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Using thermodynamics, we can prove that, for all positions r and r’ in a system, equilibrium is given by p(r) = p(r’) T(r) = T(r’) μ(r) = μ(r’) where p(r) is the pressure, T(r) is the temperature, and μα(r) is the chemical potential of species α at position r. Mathematically, this tells us that the pressure, temperature, and chemical potentials are uniform in a system at equilibrium. If there is a gradient in any of these quantities, then the system is out of equilibrium. As a consequence, momentum, energy, and mass will flow through the system to try to bring it to equilibrium. Most processes that are of practical interest are not in equilibrium and never truly achieve equilibrium. In order to describe these systems, we need to study fluid mechanics, heat transfer, and mass transport, which are also known collectively as non-equilibrium thermodynamics or transport phenomena.
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NON-EQLBM THERMODYNAMICS
Postulate I Although system as a whole is not in eqlbm., arbitrary small elements of it are in local thermodynamic eqlbm & have state fns. which depend on state parameters through the same relationships as in the case of eqlbm states in classical eqlbm thermodynamics.
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NON-EQLBM THERMODYNAMICS
Postulate II Entropy gen rate affinities fluxes All sorts of transport only take place when a force, called a driving force, is applied. Transport is generally expressed as a flux J, which is defined by the amount of mass, energy, momentum, volume, or charges that are being transported pr. area pr. time.
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NON-EQLBM THERMODYNAMICS
Purely “resistive” systems Flux is dependent only on affinity at any instant at that instant System has no “memory”-
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NON-EQLBM THERMODYNAMICS
Coupled Phenomenon Since Jk is 0 when affinities are zero,
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NON-EQLBM THERMODYNAMICS
where kinetic Coeff Relationship between affinity & flux from ‘other’ sciences Postulate III
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NON-EQLBM THERMODYNAMICS
Postulate IV Onsager theorem {in the absence of magnetic fields}
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Analysis of thermo-electric circuits
Addl. Assumption : Thermo electric phenomena can be taken as LINEAR RESISTIVE SYSTEMS {higher order terms negligible} Here K = 1,2 corresp to heat flux “Q”, elec flux “e”
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Analysis of thermo-electric circuits
Above equations can be written as Substituting for affinities, the expressions derived earlier, we get
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Analysis of thermo-electric circuits
We need to find values of the kinetic coeffs. from exptly obtainable data. Defining electrical conductivity as the elec. flux per unit pot. gradient under isothermal conditions we get from above
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Substituting the formula of normalvector:
In transport phenomena (heat transfer, mass transfer and fluid dynamics), flux is defined as the rate of flow of a property per unit area, which has the dimensions [quantity]·[time]−1·[area] j=I/A, where I=dq/dt In all cases the frequent symbol j, (or J) is used for flux, q for the physical quantity that flows, t for time, and A for area. As a mathematical concept, flux is represented by the surface integral of a vector field The surface has to be orientable, i.e. two sides can be distinguished: the surface does not fold back onto itself. Also, the surface has to be actually oriented, i.e. we use a convention as to flowing which way is counted positive; flowing backward is then counted negative. Substituting the formula of normalvector:
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Fluxes Quantity transferred through a given area per unit time Flux occurs because of a spatial and time-varying gradient of an associated system property. Flux occurs in opposition to spatial gradient Flux continues until the gradient is nullified and equilibrium is reached. Flux continues until external force stop The most general relation for a flux in the x-direction is: This relates a flux to a gradient of a property (not specically defined to be anyting at this point) Flux is a linear response; this treatment assumes a perturbative displacement from equilibrium.
