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Implications of local decorrelator growth-rate statistics for Lagrangian chaos

Investigate the implications of the observed distributions of the local growth-rate fields \(\lambda_S(\mathbf{x})\) and \(\lambda_\eta(\mathbf{x})\)—including exponential and power-law tails—for Lagrangian chaos in three-dimensional, forced, homogeneous and isotropic Navier–Stokes turbulence.

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Background

By measuring spatially local exponents for decorrelator growth, the authors find exponential tails for the strain contribution λS(x)\lambda_S(\mathbf{x}) and power-law tails for the viscous contribution λη(x)\lambda_\eta(\mathbf{x}). These findings point to strong intermittent fluctuations that could affect Lagrangian properties of turbulence, such as particle or tracer separation statistics and Lyapunov exponents.

The paper does not analyze these Lagrangian implications and explicitly defers them, identifying this as a direction for future investigation tied to the detailed statistics of βS\beta_S and βη\beta_\eta.

References

We do not explore these ideas, and in particular the origins of the power-law tails, any further in this work as well as its implications for Lagrangian chaos, but leave it for a more detailed study of the statistics of \beta_S and \beta_\eta in the future.

Intermittent fluctuations determine the nature of chaos in turbulence (2505.09538 - Banerjee et al., 14 May 2025) in Main text, final paragraph before Acknowledgements