360 research outputs found

    On how a joint interaction of two innocent partners (smooth advection & linear damping) produces a strong intermittency

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    Forced advection of passive scalar by a smooth dd-dimensional incompressible velocity in the presence of a linear damping is studied. Acting separately advection and dumping do not lead to an essential intermittency of the steady scalar statistics, while being mixed together produce a very strong non-Gaussianity in the convective range: qq-th (positive) moment of the absolute value of scalar difference, is proportional to rξqr^{\xi_{q}}, ξq=d2/4+αdq/[(d1)D]d/2\xi _{q}=\sqrt{d^{2}/4+\alpha dq/[ (d-1)D]}-d/2, where α/D\alpha /D measures the rate of the damping in the units of the stretching rate. Probability density function (PDF) of the scalar difference is also found.Comment: 4 pages, RevTex, Submitted to Phys. Fluid

    Statistical geometry in scalar turbulence

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    A general link between geometry and intermittency in passive scalar turbulence is established. Intermittency is qualitatively traced back to events where tracer particles stay for anomalousy long times in degenerate geometries characterized by strong clustering. The quantitative counterpart is the existence of special functions of particle configurations which are statistically invariant under the flow. These are the statistical integrals of motion controlling the scalar statistics at small scales and responsible for the breaking of scale invariance associated to intermittency.Comment: 4 pages, 5 figure

    Non-universality of the scaling exponents of a passive scalar convected by a random flow

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    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

    Dynamics of Fluctuation Dominated Phase Ordering: Hard-core Passive Sliders on a Fluctuating Surface

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    We study the dynamics of a system of hard-core particles sliding downwards on a one dimensional fluctuating interface, which in a special case can be mapped to the problem of a passive scalar advected by a Burgers fluid. Driven by the surface fluctuations, the particles show a tendency to cluster, but the hard-core interaction prevents collapse. We use numerical simulations to measure the auto-correlation function in steady state and in the aging regime, and space-time correlation functions in steady state. We have also calculated these quantities analytically in a related surface model. The steady state auto-correlation is a scaling function of t/L^z, where L is the system size and z the dynamic exponent. Starting from a finite intercept, the scaling function decays with a cusp, in the small argument limit. The finite value of the intercept indicates the existence of long range order in the system. The space-time correlation, which is a function of r/L and t/L^z, is non-monotonic in t for fixed r. The aging auto-correlation is a scaling function of t_1 and t_2 where t_1 is the waiting time and t_2 the time difference. This scaling function decays as a power law for t_2 \gg t_1; for t_1 \gg t_2, it decays with a cusp as in steady state. To reconcile the occurrence of strong fluctuations in the steady state with the fact of an ordered state, we measured the distribution function of the length of the largest cluster. This shows that fluctuations never destroy ordering, but rather the system meanders from one ordered configuration to another on a relatively rapid time scale

    The intermittent behavior and hierarchical clustering of the cosmic mass field

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    The hierarchical clustering model of the cosmic mass field is examined in the context of intermittency. We show that the mass field satisfying the correlation hierarchy ξnQn(ξ2)n1\xi_n\simeq Q_n(\xi_2)^{n-1} is intermittent if κ<d\kappa < d, where dd is the dimension of the field, and κ\kappa is the power-law index of the non-linear power spectrum in the discrete wavelet transform (DWT) representation. We also find that a field with singular clustering can be described by hierarchical clustering models with scale-dependent coefficients QnQ_n and that this scale-dependence is completely determined by the intermittent exponent and κ\kappa. Moreover, the singular exponents of a field can be calculated by the asymptotic behavior of QnQ_n when nn is large. Applying this result to the transmitted flux of HS1700 Lyα\alpha forests, we find that the underlying mass field of the Lyα\alpha forests is significantly intermittent. On physical scales less than about 2.0 h1^{-1} Mpc, the observed intermittent behavior is qualitatively different from the prediction of the hierarchical clustering with constant QnQ_n. The observations, however, do show the existence of an asymptotic value for the singular exponents. Therefore, the mass field can be described by the hierarchical clustering model with scale-dependent QnQ_n. The singular exponent indicates that the cosmic mass field at redshift 2\sim 2 is weakly singular at least on physical scales as small as 10 h1^{-1} kpc.Comment: AAS Latex file, 33 pages,5 figures included, accepted for publication in Ap