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Transport fluxes Eight of the most common forms of flux from the transport phenomena literature are defined as follows: Momentum flux, the rate of transfer of momentum across a unit area (N·s·m−2·s−1). (Newton's law of viscosity) Heat flux, the rate of heat flow across a unit area (J·m−2·s−1). (Fourier's law of conduction)(This definition of heat flux fits Maxwell's original definition.) Diffusion flux, the rate of movement of molecules across a unit area (mol·m−2·s−1). (Fick's law of diffusion) Volumetric flux, the rate of volume flow across a unit area (m3·m−2·s−1). (Darcy's law of groundwater flow) Mass flux, the rate of mass flow across a unit area (kg·m−2·s−1). (Either an alternate form of Fick's law that includes the molecular mass, or an alternate form of Darcy's law that includes the density.) Radiative flux, the amount of energy transferred in the form of photons at a certain distance from the source per unit area per second (J·m−2·s−1). Used in astronomy to determine the magnitude and spectral class of a star. Also acts as a generalization of heat flux, which is equal to the radiative flux when restricted to the infrared spectrum. Energy flux, the rate of transfer of energy through a unit area (J·m−2·s−1). The radiative flux and heat flux are specific cases of energy flux. Particle flux, the rate of transfer of particles through a unit area ([number of particles] m−2·s−1) These fluxes are vectors at each point in space, and have a definite magnitude and direction. Also, one can take the divergence of any of these fluxes to determine the accumulation rate of the quantity in a control volume around a given point in space. For incompressible flow, the divergence of the volume flux is zero.
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NON-EQLBM THERMODYNAMICS
Heat Flux : Momentum : Mass : Electricity :
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Concentration / chemical potential
Diffusion Mass flow process by which species change their position relative to their neighbours Driven by thermal energy and a gradient Thermal energy → thermal vibrations → Atomic jumps Concentration / chemical potential Gradient Electric Magnetic Stress
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Matter transport is down the concentration gradient
Fick’s I law Diffusion coefficient/ diffusivity No. of atoms crossing area A per unit time Cross-sectional area Concentration gradient Matter transport is down the concentration gradient Flow direction A As a first approximation assume D f(t)
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Steady-State Diffusion
Diffusion flux does not change with time Concentration profile: Concentration (kg/m3) vs. position Concentration gradient: dC/dx (kg / m4)
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Steady-State Diffusion
Fick’s first law: J proportion to dC/dx D=diffusion coefficient Concentration gradient is ‘driving force’ Minus sign means diffusion is ‘downhill’: toward lower concentrations
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Fick’s first law
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Diffusivity (D) → f(A, B, T)
Steady state diffusion C1 D f(c) Concentration → C2 D = f(c) x →
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Non-steady state J = f(x,t)
D f(c) Steady state J f(x,t) D = f(c) Diffusion D f(c) Non-steady state J = f(x,t) D = f(c)
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Equations are based on the following physical principles:
Mass is conserved Newton’s Second Law: The First Law of thermodynamics: De = dq - dw, for a system.
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Control Volume Analysis
The governing equations can be obtained in the integral form by choosing a control volume (CV) in the flow field and applying the principles of the conservation of mass, momentum and energy to the CV.
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Consider a differential volume element dV in the flow field
Consider a differential volume element dV in the flow field. dV is small enough to be considered infinitesimal but large enough to contain a large number of molecules for continuum approach to be valid. dV may be: fixed in space with fluid flowing in and out of its surface or, moving so as to contain the same fluid particles all the time. In this case the boundaries may distort and the volume may change.
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Substantial derivative
(time rate of change following a moving fluid element)
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Conservation of mass Control element u r DX Mass balance: or
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Compartmental Analysis
X in X X out X is some variable of interest A change in X = X in – X out in derivative terms:
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What is Diffusion? Definition – the process by which a substance disperses within an ambient medium over time Modeled using compartmental analysis Net change of substance at a point = (inflow rate of substance) – (outflow rate of the substance)
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Diffusion through a Region Ω
The region may contain sources and sinks.
