Model Representation for Self - Consistent - Field Theory of Isotropic Turbulence

Similar documents
arxiv: v1 [physics.flu-dyn] 4 Jul 2015

6. Renormalized Perturbation Theory

Energy spectrum of isotropic magnetohydrodynamic turbulence in the Lagrangian renormalized approximation

Small-Scale Statistics and Structure of Turbulence in the Light of High Resolution Direct Numerical Simulation

1. INTRODUCTION A COMMENT ON THE DISTANT INTERACTION ALGORITHM

Effects of Eddy Viscosity on Time Correlations in Large Eddy Simulation

2. Conservation Equations for Turbulent Flows

Energy spectrum in the dissipation range of fluid turbulence

Local shell-to-shell energy transfer via nonlocal interactions in fluid turbulence

An Introduction to Theories of Turbulence. James Glimm Stony Brook University

The infrared properties of the energy spectrum in freely decaying isotropic turbulence

Isotropic homogeneous 3D turbulence

Lagrangian Dynamics & Mixing

Max Planck Institut für Plasmaphysik

A path integral approach to the Langevin equation

A scalar subgrid model with flow structure for large-eddy simulations of scalar variances

On the decay of two-dimensional homogeneous turbulence

Bottlenecks: an interplay of equilibrium statistical mechanics and turbulence

ON THE FLUCTUATION-RESPONSE RELATION IN GEOPHYSICAL SYSTEMS

Capillary-gravity waves: The effect of viscosity on the wave resistance

UNCONDITIONAL STABILITY OF A PARTITIONED IMEX METHOD FOR MAGNETOHYDRODYNAMIC FLOWS

Turbulent Rankine Vortices

Fundamentals of Turbulence

SOME ISSUES OF TURBULENCE

The Kolmogorov Law of turbulence

Energy Transfer and Triadic Interactions in Compressible Turbulence

On the (multi)scale nature of fluid turbulence

Diffusive Transport Enhanced by Thermal Velocity Fluctuations

An evaluation of a conservative fourth order DNS code in turbulent channel flow

The Dissipation Rate Transport Equation and Subgrid-Scale Models in Rotating Turbulence

Spectral reduction for two-dimensional turbulence. Abstract

Turbulence Modeling I!

arxiv: v2 [physics.flu-dyn] 18 Feb 2019

Turbulent drag reduction by streamwise traveling waves

Decaying 2D Turbulence in Bounded Domains: Influence of the Geometry

Lagrangian acceleration in confined 2d turbulent flow

Incompressible MHD simulations

Lecture 14. Turbulent Combustion. We know what a turbulent flow is, when we see it! it is characterized by disorder, vorticity and mixing.

Turbulence: Basic Physics and Engineering Modeling

Fluctuation dynamo amplified by intermittent shear bursts

Isotropic homogeneous 3D turbulence

Kinematic and dynamic pair collision statistics of sedimenting inertial particles relevant to warm rain initiation

arxiv:cond-mat/ v1 [cond-mat.stat-mech] 24 May 2000

The viscous-convective subrange in nonstationary turbulence

F(t) equilibrium under H 0

Modelling of turbulent flows: RANS and LES

A Simple Turbulence Closure Model

- Marine Hydrodynamics. Lecture 4. Knowns Equations # Unknowns # (conservation of mass) (conservation of momentum)

Scale interactions and scaling laws in rotating flows at moderate Rossby numbers and large Reynolds numbers

arxiv: v1 [physics.flu-dyn] 15 Dec 2018

Natalia Tronko S.V.Nazarenko S. Galtier

Topics in Fluid Dynamics: Classical physics and recent mathematics

Mathematical Hydrodynamics

Math 575-Lecture Viscous Newtonian fluid and the Navier-Stokes equations

Probability density function (PDF) methods 1,2 belong to the broader family of statistical approaches

(U c. t)/b (U t)/b

Lecture 2. Turbulent Flow

Energy transfer and dissipation in forced isotropic turbulence

WHITE NOISE APPROACH TO FEYNMAN INTEGRALS. Takeyuki Hida

DIRECT NUMERICAL SIMULATION OF SPATIALLY DEVELOPING TURBULENT BOUNDARY LAYER FOR SKIN FRICTION DRAG REDUCTION BY WALL SURFACE-HEATING OR COOLING

