Research Journal of Applied Sciences, Engineering and Technology 4(20): 4150-4159, 2012 ISSN: 2040-7467 © Maxwell Scientific Organization, 2012 Submitted: April 23, 2012 Accepted: May 23 , 2012 Published: October 15, 2012 Transport Equation for the Joint Distribution Function of Velocity, Temperature and Concentration in Convective Turbulent Flow in Presence of Dust Particles M.A.K. Azad, M.H.U. Molla and M.Z. Rahman Department of Applied Mathematics, University of Rajshahi, Rajshahi-6205, Bangladesh Abstract: In this study, an attempt is made to study the joint distribution functions for simultaneous velocity, temperature, concentration fields in turbulent flow in presence of dust particles. The various properties of the constructed joint distribution functions such as, reduction property, separation property, coincidence and symmetric properties have been discussed. The transport equations for one and two point joint distribution functions in presence of dust particles have been derived. Keywords: Concentration, distribution functions, dust particles, turbulence INTRODUCTION In molecular kinetic theory in physics, a particle's distribution function is a function of several variables. Particle distribution functions are often used in plasma physics to describe wave-particle interactions and velocity-space instabilities. Distribution functions are also used in fluid mechanics, statistical mechanics and nuclear physics. A distribution function may be specialized with respect to a particular set of dimensions. Distribution functions may also feature non-isotropic temperatures, in which each term in the exponent is divided by a different temperature. The mathematical analog of a distribution is a measure; the time evolution of a measure on a phase space is the topic of study in dynamical systems. In the past, several researchers discussed the distribution functions in the statistical theory of turbulence. Lundgren (1967) derived the transport equation for the distribution of velocity in turbulent flow. Bigler (1976) gave the hypothesis that in turbulent flames, the thermo chemical quantities can be related locally to few scalars and considered the probability density function of these scalars. Kishore (1978) studied the distributions functions in the statistical theory of MHD turbulence of an incompressible fluid. Dixit and Upadhyay (1989) discussed the Distribution functions in the statistical theory of MHD turbulence of an incompressible fluid in presence of the coriolis force. Pope (1981) derived the transport equation for the joint probability density function of velocity and scalars in turbulent flow. Kollman and Janica (1982) obtained the transport equation for the probability density function of a scalar in turbulent shear flow. Kishore and Singh (1984) derived the transport equation for the bivariate joint distribution function of velocity and temperature in turbulent flow. Also Kishore and Singh (1985) have been derived the transport equation for the joint distribution function of velocity, temperature and concentration in convective turbulent flow. Sarker and Kishore (1991) discussed the distribution functions in the statistical theory of convective MHD turbulence of an incompressible fluid. Also Sarker and Kishore (1999) studied the distribution functions in the statistical theory of convective MHD turbulence of mixture of a miscible incompressible fluid. Azad and Sarker (2004) discussed Statistical theory