghasri Mukhopadhyay, S\'everine Millet

Wall slip reduces Marangoni back-stress and stabilizes surfactant-laden falling films into single broad crests or flat sheets.

arxiv:2605.17519 v1 · 2026-05-17 · physics.flu-dyn · math.AP

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Claims

C1strongest claim

Wall slip emerges as a key control parameter, reducing viscous resistance and mitigating Marangoni back-stress. The slip parameter β is a useful control knob for surfactant-laden films that prevents fragile multi-hump bound states and promotes single broad crests or almost flat sheets.

C2weakest assumption

The long-wave approximation together with the chosen conservative bulk-surface mass balance and Navier slip condition remain quantitatively accurate across the full range of equilibrium surfactant coverages, Marangoni strengths, and adsorption kinetics examined in the nonlinear simulations.

C3one line summary

Wall slip in surfactant-laden falling films produces non-monotonic critical Reynolds numbers with equilibrium coverage, drives a single-to-double-hump transition in solitary waves, and resolves spurious interfacial mass growth via a revised conservative surface balance.

References

22 extracted · 22 resolved · 1 Pith anchors

[1] Solutocapillary instability in slipping falling films 2026 · arXiv:2605.17519
[2] ∂Γ ∂t + 1p 1 +ε 2h2x ∂(Γus) ∂x # = ε2 P es p 1 +ε 2h2x ∂ ∂x
[3] 2 This eigen value corresponds to the hydrodynamic Kapitza modeα (1); for more information, see Appendix B
[4] For, ˆV= 2 ˆUN = (gsinθ ˆh2 N /ν)(1 + 2β) as twice the dimensional Nusselt free surface velocity and redefine the Reynolds number asRe= ˆUNˆhN /ν, thenRe/F r 2 = 2/(1 + 2β)[52]
[5] For detailed information, see Mukhopadhyay & Mukhopadhyay [36] 2000

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Cited by

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First computed 2026-05-20T00:04:43.457205Z
Builder pith-number-builder-2026-05-17-v1
Signature Pith Ed25519 (pith-v1-2026-05) · public key
Schema pith-number/v1.0

Canonical hash

8423d366ca0114ba866ee98c96969c126f9ff43916eb813fd64f8a5c53e1b254

Aliases

arxiv: 2605.17519 · arxiv_version: 2605.17519v1 · doi: 10.48550/arxiv.2605.17519 · pith_short_12: QQR5GZWKAEKL · pith_short_16: QQR5GZWKAEKLVBTO · pith_short_8: QQR5GZWK
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curl -sH 'Accept: application/ld+json' https://pith.science/pith/QQR5GZWKAEKLVBTO5GGJNFU4CJ \
  | jq -c '.canonical_record' \
  | python3 -c "import sys,json,hashlib; b=json.dumps(json.loads(sys.stdin.read()), sort_keys=True, separators=(',',':'), ensure_ascii=False).encode(); print(hashlib.sha256(b).hexdigest())"
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Canonical record JSON
{
  "metadata": {
    "abstract_canon_sha256": "413bcf0d0bd9d9be069ba71ecc2e11c8c9c2e9dbce1d0cfc90a9a81283ae9a19",
    "cross_cats_sorted": [
      "math.AP"
    ],
    "license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
    "primary_cat": "physics.flu-dyn",
    "submitted_at": "2026-05-17T16:03:36Z",
    "title_canon_sha256": "26f74b6aee265081f538580cddf42b09acc3bf1da944fb6567495f11a1fe8b52"
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  "source": {
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    "kind": "arxiv",
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}