On modeling pressure diusion. in non-homogeneous shear ows. By A. O. Demuren, 1 M. M. Rogers, 2 P. Durbin 3 AND S. K. Lele 3

Contribution of Reynolds stress distribution to the skin friction in wall-bounded flows

Some remarks on grad-div stabilization of incompressible flow simulations

STRESS TRANSPORT MODELLING 2

Coupled systems of two-dimensional turbulence

CVS filtering to study turbulent mixing

On Decaying Two-Dimensional Turbulence in a Circular Container

The decay of axisymmetric omogeneous turbulence

arxiv:cond-mat/ v3 [cond-mat.stat-mech] 2 Feb 2005

Simulations of Three-Dimensional Turbulent Mixing for Schmidt Numbers of the Order 1000

arxiv:cond-mat/ v2 [cond-mat.stat-mech] 22 Jan 1998

Turbulence models of gravitational clustering

A Hydrodynamic Interpretation of Quantum Mechanics via Turbulence

The Kraichnan Kazantsev Dynamo

M.A. Aziz, M.A.K. Azad and M.S. Alam Sarker Department of Applied Mathematics, University of Rajshahi-6205, Bangladesh

Ensemble averaged dynamic modeling. By D. Carati 1,A.Wray 2 AND W. Cabot 3

A Momentum Exchange-based Immersed Boundary-Lattice. Boltzmann Method for Fluid Structure Interaction

Energy dissipation caused by boundary layer instability at vanishing viscosity

CHAPTER V. Brownian motion. V.1 Langevin dynamics

Project Topic. Simulation of turbulent flow laden with finite-size particles using LBM. Leila Jahanshaloo

TURBULENCE IN FLUIDS AND SPACE PLASMAS. Amitava Bhattacharjee Princeton Plasma Physics Laboratory, Princeton University

Eddy-diffusivity fields in turbulent transport: explicit expressions

A Simple Turbulence Closure Model. Atmospheric Sciences 6150

Stability of Shear Flow

Lecture 4: The Navier-Stokes Equations: Turbulence

Weak Turbulence of Gravity Waves

Nonequilibrium Dynamics in Astrophysics and Material Science YITP, Kyoto

Brownian Motion and Langevin Equations

Institute for Computer Applications in Science and Engineering. NASA Langley Research Center, Hampton, VA 23681, USA. Jean-Pierre Bertoglio

Lifshitz Hydrodynamics

O. A Survey of Critical Experiments

Statistical studies of turbulent flows: self-similarity, intermittency, and structure visualization

LES of Turbulent Flows: Lecture 3

Satyajit Barman, Anando G. Chatterjee, 1, e) Ravi Samtaney, 2, f) 3, 4, g)

The Truth about diffusion (in liquids)

Energy dissipating structures generated by dipole-wall collisions at high Reynolds number

Defense Technical Information Center Compilation Part Notice

Direct Numerical Simulation of fractal-generated turbulence

Characteristics of Linearly-Forced Scalar Mixing in Homogeneous, Isotropic Turbulence

Note the diverse scales of eddy motion and self-similar appearance at different lengthscales of the turbulence in this water jet. Only eddies of size

Transcription:

arxiv:cond-mat/41227v1 [cond-mat.stat-mech] 14 Jan 24 Model Representation for Self - Consistent - Field Theory of Isotropic Turbulence R. V. R. Pandya Department of Mechanical Engineering University of Puerto Rico at Mayaguez Mayaguez, Puerto Rico, PR 681, USA January 24, 217 Abstract In this paper, Langevin model equation is proposed for Fourier modes of velocity field of isotropic turbulence whose statistical properties are identical to those governed by equations of Self-Consistent-Field (SCF) theory of turbulence [J. R. Herring, Physics of Fluids 9, 216 (1966)]. 1 Introduction Kraichnan s seminal and pioneering work on Direct Interaction Approximation (DIA) ([Kraichnan(1958)], [Kraichnan(1959)]) and Lagrangian History Direct Interaction Approximation (LHDIA) ([Kraichnan(1965)]) has been influential in setting the right tone in the field of theory of turbulence and leading to other fundamental renormalized approaches for turbulence closure ([Edwards(1964)], [Herring(1965), Herring(1966)], [McComb(1978)], [Kaneda(1981)], [L vov(1991)]). Various renormalized approaches are critically reviewed by[leslie(1973)],[mccomb(199)],[mccomb(1995)],[l vov(1991)], and[lesieur(1997)]. And the Self-Consistent-Field (SCF) approach of[herring(1966)] having close relationship with DIA ([Herring & Kraichnan(1972)]) is the central focus in this paper. 1

