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PreprintCC BY 4.0arXiv

Regional accuracy of physics-informed neural networks (PINNs) for recirculation in a deep lid-driven cavity

Abstract

Deep lid-driven cavities contain strong motion beneath the lid and much weaker recirculation at depth, so agreement in bulk velocity is an incomplete assessment of a computed flow. We examine data-free physics-informed neural networks (PINNs) for steady, two-dimensional incompressible flow in a cavity of depth-to-width ratio five at Reynolds numbers 100, 250, 500 and 1000. An established hard-constrained streamfunction formulation is combined with prescribed regional collocation, transferred initialization, and selected residual-scaling and envelope variants. Independent spectral/hp calculations with the same Gaussian-regularized lid provide the reference fields. For a cavity of depth-to-width ratio D/W=5 at Reynolds numbers Re=100, 250, 500, and 1000, evaluation on a common 121×605 grid gives interior relative velocity discrepancies of 5.130\%--7.850\%. Over the same cases, floor-region relative velocity discrepancies remain below 5\%, with absolute RMS discrepancies ranging from 1.255×10−10U to 2.332×10−9U, where U is the lid-velocity scale. In a separate 161×801 assessment at Rey=1000, the refined workflow lowers interior velocity discrepancy from 5.624\% to 2.658\% and gauge-aligned pressure RMS discrepancy from 2.793×10−3 to 1.167×10−3ρU2. The improvements compare accumulated training workflows and do not isolate regional sampling. Configuration rankings depend on both region and observable. These finite-budget comparisons establish where the retained workflows agree with the reference and where rotational-field discrepancies remain substantial.

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BibTeX
@misc{roohi2026regional,
  title = {{Regional accuracy of physics-informed neural networks (PINNs) for recirculation in a deep lid-driven cavity}},
  author = {Ehsan Roohi and Christopher J. McDevitt},
  howpublished = {arXiv},
  year = {2026},
  month = oct,
  doi = {10.48550/arxiv.2610.38814},
  eprint = {2610.38814},
  archivePrefix = {arXiv},
  url = {https://arxiv.org/abs/2610.38814},
  note = {CC BY 4.0},
}
RIS
TY  - UNPB
TI  - Regional accuracy of physics-informed neural networks (PINNs) for recirculation in a deep lid-driven cavity
AU  - Ehsan Roohi
AU  - Christopher J. McDevitt
PY  - 2026
DA  - 2026/10/28
PB  - arXiv
DO  - 10.48550/arxiv.2610.38814
UR  - https://arxiv.org/abs/2610.38814
AB  - Deep lid-driven cavities contain strong motion beneath the lid and much weaker recirculation at depth, so agreement in bulk velocity is an incomplete assessment of a computed flow. We examine data-free physics-informed neural networks (PINNs) for steady, two-dimensional incompressible flow in a cavity of depth-to-width ratio five at Reynolds numbers 100, 250, 500 and 1000. An established hard-constrained streamfunction formulation is combined with prescribed regional collocation, transferred initialization, and selected residual-scaling and envelope variants. Independent spectral/hp calculations with the same Gaussian-regularized lid provide the reference fields. For a cavity of depth-to-width ratio D/W=5 at Reynolds numbers Re=100, 250, 500, and 1000, evaluation on a common 121×605 grid gives interior relative velocity discrepancies of 5.130\%--7.850\%. Over the same cases, floor-region relative velocity discrepancies remain below 5\%, with absolute RMS discrepancies ranging from 1.255×10^−10U to 2.332×10^−9U, where U is the lid-velocity scale. In a separate 161×801 assessment at Rey=1000, the refined workflow lowers interior velocity discrepancy from 5.624\% to 2.658\% and gauge-aligned pressure RMS discrepancy from 2.793×10^−3 to 1.167×10^−3ρU^2. The improvements compare accumulated training workflows and do not isolate regional sampling. Configuration rankings depend on both region and observable. These finite-budget comparisons establish where the retained workflows agree with the reference and where rotational-field discrepancies remain substantial.
ER  -