Turbulence with pressure: Anomalous scaling of a passive vector field

N. V. Antonov, Michal Hnatich, Juha Honkonen, and Marian Jurčišin
Phys. Rev. E 68, 046306 – Published 27 October 2003
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Abstract

The field theoretic renormalization group (RG) and the operator-product expansion are applied to the model of a transverse (divergence-free) vector quantity, passively advected by the “synthetic” turbulent flow with a finite (and not small) correlation time. The vector field is described by the stochastic advection-diffusion equation with the most general form of the inertial nonlinearity; it contains as special cases the kinematic dynamo model, linearized Navier-Stokes (NS) equation, the special model without the stretching term that possesses additional symmetries and has a close formal resemblance with the stochastic NS equation. The statistics of the advecting velocity field is Gaussian, with the energy spectrum E(k)k1ɛ and the dispersion law ωk2+η, k being the momentum (wave number). The inertial-range behavior of the model is described by seven regimes (or universality classes) that correspond to nontrivial fixed points of the RG equations and exhibit anomalous scaling. The corresponding anomalous exponents are associated with the critical dimensions of tensor composite operators built solely of the passive vector field, which allows one to construct a regular perturbation expansion in ɛ and η; the actual calculation is performed to the first order (one-loop approximation), including the anisotropic sectors. Universality of the exponents, their (in)dependence on the forcing, effects of the large-scale anisotropy, compressibility, and pressure are discussed. In particular, for all the scaling regimes the exponents obey a hierarchy related to the degree of anisotropy: the more anisotropic is the contribution of a composite operator to a correlation function, the faster it decays in the inertial range. The relevance of these results for the real developed turbulence described by the stochastic NS equation is discussed.

  • Received 16 May 2003

DOI:https://doi.org/10.1103/PhysRevE.68.046306

©2003 American Physical Society

Authors & Affiliations

N. V. Antonov1, Michal Hnatich2, Juha Honkonen3, and Marian Jurčišin2,4

  • 1Department of Theoretical Physics, St. Petersburg University, Uljanovskaja 1, St. Petersburg, Petrodvorez 198504, Russia
  • 2Institute of Experimental Physics, Slovak Academy of Sciences, Watsonova 47, 04011 Košice, Slovakia
  • 3Department of Physical Sciences, Theoretical Physics Division, P.O. Box 64 (Gustaf Hällströmin katu 2), FIN-00014 University of Helsinki, Helsinki, Finland
  • 4N.N. Bogoliubov Laboratory of Theoretical Physics, Joint Institute for Nuclear Research, 141980 Dubna, Moscow Region, Russia

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Vol. 68, Iss. 4 — October 2003

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