[Herring(1965)] developed the SCF approach for stationary isotropic turbulence and subsequently generalized to the non-stationary isotropic turbulence ([Herring(1966)]). Instead of applying the perturbation technique to the Navier-Stokes equations, following [Edwards(1964)] framework, Herring preferred Livouville equation for probability distribution function of Fourier modes of the velocity field. Then, a self-consistentfield procedure was carried out around the zeroth order probability distribution which is the product of exact single mode distribution. This led [Herring(1966)] to derive equations governing time evolutions of Green s function, single-time velocity correlation and two-time velocity correlation. Yet another method of[balescu & Senatorski(197)] yielded the SCF set of equations and thus doubly justified these equations. The equations for Green s function and single-time velocity correlation are identical in form to the corresponding DIA s equations and generalized fluctuation-dissipation relation represents the equation for two-time velocity correlation in the SCF approach. Despite being closer to Edwards s theory framework and closer to DIA in terms of the final equations, well justified SCF approach lacks a model representation. Whereas model representations are known to exist for DIA ([Kraichnan(197)]) and extended Edwards s theory ([Kraichnan(1971)]) associated with the non-stationary turbulence. Also, model representations are available for Kaneda s theory ([Kaneda(1981)]) and [McComb(1978)] local energy transfer (LET) theory ([Pandya(24)]). The model representation, if exists, assures the fact that statistical properties predicted by SCF are those of a realizable velocity field and consequently establishes certain consistency properties. The purpose of this paper is to suggest an existence of Langevin model representation for SCF. Consequently, to make sure that SCF does not lag behind other theories when judged from the perspective of realizability and model representation. 2 SCF theory equations In this section, closed set of equations describing the statistical properties of isotropic turbulence as obtained by SCF approach of [Herring(1966)] are presented. I should be excused for not using the original notations of Herring, rather using the notations of [McComb(199)] while presenting SCF equations. The Fourier modes u i (k,t) defined by u i (x,t) = d 3 ku i (k,t)exp(ik x), (1) 2

of the velocity field u i (x,t) of homogeneous, isotropic, incompressible fluid turbulence in space-time (x t) domain satisfy the following Navier-Stokes equation written in Fourier wavevector (k) and time domain: ( t +νk2 )u i (k,t) = M ijm (k) Here ν is kinematic viscosity of fluid, inertial transfer operator d 3 pu j (p,t)u m (k p,t). (2) M ijm (k) = (2i) 1 [k j P im (k)+k m P ij (k)], (3) the projector P ij (k) = δ ij k i k j k 2, k = k, and δ ij is the Kronecker delta. The subscripts take the values 1, 2 or 3 alongwith the usual summation convention over repeatedsubscript. Thetwo-timevelocitycorrelationQ in (k,k ;t,t ) = u i (k,t)u n (k,t ), single-time velocity correlation Q in (k,k ;t,t) = u i (k,t)u n (k,t) of the velocity field u i (k,t)andthegreen sfunctiong in (k;t,t )canbesimplified forisotropicturbulence, and written as Q in (k,k ;t,t ) = P in (k)q(k;t,t )δ(k+k ), (4) and Q in (k,k ;t,t) = P in (k)q(k;t,t)δ(k+k ), (5) G in (k;t,t ) = P in (k)g(k;t,t ), (6) where represents ensemble average and δ represents Dirac delta function. The SCF equation for G(k;t,t ) may be written as ( ) t +νk2 G(k;t,t )+ d 3 pl(k,p) dsg(p;t,s)q( k p ;t,s)g(k;s,t ) = t > t t and G(k;t,t ) = 1. The SCF equation for Q(k;t,t) may be written as ( ) t +2νk2 Q(k;t,t)+2 where = 2 d 3 pl(k,p) d 3 pl(k,p) dsg(p;t,s)q( k p ;t,s)q(k;t,s) (7) dsg(k;t,s)q( k p ;t,s)q(p;t,s) (8) L(k,p) = [µ(k2 +p 2 ) kp(1+2µ 2 )](1 µ 2 )kp k 2 +p 2 2kpµ (9) 3

