1,551 research outputs found
ANOMALOUS SCALING OF THE PASSIVE SCALAR
We establish anomalous inertial range scaling of structure functions for a
model of advection of a passive scalar by a random velocity field. The velocity
statistics is taken gaussian with decorrelation in time and velocity
differences scaling as in space, with . The
scalar is driven by a gaussian forcing acting on spatial scale and
decorrelated in time. The structure functions for the scalar are well defined
as the diffusivity is taken to zero and acquire anomalous scaling behavior for
large pumping scales . The anomalous exponent is calculated explicitly for
the 4^{\m\rm th} structure function and for small and it differs
from previous predictions. For all but the second structure functions the
anomalous exponents are nonvanishing.Comment: 8 pages, late
Multiscaling in passive scalar advection as stochastic shape dynamics
The Kraichnan rapid advection model is recast as the stochastic dynamics of
tracer trajectories. This framework replaces the random fields with a small set
of stochastic ordinary differential equations. Multiscaling of correlation
functions arises naturally as a consequence of the geometry described by the
evolution of N trajectories. Scaling exponents and scaling structures are
interpreted as excited states of the evolution operator. The trajectories
become nearly deterministic in high dimensions allowing for perturbation theory
in this limit. We calculate perturbatively the anomalous exponent of the third
and fourth order correlation functions. The fourth order result agrees with
previous calculations.Comment: 14 pages, LaTe
Anomalous scaling of a passive scalar advected by the synthetic compressible flow
The field theoretic renormalization group and operator product expansion are
applied to the problem of a passive scalar advected by the Gaussian
nonsolenoidal velocity field with finite correlation time, in the presence of
large-scale anisotropy. The energy spectrum of the velocity in the inertial
range has the form , and the correlation time at
the wavenumber scales as . It is shown that, depending on the
values of the exponents and , the model exhibits various types
of inertial-range scaling regimes with nontrivial anomalous exponents. Explicit
asymptotic expressions for the structure functions and other correlation
functions are obtained; they are represented by superpositions of power laws
with nonuniversal amplitudes and universal (independent of the anisotropy)
anomalous exponents, calculated to the first order in and in
any space dimension. These anomalous exponents are determined by the critical
dimensions of tensor composite operators built of the scalar gradients, and
exhibit a kind of hierarchy related to the degree of anisotropy: the less is
the rank, the less is the dimension and, consequently, the more important is
the contribution to the inertial-range behavior. The leading terms of the even
(odd) structure functions are given by the scalar (vector) operators. The
anomalous exponents depend explicitly on the degree of compressibility.Comment: 25 pages; REVTeX file with LATeX figures insid
Lagrangian acceleration statistics in turbulent flows
We show that the probability densities af accelerations of Lagrangian test
particles in turbulent flows as measured by Bodenschatz et al. [Nature 409,
1017 (2001)] are in excellent agreement with the predictions of a stochastic
model introduced in [C. Beck, PRL 87, 180601 (2001)] if the fluctuating
friction parameter is assumed to be log-normally distributed. In a generalized
statistical mechanics setting, this corresponds to a superstatistics of
log-normal type. We analytically evaluate all hyperflatnes factors for this
model and obtain a flatness prediction in good agreement with the experimental
data. There is also good agreement with DNS data of Gotoh et al. We relate the
model to a generalized Sawford model with fluctuating parameters, and discuss a
possible universality of the small-scale statistics.Comment: 10 pages, 2 figure
2-Dimensional Turbulence: yet another Conformal Field Theory Solution
A new conformal field theory description of two-dimensional turbulence is
proposed. The recently established class of rational logarithmic conformal
field theories provides a unique candidate solution which resolves many of the
drawbacks of former approaches via minimal models. This new model automatically
includes magneto-hydrodynamic turbulence and the Alf'ven effect.Comment: 11 pages, LaTeX (or better LaTeX2e), no figures, also available at
http://www.sns.ias.edu/~flohr/, only the report number and three typos are
correcte
Non-universality of the scaling exponents of a passive scalar convected by a random flow
We consider passive scalar convected by multi-scale random velocity field
with short yet finite temporal correlations. Taking Kraichnan's limit of a
white Gaussian velocity as a zero approximation we develop perturbation theory
with respect to a small correlation time and small non-Gaussianity of the
velocity. We derive the renormalization (due to temporal correlations and
non-Gaussianity) of the operator of turbulent diffusion. That allows us to
calculate the respective corrections to the anomalous scaling exponents of the
scalar field and show that they continuously depend on velocity correlation
time and the degree of non-Gaussianity. The scalar exponents are thus non
universal as was predicted by Shraiman and Siggia on a phenomenological ground
(CRAS {\bf 321}, 279, 1995).Comment: 4 pages, RevTex 3.0, Submitted to Phys.Rev.Let
Passive scalar convection in 2D long-range delta-correlated velocity field: Exact results
The letter presents new field-theoretical approach to 2D passive scalar
problem. The Gaussian form of the distribution for the Lyapunov exponent is
derived and its parameters are found explicitly.Comment: 11 pages, RevTex 3.0, IFUM-94/455/January-F
Anomalous Scaling in a Model of Passive Scalar Advection: Exact Results
Kraichnan's model of passive scalar advection in which the driving velocity
field has fast temporal decorrelation is studied as a case model for
understanding the appearance of anomalous scaling in turbulent systems. We
demonstrate how the techniques of renormalized perturbation theory lead (after
exact resummations) to equations for the statistical quantities that reveal
also non perturbative effects. It is shown that ultraviolet divergences in the
diagrammatic expansion translate into anomalous scaling with the inner length
acting as the renormalization scale. In this paper we compute analytically the
infinite set of anomalous exponents that stem from the ultraviolet divergences.
Notwithstanding, non-perturbative effects furnish a possibility of anomalous
scaling based on the outer renormalization scale. The mechanism for this
intricate behavior is examined and explained in detail. We show that in the
language of L'vov, Procaccia and Fairhall [Phys. Rev. E {\bf 50}, 4684 (1994)]
the problem is ``critical" i.e. the anomalous exponent of the scalar primary
field . This is precisely the condition that allows for
anomalous scaling in the structure functions as well, and we prove that this
anomaly must be based on the outer renormalization scale. Finally, we derive
the scaling laws that were proposed by Kraichnan for this problem, and show
that his scaling exponents are consistent with our theory.Comment: 43 pages, revtex
Burgers Turbulence with Large-scale Forcing
Burgers turbulence supported by white-in-time random forcing at low
wavenumbers is studied analytically and by computer simulation. It is concluded
that the probability density Q of velocity gradient displays four asymptotic
regimes at very large Reynolds number: (A) a region of large positive gradient
where Q decays rapidly (reduction of gradient by stretching); (B) an
intermediate region of negative gradient where Q falls off as the inverse third
power of gradient (transient inviscid steepening of negative gradient); (C) an
outer power-law region of negative gradient where Q falls off as the reciprocal
of gradient (shoulders of mature shocks); (D) a final region of large gradient
where Q decays very rapidly (interior of mature shocks). The probability
density of velocity difference across an interval r, divided by r, lies on Q
throughout regions A and B and into the middle of C, for small enough
inertial-range r.Comment: Revtex (8 pages) with 11 postscript figures (separate file
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