of certain distribution functions in MHD turbulence in a rotating system in presence of dust particles. Islam and Sarker (2007) studied distribution functions in the statistical theory of MHD turbulence for velocity and concentration undergoing a first order reaction. But at this stage, one is met with the difficulty that the N-point distribution function depends upon the N+1-point distribution function and thus result is an unclosed system. This so-called closer problem is encountered in turbulence, Kinetic theory and other non-linear system. In this study, we have been derived the joint distribution functions for the evolution of transport equations and various properties of the distribution function have been discussed for velocity, temperature, concentration in convective turbulent flow in presence of dust particles. MATERIALS AND METHODS Basic equations: The equation of motion and field equations of temperature and concentration in presence of dust particles are given by: Corresponding Author: M.A.K. Azad, Department of Applied Mathematics, University of Rajshahi, Rajshahi-6205, Bangladesh 4150 Res. J. Appl. Sci. Eng. Technol., 4(20): 4150-4159, 2012 u u u t x x dx 1 u x , t u x , t 0 4 x x x x u ƒu v x x u x x x t c c c D u x x x t (2) (3) u v 0 x x With where, uα (x, t) (x, t) c v ƒ N = = = = = = ρ D γ cp vα kT = = = = = = Component of turbulent velocity Temperature fluctuation Concentration of contaminants Kinematics viscosity KN/ρ = Dimension of frequency Constant number of density of the dust particle Fluid density Diffusive coefficient for contaminants kT /ρcp = Thermal diffusivity Specific heat at constant pressure Dust particle velocity Thermal conductivity Here u and x are vector quantities in the whole process. Formulation of the problem: We consider the turbulence and the concentration fields are homogeneous, also consider a large ensemble of mixture of miscible fluids in which each member is an infinite incompressible heat conducting fluid in turbulent state. The fluid velocity u, temperature θ and concentration c are randomly distributed functions of position and time and satisfy their field equations. Different members of ensemble are subjected to different initial conditions and the aim is to find out a way by which we can determine the ensemble averages at the initial time. The present aim is to construct a joint distribution functions, study its properties and derive an equation for its evolution of this joint distribution functions in presence of dust particles. fluid velocity u, temperature θ, concentration c at each point of the flow field in turbulence. Lundgren (1967) and Sarker and Islam (2002) has studied the flow field on the basis of one variable character only (namely the fluid velocity u) but we can study it for two or more variable characters as well. The corresponding to each point of the flow field, we have three measurable characteristics. We represent the three variables by v, φ and ψ and denote the pairs of these variables at the points x(1), x(2),…, x(n) as (v(1), φ(1),ψ(1)), (v(2), φ(2),ψ(2)), - - -, (v(n), φ(n),ψ(n)), at a fixed instant of time. It is possible that the same pair may be occurring more than once; therefore, we simplify the problem by an assumption that the distribution is discrete (in the sense that no pairs occur more than once). Instead of considering discrete points in the flow field if we consider the continuous distribution of the variables and ψ over the