and µ is the cosine of the angle between the vectors k and p. These equations (7) and (8) have form identical to the corresponding equations obtained by DIA theory. In SCF approach, the equation for Q(k;t,t ) is associated with generalized fluctuationdissipation relation Q(k;t,t ) = G(k;t,t )Q(k;t,t ), t t. (1) We write the equation for Q(k;t,t ), by using equations (7) and (1), in the following form convenient for further use: ( ) t +νk2 Q(k;t,t )+ d 3 pl(k,p) dsg(p;t,s)q( k p ;t,s)q(k;s,t ) = d 3 pl(k,p) dsg(p;t,s)q( k p ;t,s)q(k;s,t ). (11) Thus equations (7), (8) and (11) form a closed set of final equations of SCF approach of [Herring(1966)]. Now the goal is to obtain model equation for u i (k,t) which would have statistical properties identical to those as predicted by this closed set of equations. And a Langevin equation as a model representation for SCF is presented in the section to follow. 3 Langevin model equation for SCF Similar to Langevin model representation for DIA, consider a Langevin equation for u i (k,t) written as ( ) t +νk2 u i (k,t)+ dsη(k;t,s)u i (k,s) = f i (k,t)+b i (k,t) (12) where η(k;t,s) is statistically sharp damping function, f i (k,t) is a forcing term with zero mean and b i (k,t) is white noise forcing term having zero mean. It should be noted that b i (k,t) is an additional new forcing term that is not present in DIA s Langevin model representation. We consider these two different forcing terms to be statistically independent f i (k,t)b n (k,t ) = k,t (13) 4

and their statistical properties for isotropic turbulence,written as and f i (k,t)f n (k,t ) = P in (k)f(k,t,t )δ(k+k ) (14) b i (k,t)b n (k,t ) = P in (k)b(k,t)δ(k+k )δ(t t ). (15) For particular choice of η(k;t,s), F(k,t,t ) and B(k,t), the Langevin equation (12) would recover the closed set of SCF equations (7), (8) and (11). Now we obtain that particular choice. For isotropic turbulence, the Green s function of the Langevin equation (12) satisfies ( ) t t +νk2 G(k;t,t )+ dsη(k;t,s)g(k;s,t ) = t > t (16) t and G(k;t,t ) = 1. The expression for η given by η(k;t,s) = d 3 pl(k,p)g(p;t,s)q( k p ;t,s) (17) would make equation (16) identical to SCF equation (7) for the Green s function. To obtain F(k,t,s) we compare equation (11) with the equation for Q(k;t,t ) obtained from Langevin equation (12), written as ( ) t t +νk2 Q(k;t,t )+ dsη(k;t,s)q(k;s,t ) = dsg(k;t,s)f(k,t,s). (18) While writing this equation we have made use of equations (13)-(15). On comparison and making use of expression for η and generalized fluctuation-dissipation relation (1), we obtain F(k,t,s) = η(k;t,s)q(k;s,s) (19) whichwouldmake(18)identicaltoscfequation(11)forq(k;t,t ). Nowtheequation for Q(k;t,t) as obtained from the Langevin equation (12) and using equations (13)- (15) can be written as ( ) t t +2νk2 Q(k;t,t)+2 dsη(k;t,s)q(k;t,s) = 2 dsg(k;t,s)f(k,t,s)+b(k,t). (2) 5

