Skip to content
DraconiticResearch
Search Sources API
203,203 studies31 sourcesUpdated 30 min ago
PreprintCC BY 4.0arXiv

Eddies that ride the flow: a model of turbulence with Richardson dispersion and anomalous dissipation

Abstract

We construct a divergence-free velocity field u(x,t) on 𝕋n that is a genuine function of position and carries both defining properties of turbulent transport: Richardson pair dispersion and a dissipative anomaly. No synthetic field has carried both, because the frame that gives the first destroys the field the second requires. The key is a dichotomy: deforming a spectrally localised pattern smears it across scales, whereas pushing its generating centres forward and re-convolving leaves the spectral envelope exactly invariant --- so transporting the eddy centres preserves both cascade and frame. In the field the finite-size Lyapunov exponent obeys ζ(R)=h(R)−1 threshold by threshold within the scaling range, with a sweeping deficit Δsw=+0.038±0.019, consistent with zero, against +0.091±0.019 for the frozen field on the same data, a gap that doubles at Navier--Stokes intermittency. Companion papers prove that this family shows Richardson dispersion and a dissipative anomaly (Fefferman and Mayboroda 2026), and that a scalar advected by this flow obeys Yaglom's relation (De Lellis 2026), at small Kubo number. Trajectories forget their starting point as the smallest eddy is removed: the median separation of pairs released from one point with independent Brownian kicks varies as κp0.0333±0.0038 over 22 decades of particle diffusivity, against κp1/2 for a smooth control. A scalar in the same field closes the exact scale-by-scale variance budget, four independently measured terms balancing the dissipation to 15\% over 1.2 decades with no adjustable constant, and reaches its inertial--convective asymptote SL=−χr to 0.9995±0.0018 once the measured diffusive transfer is restored, while under an imposed mean gradient χ changes by 14\% over a factor 5.8 in κ.

Related

  1. Scalar Dissipation Criticality in Compressible Magnetized Turbulence
    Svitlana Mayboroda, David N. Spergel, Camillo De Lellis
    arXivPreprintCC BY 4.0Full textGalaxiesFluid dynamicsarXiv
  2. Turbulence Cascade in Cygnus X Revealed by Multipoint Velocity Dispersion Function Method
    Junjie Huang, Yangjun Pu, Keping Qiu +3
    The Astrophysical JournalPeer-reviewedCC BY 4.0Full textSolar & stellar physicsCrossref
  3. Probing turbulence in the ionized interstellar medium using young pulsars. I. Dispersion measure variations
    S.J.I Melfor, A Parthasarathy, S Johnston +9
    Astronomy & Astrophysics - A&APeer-reviewedCC BY 4.0Full text1 citedHigh-energy astrophysicsGeneral physicsHALarXiv
  4. Anomalous Electric Fields in Earth's Turbulent Magnetosheath: Insights From 3D Hybrid Simulations
    Jeffersson A. Agudelo Rueda, Julia E. Stawarz, Luca Franci +3
    HALPreprintCC BY 4.0Full textPlanetary science & exoplanetsPlasma physicsHAL
  5. A0538-66: A transient ultraluminous X-ray source with a relativistic outflow, 69,ms pulsations, and anomalous optical activity
    Lorenzo Ducci, Sandro Mereghetti, Ciro Pinto +8
    Astronomy & AstrophysicsPeer-reviewedPublisher termsSolar & stellar physicsCrossref
BibTeX
@misc{jimenez2026eddies,
  title = {{Eddies that ride the flow: a model of turbulence with Richardson dispersion and anomalous dissipation}},
  author = {Raul Jimenez and Svitlana Mayboroda and Camillo de Lellis and David N. Spergel and Max Engelstein},
  howpublished = {arXiv},
  year = {2026},
  month = nov,
  doi = {10.48550/arxiv.2611.07121},
  eprint = {2611.07121},
  archivePrefix = {arXiv},
  url = {https://arxiv.org/abs/2611.07121},
  note = {CC BY 4.0},
}
RIS
TY  - UNPB
TI  - Eddies that ride the flow: a model of turbulence with Richardson dispersion and anomalous dissipation
AU  - Raul Jimenez
AU  - Svitlana Mayboroda
AU  - Camillo de Lellis
AU  - David N. Spergel
AU  - Max Engelstein
PY  - 2026
DA  - 2026/11/04
PB  - arXiv
DO  - 10.48550/arxiv.2611.07121
UR  - https://arxiv.org/abs/2611.07121
AB  - We construct a divergence-free velocity field u(x,t) on 𝕋^n that is a genuine function of position and carries both defining properties of turbulent transport: Richardson pair dispersion and a dissipative anomaly. No synthetic field has carried both, because the frame that gives the first destroys the field the second requires. The key is a dichotomy: deforming a spectrally localised pattern smears it across scales, whereas pushing its generating centres forward and re-convolving leaves the spectral envelope exactly invariant --- so transporting the eddy centres preserves both cascade and frame. In the field the finite-size Lyapunov exponent obeys ζ(R)=h(R)−1 threshold by threshold within the scaling range, with a sweeping deficit Δ_sw=+0.038±0.019, consistent with zero, against +0.091±0.019 for the frozen field on the same data, a gap that doubles at Navier--Stokes intermittency. Companion papers prove that this family shows Richardson dispersion and a dissipative anomaly (Fefferman and Mayboroda 2026), and that a scalar advected by this flow obeys Yaglom's relation (De Lellis 2026), at small Kubo number. Trajectories forget their starting point as the smallest eddy is removed: the median separation of pairs released from one point with independent Brownian kicks varies as κ_p^0.0333±0.0038 over 22 decades of particle diffusivity, against κ_p^1/2 for a smooth control. A scalar in the same field closes the exact scale-by-scale variance budget, four independently measured terms balancing the dissipation to 15\% over 1.2 decades with no adjustable constant, and reaches its inertial--convective asymptote S_L=−χr to 0.9995±0.0018 once the measured diffusive transfer is restored, while under an imposed mean gradient χ changes by 14\% over a factor 5.8 in κ.
ER  -