entire flow field, statistically behavior of the fluid may be described by the distribution function F(v, φ ,ψ) which is normalized so that: F v, , dv d d 1 where, the integration ranges over all the possible values of v, φ and ψ. We shall make use of the same normalization condition for the discrete distributions also. The joint distribution functions of the above quantities can be defined in terms of Dirac Deltafunctions. The one-point joint distribution function F1(1) (v(1), (1) (1) φ ,ψ ) is defined in such a way that F1(1) (v(1), φ(1),ψ(1)) dv(1) φ(1) dψ(1) is the probability that the fluid velocity, temperature and concentration field at a time t are in the element dv(1) about v(1), φ(1) about φ(1) and dψ(1) about ψ(1), respectively and is given as: u v c F11 v 1 , 1 , 1 1 1 1 1 1 1 (4) where, δ is the Dirac delta-function defined as: u v dv 1 at the po int u v 0 otherwise Two-point joint distribution function is given by: Joint distribution function in convective turbulence and their properties: It may be considered that the 4151 F21, 2 u 1 v 1 1 1 c 1 1 u 2 v 2 2 2 c 2 2 (5) Res. J. Appl. Sci. Eng. Technol., 4(20): 4150-4159, 2012 And similarly: and three point distribution function is shown by: c u v c u v c F31, 2,3 u 1 v 1 1 1 1 1 2 2 2 2 3 2 3 3 Lim x 3 x 2 2 (6) 3 Similarly, we can define an infinite numbers of multi-point joint distribution functions F4(1,2,3,4), F5(1,2,3,4,5) and so on. The joint distribution functions so constructed have the following properties: Reduction properties: Integration with respect to pair of variables at one-point, lowers the order of distribution function by one. For example: v 2 v 1 , 2 1 F21, 2 dv 2 d 2 d 2 F11 And hence it follows that: Lim x 2 x 1 Similarly: F31, 2,3 dv 3 d 3 d 3 F21, 2 Lim x 3 x 2 F31, 2,3 F21, 2 v 3 v 1 3 1 3 1 etc. and so on. Also the integration with respect to any one of the variables reduces the number of Delta-functions from the distribution function by one as: 1 F1 dv 1 1 1 F1 d 1 1 u 1 c 1 v 1 c 1 1 1 c 2 Fn1, 2,r ,s ,n Fn1, 2,s ,r ,n Continuity equation in terms of distribution functions: An infinite number of continuity equations can be derived for the convective turbulent flow and the continuity equations can be easily expressed in terms of distribution functions and are obtained directly by div u = 0: F21, 2 dv 2 1 1 c 1 1 2 Symmetric conditions: and 2 0 and so on. Separation properties: The pairs of variables at the two points are statistically independent of each other if these points are far apart from each other in the flow field i.e., Lim x 2 x 1 F21, 2 F11 v 2 v 1 2 1 2 1 F21, 2 dv 2 d 2 d 2 F11 and 2 1 But also F2(1, 2) must have the property: F11 dv 1 d 1 d 1 1 2 e t c. Co-incidence property: When two points coincide in the flow field, the components at these points should be obviously the same that is F2 (1, 2) must be zero. Thus: 3 3 F31, 2,3 F21, 2 F13 F21, 2 F11 F12 u1 x1 1 u F11 dv 1 d 1 d 1 x1 u1 F11 dv 1 d 1 d 1 x1 x1 v1 F11 dv 1 d 1 d 1 x1 4152 u 1 F11 dv 1 d 1 d 1 F11 1 1 1 v dv d d 1 x1 (7) Res. J. Appl. Sci. Eng. Technol., 4(20): 4150-4159, 2012 and similarly: 0 F11 1 1 1 1 dv d d x1 (8) Which are the first order continuity equations in which only one point distribution function is involved. For second-order continuity equations, if we multiply the continuity equation by: xr v F dvr d r d r xs v F dvs d s d s x1 1 u u 1 u 1 v 1 1 1 c 1 1 1 1, 2 1 dv d 1 d 1 1 v F1 x 1 F11, 2 dv 1d 1d 1 x1 (9) v1 FN1, 2, N dv 1d 1d 1 