189 research outputs found

    The Scaling Structure of the Velocity Statistics in Atmospheric Boundary Layer

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    The statistical objects characterizing turbulence in real turbulent flows differ from those of the ideal homogeneous isotropic model.They containcontributions from various 2d and 3d aspects, and from the superposition ofinhomogeneous and anisotropic contributions. We employ the recently introduceddecomposition of statistical tensor objects into irreducible representations of theSO(3) symmetry group (characterized by jj and mm indices), to disentangle someof these contributions, separating the universal and the asymptotic from the specific aspects of the flow. The different jj contributions transform differently under rotations and so form a complete basis in which to represent the tensor objects under study. The experimental data arerecorded with hot-wire probes placed at various heights in the atmospheric surfacelayer. Time series data from single probes and from pairs of probes are analyzed to compute the amplitudes and exponents of different contributions to the second order statistical objects characterized by j=0j=0, j=1j=1 and j=2j=2. The analysis shows the need to make a careful distinction between long-lived quasi 2d turbulent motions (close to the ground) and relatively short-lived 3d motions. We demonstrate that the leading scaling exponents in the three leading sectors (j=0,1,2j = 0, 1, 2) appear to be different butuniversal, independent of the positions of the probe, and the large scaleproperties. The measured values of the exponent are ζ2(j=0)=0.68±0.01\zeta^{(j=0)}_2=0.68 \pm 0.01, ζ2(j=1)=1.0±0.15\zeta^{(j=1)}_2=1.0\pm 0.15 and ζ2(j=2)=1.38±0.10\zeta^{(j=2)}_2=1.38 \pm 0.10. We present theoretical arguments for the values of these exponents usingthe Clebsch representation of the Euler equations; neglecting anomalous corrections, the values obtained are 2/3, 1 and 4/3 respectively.Comment: PRE, submitted. RevTex, 38 pages, 8 figures included . Online (HTML) version of this paper is avaliable at http://lvov.weizmann.ac.il

    Statistical Description of Acoustic Turbulence

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    We develop expressions for the nonlinear wave damping and frequency correction of a field of random, spatially homogeneous, acoustic waves. The implications for the nature of the equilibrium spectral energy distribution are discussedComment: PRE, Submitted. REVTeX, 16 pages, 3 figures (not included) PS Source of the paper with figures avalable at http://lvov.weizmann.ac.il/onlinelist.htm

    Electrical Detection and Magnetic-Field Control of Spin States in Phosphorus-Doped Silicon

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    Electron paramagnetic resonance of ensembles of phosphorus donors in silicon has been detected electrically with externally applied magnetic fields lower than 200 G. Because the spin Hamiltonian was dominated by the contact hyperfine term rather than by the Zeeman terms at such low magnetic fields, superposition states α∣↑↓>+β∣↓↑> \alpha{}| \uparrow \downarrow >+\beta{}| \downarrow \uparrow > and −β∣↑↓>+α∣↓↑>-\beta{}| \uparrow \downarrow > + \alpha{}| \downarrow \uparrow > were formed between phosphorus electron and nuclear spins, and electron paramagnetic resonance transitions between these superposition states and ∣↑↑>| \uparrow \uparrow > or ∣↓↓>| \downarrow \downarrow > states are observed clearly. A continuous change of α\alpha{} and β\beta{} with the magnetic field was observed with a behavior fully consistent with theory of phosphorus donors in silicon.Comment: 6 pages, 5 figure

    Parametric generation of second sound in superfluid helium: linear stability and nonlinear dynamics

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    We report the experimental studies of a parametric excitation of a second sound (SS) by a first sound (FS) in a superfluid helium in a resonance cavity. The results on several topics in this system are presented: (i) The linear properties of the instability, namely, the threshold, its temperature and geometrical dependencies, and the spectra of SS just above the onset were measured. They were found to be in a good quantitative agreement with the theory. (ii) It was shown that the mechanism of SS amplitude saturation is due to the nonlinear attenuation of SS via three wave interactions between the SS waves. Strong low frequency amplitude fluctuations of SS above the threshold were observed. The spectra of these fluctuations had a universal shape with exponentially decaying tails. Furthermore, the spectral width grew continuously with the FS amplitude. The role of three and four wave interactions are discussed with respect to the nonlinear SS behavior. The first evidence of Gaussian statistics of the wave amplitudes for the parametrically generated wave ensemble was obtained. (iii) The experiments on simultaneous pumping of the FS and independent SS waves revealed new effects. Below the instability threshold, the SS phase conjugation as a result of three-wave interactions between the FS and SS waves was observed. Above the threshold two new effects were found: a giant amplification of the SS wave intensity and strong resonance oscillations of the SS wave amplitude as a function of the FS amplitude. Qualitative explanations of these effects are suggested.Comment: 73 pages, 23 figures. to appear in Phys. Rev. B, July 1 st (2001

    Exact Resummations in the Theory of Hydrodynamic Turbulence: II A Ladder to Anomalous Scaling