Comparison of this equation with SCF equation (8) for Q(k;t,t), making use of expressions for η(k;t,s), F(k,t,s) given by equations (17) and (19) respectively and using equation (1) we obtain B(k,t) = 2 d 3 pl(k,p) dsg(k;t,s)q( k p ;t,s)q(p;t,s) 2 dsη(k;t,s)q(k;t,s) (21) which makes equation (2) identical to equation (8). Thus, the Langevin equation (12) along with the expression for η given by (17) and statistical properties of the two forcing functions F(k,t,s) and B(k,t) given by (19) and (21) respectively, is the required model representation for SCF approach of [Herring(1966)]. 4 Concluding remarks A long awaited model representation for self-consistent-field approach of[herring(1966)] has been suggested in this paper. This model is in the form of a Langevin equation having two statistically independent forcing terms in contrary to one forcing term present in DIA s Langevin model representation. The proposed model assures that the closed set of equations of SCF approach generates statistical properties of the velocity field that is realizable. It should be noted that the expression for η(k;t,s) is identical to that present in DIA s Langevin model representation ([Kraichnan(197)]). It is worth mentioning here the reason for different type of model representations for SCF approach, LET theory and extended Edwards s theory despite the fact that the generalized fluctuation-dissipation relation is central to all of them. The SCF approach has been modelled here by Langevin equation whereas LET and extended Edwards s theories have an almost-markovian model representations([pandya(24)], [Kraichnan(1971)]). This difference is mainly due to an additional condition for Green s function i.e. G(k;t,t ) = G(k;t,s)G(k;s,t ) which is the property of only LET and extended Edwards s theories and is satisfied by an almost-markovian equation and not satisfied by the Langevin equation and SCF approach. Acknowledgement I acknowledge the financial support provided by the University of Puerto Rico at Mayaguez, Puerto Rico, USA. 6

References [Balescu & Senatorski(197)] Balescu, R. & Senatorski, A. 197 A new approach to the theory of fully developed turbulence. Ann. Phys. 58, 587 624. [Edwards(1964)] Edwards, S. F. 1964 The statistical dynamics of homogeneous turbulence. J. Fluid Mech. 18, 239 273. [Herring(1965)] Herring, J. R. 1965 Self-consistent-field approach to turbulence theory. Phys. Fluids 8, 2219 2225. [Herring(1966)] Herring, J. R. 1966 Self-consistent-field approach to nonstationary turbulence. Phys. Fluids 9, 216 211. [Herring & Kraichnan(1972)] Herring, J. R. & Kraichnan, R. H. 1972 Comparison of some approximamtions for isotropic turbulence. In Lecture Notes in Physics, Vol. 12, Statistical Models and Turbulence. Springer, Berlin. [Kaneda(1981)] Kaneda, Y. 1981 Renormalized expansions in the theory of turbulence with the use of the Lagrangian position function. J. Fluid Mech. 17, 131 145. [Kraichnan(1958)] Kraichnan, R. H. 1958 Irreversible statistical mechanics of incompressible hydromagnetic turbulence. Phys. Rev. 19, 147 1422. [Kraichnan(1959)] Kraichnan, R. H. 1959 The structure of isotropic turbulence at very high Reynolds numbers. J. Fluid Mech. 5, 497 543. [Kraichnan(1965)] Kraichnan, R. H. 1965 Lagrangian-history closure approximation for turbulence. Phys. Fluids 8, 575 598. [Kraichnan(197)] Kraichnan, R. H. 197 Convergents to turbulence functions. J. Fluid Mech. 41, 189 217. [Kraichnan(1971)] Kraichnan, R. H. 1971 An almost-markovian Galileaninvariant turbulence model. J. Fluid Mech. 47, 513 524. [Lesieur(1997)] Lesieur, M. 1997 Turbulence in Fluids, 3rd edn. Dordrecht: Kluwer. [Leslie(1973)] Leslie, D. C. 1973 Developments in the Theory of Turbulence. Oxford: Clarendon Press. 7

[L vov(1991)] L vov, V. S. 1991 Scale invariant-theory of fully-developed hydrodynamic turbulence - Hamiltonian approach. Phys. Rep. 27, 1 47. [McComb(1978)] McComb, W. D. 1978 A theory of time-dependent isotropic turbulence. J. Phys. A 11, 613 632. [McComb(199)] McComb, W. D. 199 The Physics of Fluid Turbulence. New York, NY: Oxford University Press. [McComb(1995)] McComb, W. D. 1995 Theory of turbulence. Rep. Prog. Phys. 58, 1117 126. [Pandya(24)] Pandya, R. V. R. 24 Model representation for local energy transfer theory of isotropic turbulence. Submitted to Journal of Fluid Mechanics. 8