x1 u 1 1 u x 1 x 1 (10) 1 0 (14) t t c u1 v1 1 1 (11) u1 v1 c1 1 (12) The continuity equations are symmetric in their arguments i.e., u1 v1 v1 1 1 1 1 ut t u1 v1 1 1 1 1 1 1 u1 v1 c1 1 1 1 1 c1 1 and 0 1 1FN1, 2, N dv1d 1d 1 x F11 dv 1 d 1 d 1 F1 u1 v1 1 1 c1 1 t t 1 1 c1 1 u1 v1 t The Nth-order continuity equations are: 0 1 v Equations for the evolution of joint distribution functions: This, in fact is done by making use of the definitions of the constructed distribution functions, the transport equation for F(v, φ, ψ, x,t) is obtained from the definition of F and from the transport Eq. (1), (2) and (3). Differentiating Eq. (4) we get: and similarly: 0 (13) and all the properties of the distribution function obtained in section (4) can also be easily verified. u 2 v 2 2 2 c 2 2 0 N x1 u 2 v 2 2 2 c 2 2 u1 x1 s 1,2, r s N x 1 and if we take the ensemble average, we obtain: N Since, the divergence property is an important property and it is easily verified by the use of the property of distribution function as: u 2 v 2 2 2 c 2 2 0 u 2 v 2 2 2 c 2 2 r 1,2, s r N 1 ct c1 1 1 Using Eq. (1), (2) and (3) in (15) we get: 4153 (15) Res. J. Appl. Sci. Eng. Technol., 4(20): 4150-4159, 2012 1 F1 t 1 1 c 1 1 1 u 1 1 2 2 u 1 1 2 u 2 u 4 x x x x 1 1 1 u v 2 v 1 dx 1 1 x 1 x 2 x 1 x 1 u ƒ u v 1 u 1 v 1 c 1 1 u1 1 1 1 1 1 1 1 x x x c 1 1 1 u 1 v 1 1 1 u1 1 D 1 1 c 1 1 c x x x u 1 F11 1 1 c 1 1 u1 1 1 u 1 v 1 t x v u 1 v 1 c 1 1 u1 1 1 1 x 1 1 u 1 v 1 1 1 u1 1 1 c 1 1 1 x 1 4 1 1 c 1 1 ƒ u 1 v1 u 1 v 1 v1 1 1 u 1 v 1 1 1 D 1 1 c 1 1 c x x 1 1 1 u v v u 1 v 1 c 1 1 1 1 1 1 1 1 x x dx 2 2 2 u u x 2 x 2 x 1 x 2 1 1 c 1 1 1 1 u1 1 u 1 v 1 v x x c 1 c 1 1 x 1 1 0 (16) Various terms in the above equation can be simplified as that they may be expressed in terms of one point and two point distribution functions. The second, third and fourth term on the left hand side of the above equation are simplified in a similar fashion and take the forms as follows: u 1 u 1 v 1 x 1 1 1 c 1 1 u 1 1 1 c 1 1 u 1 u 1 v 1 x 1 v1 u 1 1 1 v (17) 4154 Res. J. Appl. Sci. Eng. Technol., 4(20): 4150-4159, 2012 1 1 1 x 1 1 1 1 x 1 u 1 v 1 c 1 1 u 1 u 1 v 1 c 1 1 u 1 (18) c 1 1 1 1 1 c x c 1 1 x 1 u 1 v 1 1 1 u 1 u 1 v 1 1 1 u 1 (19) Adding Eq. (17), (18) and (19) we get: 1 1 c 1 1 u1 u 1 v 1 x 1 1 1 x 1 1 1 1 c x u 1 v 1 c 1 1 u1 u 1 v 1 1 1 u1 u 1 u 1 v 1 1 1 c 1 1 x 1 1 1 v F1 x 1 v1 Applying the properties of distributi on function F11 x 1 (20) We reduce the fifth term on left hand side of Eq. (16): x 1 1 1 c 1 1 1 v1 4 2 x x 1 x 2 1 4 dx 2 2 2 u u x 2 x 2 x 1 x 2 1 1 1 u v v v 2 F 1, 2 dx 2 dv 2 d 2 d 2 x 2 2 2 We reduce the sixth term on left hand side of Eq. (16): 4155 (21) Res. J. Appl. Sci. Eng. Technol., 4(20): 4150-4159, 2012 1 u u 1 v 1 x 1 x 1 v 1 1 1 c 1 1 1 1 1 c 1 1 u 1 v 1 1 1 1 u v x x v1 1 1 1 c 1 1 u 1 v 1 1 1 1 u v x x 2 2 2 2 2 2 2 u c u v Lim v1 x 2 x 1 x 2 x 2 1 1 c 1 1 u 1 v 1 dv 2 d 2 d 2 1 u 1 1 c 1 1 u 1 v 1 1 x x 1 2 2 v 2 F21, 2 dv 2 d 2 d 2 1 x Lim 2 1 x v x x (22) We reduce the 7th term on left hand side of Eq. (16): 1 1 c 1 1 ƒu 1 v1 ƒ u 1 v1 1 1 1 u v v u 1 v 1 1 1 c 1 1 v1 1 1 1 1 c 1 1 1 u v v F11 v1 ƒ u 1 v1 ƒ u 1 v1 (23) Similarly, 8th and 9th terms of left hand side of (16) can be simplified as follows: 1 1 1 1 1 x x 1 Lim 2 2 2 F21, 2 dv 2 d 2 d 2 x 2 x 1 x x u 1 v 1 c 1 1 1 1 1 1 c 1 c x 1 x 1 Lim D 2 2 2 F21, 2 dv 2 d 2 d 2 2 1 x x x x u 1 v 1 1 1 D 1 4156 (24) (25) Res. J. Appl. Sci. Eng. Technol., 4(20): 4150-4159, 2012 