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    In paper I of this series on fluid turbulence we showed that exact resummations of the perturbative theory of the structure functions of velocity differences result in a finite (order by order) theory. These findings exclude any known perturbative mechanism for anomalous scaling of the velocity structure functions. In this paper we continue to build the theory of turbulence and commence the analysis of nonperturbative effects that form the analytic basis of anomalous scaling. Starting from the Navier-Stokes equations (at high Reynolds number Re) we discuss the simplest examples of the appearance of anomalous exponents in fluid mechanics. These examples are the nonlinear (four-point) Green's function and related quantities. We show that the renormalized perturbation theory for these functions contains ``ladder`` diagrams with (convergent!) logarithmic terms that sum up to anomalous exponents. Using a new sum rule which is derived here we calculate the leading anomalous exponent and show that it is critical in a sense made precise below. This result opens up the possibility of multiscaling of the structure functions with the outer scale of turbulence as the renormalization length. This possibility will be discussed in detail in the concluding paper III of this series.Comment: PRE in press, 15 pages + 21 figures, REVTeX, The Eps files of figures will be FTPed by request to [email protected]

    Recent Developments in Understanding Two-dimensional Turbulence and the Nastrom-Gage Spectrum

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    Two-dimensional turbulence appears to be a more formidable problem than three-dimensional turbulence despite the numerical advantage of working with one less dimension. In the present paper we review recent numerical investigations of the phenomenology of two-dimensional turbulence as well as recent theoretical breakthroughs by various leading researchers. We also review efforts to reconcile the observed energy spectrum of the atmosphere (the spectrum) with the predictions of two-dimensional turbulence and quasi-geostrophic turbulence.Comment: Invited review; accepted by J. Low Temp. Phys.; Proceedings for Warwick Turbulence Symposium Workshop on Universal features in turbulence: from quantum to cosmological scales, 200

    Far-off-resonant wave interaction in one-dimensional photonic crystals with quadratic nonlinearity

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    We extend a recently developed Hamiltonian formalism for nonlinear wave interaction processes in spatially periodic dielectric structures to the far-off-resonant regime, and investigate numerically the three-wave resonance conditions in a one-dimensional optical medium with χ(2)\chi^{(2)} nonlinearity. In particular, we demonstrate that the cascading of nonresonant wave interaction processes generates an effective χ(3)\chi^{(3)} nonlinear response in these systems. We obtain the corresponding coupling coefficients through appropriate normal form transformations that formally lead to the Zakharov equation for spatially periodic optical media.Comment: 14 pages, 4 figure

    Pion Generalized Dipole Polarizabilities by Virtual Compton Scattering πe→πeγ\pi e \to \pi e\gamma

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    We present a calculation of the cross section and the event generator of the reaction πe→πeγ\pi e\to \pi e \gamma. This reaction is sensitive to the pion generalized dipole polarizabilities, namely, the longitudinal electric αL(q2)\alpha_L(q^2), the transverse electric αT(q2)\alpha_T(q^2), and the magnetic β(q2)\beta(q^2) which, in the real-photon limit, reduce to the ordinary electric and magnetic polarizabilities αˉ\bar{\alpha} and βˉ\bar{\beta}, respectively. The calculation of the cross section is done in the framework of chiral perturbation theory at O(p4){\cal O}(p^4). A pion VCS event generator has been written which is ready for implementation in GEANT simulation codes or for independent use.Comment: 33 pages, Revtex, 15 figure

    Predictive powers of chiral perturbation theory in Compton scattering off protons

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    We study low-energy nucleon Compton scattering in the framework of baryon chiral perturbation theory (Bχ\chiPT) with pion, nucleon, and Δ\Delta(1232) degrees of freedom, up to and including the next-to-next-to-leading order (NNLO). We include the effects of order p2p^2, p3p^3 and p4/Δp^4/\varDelta, with Δ≈300\varDelta\approx 300 MeV the Δ\Delta-resonance excitation energy. These are all "predictive" powers in the sense that no unknown low-energy constants enter until at least one order higher (i.e, p4p^4). Estimating the theoretical uncertainty on the basis of natural size for p4p^4 effects, we find that uncertainty of such a NNLO result is comparable to the uncertainty of the present experimental data for low-energy Compton scattering. We find an excellent agreement with the experimental cross section data up to at least the pion-production threshold. Nevertheless, for the proton's magnetic polarizability we obtain a value of (4.0±0.7)×10−4(4.0\pm 0.7)\times 10^{-4} fm3^3, in significant disagreement with the current PDG value. Unlike the previous χ\chiPT studies of Compton scattering, we perform the calculations in a manifestly Lorentz-covariant fashion, refraining from the heavy-baryon (HB) expansion. The difference between the lowest order HBχ\chiPT and Bχ\chiPT results for polarizabilities is found to be appreciable. We discuss the chiral behavior of proton polarizabilities in both HBχ\chiPT and Bχ\chiPT with the hope to confront it with lattice QCD calculations in a near future. In studying some of the polarized observables, we identify the regime where their naive low-energy expansion begins to break down, thus addressing the forthcoming precision measurements at the HIGS facility.Comment: 24 pages, 9 figures, RevTeX4, revised version published in EPJ
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