    Dynamics of a passive sliding particle on a randomly fluctuating surface

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    We study the motion of a particle sliding under the action of an external field on a stochastically fluctuating one-dimensional Edwards-Wilkinson surface. Numerical simulations using the single-step model shows that the mean-square displacement of the sliding particle shows distinct dynamic scaling behavior, depending on whether the surface fluctuates faster or slower than the motion of the particle. When the surface fluctuations occur on a time scale much smaller than the particle motion, we find that the characteristic length scale shows anomalous diffusion with ξ(t)t2ϕ\xi(t)\sim t^{2\phi}, where ϕ0.67\phi\approx 0.67 from numerical data. On the other hand, when the particle moves faster than the surface, its dynamics is controlled by the surface fluctuations and ξ(t)t1/2\xi(t)\sim t^{{1/2}}. A self-consistent approximation predicts that the anomalous diffusion exponent is ϕ=2/3\phi={2/3}, in good agreement with simulation results. We also discuss the possibility of a slow cross-over towards asymptotic diffusive behavior. The probability distribution of the displacement has a Gaussian form in both the cases.Comment: 6 pages, 4 figures, error in reference corrected and new reference added, submitted to Phys. Rev.

    Universal decay of scalar turbulence

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    The asymptotic decay of passive scalar fields is solved analytically for the Kraichnan model, where the velocity has a short correlation time. At long times, two universality classes are found, both characterized by a distribution of the scalar -- generally non-Gaussian -- with global self-similar evolution in time. Analogous behavior is found numerically with a more realistic flow resulting from an inverse energy cascade.Comment: 4 pages, 3 Postscript figures, submitted to PR

    Quantum Critical Scaling in a Moderately Doped Antiferromagnet

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    Using high temperature expansions for the equal time correlator S(q)S(q) and static susceptibility χ(q)\chi(q) for the t-J model, we present evidence for quantum critical (QC), z ⁣= ⁣1z\!=\!1, behavior at intermediate temperatures in a broad range of t/Jt/J ratio, doping, and temperatures. We find that the dynamical susceptibility is very close to the universal scaling function computable for the asymptotic QC regime, and that the dominant energy scale is temperature. Our results are in excellent agreement with measurements of the spin-echo decay rate, 1/T2G1/T_{\rm 2G}, in La2_2CuO4_4, and provide qualitative understanding of both 1/T11/T_1 and 1/T2G1/T_{\rm 2G} nuclear relaxation rates in doped cuprates.Comment: 11 pages, REVTeX v3.0, PostScript file for 3 figures is attached, UIUC-P-93-07-068. In this revised version, we calculate the scaling functions and thus present new and more direct evidence in favor of our original conclusion

    Generalized CP^1 model from t_1-t_2-J model

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    A long-wavelength, low-frequency effective theory is obtained from t1t2Jt_1-t_2-J model. The action is written in terms of two-component bose spinor fields (CP^1 fields) and two spinless Fermi fields. The generalized CP^1 model is invariant under U(1) gauge transformations. The bose fields and one of the Fermi fields have charge +1 while the other Fermi field has charge -1 with respect to these transformations. A simple mean-feild theory of a gauge-symmerty breaking, based on a four-fermion interaction, is discussed. An effective theory of frustrated antiferromagnetism is obtained integrating out the Fermi fields around the mean-fields. Another option is used to parametrize the long distance fluctuations in t1t2Jt_1-t_2-J model, with the help of gauge invariant fields. It is argued that the resulting Fermi quasiparticles of the t1t2Jt_1-t_2-J model have both charge and spin. The effective action is rewritten in terms of spin 1/2 Fermi spinor, which has the charge of the holes, and unit vector.Comment: 22 pages, RevTex, no figure

    Spatiotemporal Chaos, Localized Structures and Synchronization in the Vector Complex Ginzburg-Landau Equation

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    We study the spatiotemporal dynamics, in one and two spatial dimensions, of two complex fields which are the two components of a vector field satisfying a vector form of the complex Ginzburg-Landau equation. We find synchronization and generalized synchronization of the spatiotemporally chaotic dynamics. The two kinds of synchronization can coexist simultaneously in different regions of the space, and they are mediated by localized structures. A quantitative characterization of the degree of synchronization is given in terms of mutual information measures.Comment: 6 pages, using bifchaos.sty (included). 7 figures. Related material, including higher quality figures, could be found at http://www.imedea.uib.es/PhysDept/publicationsDB/date.html . To appear in International Journal of Bifurcation and Chaos (1999
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