Substituting the results (20)-(25) in Eq. (16), we get the transport equation for one point distribution function F1(1) (v, φ ,ψ) in turbulent flow in presence of dust particles: 2 1 1, 2 2 2 2 2 2 v 2 F2 dx dv d d 2 1 2 4 x x x x 2 2 v 2 F21, 2 dv 2 d 2 d 2 1 Lim 2 1 v x x x x 1 F11 1 F1 v 1 t x v1 1 x 1 Lim1 2 x 2 1, 2 2 2 2 2 2 F2 dv d d x x Lim D x 2 x 1 2 1, 2 2 2 2 1 ƒ u 1 v1 2 2 F2 dv d d 1 F1 0 x x v (26) , Similarly, a transport equation for two-point distribution function in turbulent flow in presence of dust particles can be derived by differentiating Eq. (5) and using Eq. (1), (2) and (3) and simplifying in the same manner which is: F21, 2 1 2 1, 2 v F2 v x 1 t x2 v2 1 4 x 2 x 2 x 3 2 1 3 v x3 1 4 x1 x 1 x3 v 1 , 2 , 3 3 3 3 F3 dx dv d d 3 2 1, 2,3 3 3 3 3 v 3 F dx dv d d x 3 3 3 3 v 3 F31, 2,3 dv 3 d 3 d 3 1 Lim Lim 2 3 1 3 x 2 x x x v v x x 3 3 3 F31, 2,3 dv 3 d 3 d 3 1 Lim 2 3Lim 3 1 2 x x x x x x D 1 Lim Lim 2 3 3 3 F31, 2,3 dv 3 d 3 d 3 2 3 3 1 x x x x x x ƒ u 1 v1 F21,2 0 v2 (27) Continuing this way, we can derive the equations for evolution of F3(1, 2, 3), F4(1, 2, 3, 4) and so on. Logically, it is possible to have an equation for every Fn (n is an integer) but the system of equations so obtained is not closed. It seems that certain approximations will be required thus obtained. RESULTS AND DISCUSSION If the fluid is clean then f = 0 and the transport equation for one point join distribution function F1(1) (v, φ ,ψ ) in turbulent flow Eq. (26) becomes: 4157 Res. J. Appl. Sci. Eng. Technol., 4(20): 4150-4159, 2012 2 1 1, 2 2 2 2 2 2 v 2 F2 dx dv d d 2 1 2 x x 4 x x 1 Lim 2 2 v 2 F21, 2 dv 2 d 2 d 2 2 1 v x x x x 1 F11 1 F1 v 1 t x v1 1 Lim x 2 x 1 1 2 F21, 2 dv 2 d 2 d 2 2 x x 2 Lim D x 2 x 1 2 1, 2 2 2 2 0 2 2 F2 dv d d x x Which was obtained earlier by Kishore and Singh (1984). For concluding the system of equations for the joint distribution functions, some approximations are required. Closure scheme can be used here and closure can be obtained by decomposing F2(1, 2) as: F2(1,2) = (1 + ε)F1(1) F1(2) (28) F31,2,3 1 F11 F12 F13 (29) 2 where, ε is the correlation coefficient between the particles. The transport equation for the joint distribution function of velocity, temperature and concentration field have been presented to provide the advantageous basis for modeling the turbulent flows in presence of dust particles. ACKNOWLEDGMENT The authors (M. A. K. Azad and M. H. U. Molla) thankfully acknowledge the Ministry of Science and Information and Communication Technology of the Peoples Republic of Bangladesh for granting NSICT fellowship and are also thankful to the Department of Applied Mathematics, University of Rajshahi for providing all facilities during this study. REFERENCES Azad, M.A.K. and M.S.A. Sarker, 2004. Statistical theory of certain distribution functions in MHD turbulence in a rotating system in presence of dust particles: Rajshahi university studies. Part-B. J. Sci., 32: 193-210. Bigler, R.W., 1976. The structure of diffusion flames. Combustion Sci. Tech., 13: 155. Dixit, T. and B.N. Upadhyay, 1989. Distribution functions in the statistical theory of MHD turbulence of an incompressible fluid in the presence of the coriolis force. Astrophy. Space Sci., 153: 297. Islam, M.A. and M.S.A. Sarker, 2007. Distribution functions in the statistical theory of MHD turbulence for velocity and concentration undergoing a first order reaction. 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