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Modeling Diffusion (the nuts and bolts)
u = u(x, y, z, t) = density at a point in the region f = f(x, y, z, t) = production at a point (a density) in the region due to sources and sinks J = J(x, y, z, t) = flux density at a point
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Some Calculus = total mass in region = rate of mass change in region
= total production of mass in region due to sources and sinks
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The Confusing Quantity of Flux
J = J(x, y, z, t) = flux density at a point (density x velocity) The units of flux are: small flux in the negative x direction large flux in the positive x direction
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What can we do with Flux? Mass leaving the region through the boundary will be the component of the flux that is in the direction of the surface normal = total flux out of the region in the direction of at a point on the boundary = total flux (accumulation of mass) out of the region through the boundary
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Putting Together the Pieces
Using compartmental analysis we can write an equation relating all the components we have developed thus far. rate of substance change = amount produced in the region – amount that escapes the region
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gradient Divergence Theorem (Gauss’s Theorem) a Method of modifying the flux integral The amount of mass that overflows the boundary must be equal to the total change in mass within the boundary. Total flow across the boundary = cumulative flow in the region omega The Bathtub Overflow Theorem Johann Carl Friedrich Gauss Born: 30 April 1777 Brunswick, Germany Died: 23 Feb 1855 Göttingen, Germany
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Simplification Divergence Theorem
Eq2: a = b – total cumulative rate of flow
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Almost there… Theorem from Real Analysis If you integrate over all subregions of “OMEGA” and get zero, the expression integrated must also be equal to zero
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The Unrefined Diffusion Equation
density change at a point over time = density production at that point per unit time – the divergence (the rate of flow from that point)
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Fick’s Law Gradient Adolph Fick
During diffusion we assume particles move in the direction of least density. They move down the concentration gradient In mathematical terms we will assume Flux density = Diffusion coefficient * the gradient of the concentration, negative means flow is in the direction of least density Where D is a constant of proportionality called the Diffusion Coefficient Adolph Fick Born: 1829 Cassel, Germany Died: 1879
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Ockham’s Razor When faced with a choice between two things, choose the simpler. If we assume D is constant and substitute the new expression we found for flux using Fick’s Law we can remove the flux density component of our diffusion equation as follows: William of Ockham Born: 1288 Ockham, England Died: 9 April Munich, Bavaria
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The Laplacian Pierre-Simon Laplace
Born: 23 March 1749 Normandy, France Died: 5 March 1827 Paris, France
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The Refined Diffusion Equation
Separate slide for Laplacian explanation, picture
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Initial and Boundary Conditions
1. Initial conditions (IC) : The initial state of the primary variables of the system: For non-horizontal systems: Where Pref is reference pressure & ρ is fluid densities
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Multiphase Flow Continuity equation for each fluid phase :
Darcy equation for each phase : Oil density equation: roL: the part of oil remaining liquid at the surface roG : the part that is gas at the surface
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Continuity Equation Consider the CV fixed in space. Unlike the earlier case the shape and size of the CV are the same at all times. The conservation of mass can be stated as: Net rate of outflow of mass from CV through surface S = time rate of decrease of mass inside the CV
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The net outflow of mass from the CV can be written as
Note that by convention is always pointing outward. Therefore can be (+) or (-) depending on the directions of the velocity and the surface element.
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Total mass inside CV Time rate of increase of mass inside CV (correct this equation) Conservation of mass can now be used to write the following equation See text for other ways of obtaining the same equation.
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Integral form of the conservation of mass equation thus becomes
Computational Fluid Dynamics (AE/ME 339) K. M. Isaac MAEEM Dept., UMR Integral form of the conservation of mass equation thus becomes
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Computational Fluid Dynamics (AE/ME 339) K. M. Isaac
MAEEM Dept., UMR
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An infinitesimally small element fixed in space
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Net outflow in x-direction
Net outflow in y-direction Net outflow in z-direction Net mass flow =
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Net rate of outflow from CV = time rate of decrease of mass
volume of the element = dx dy dz mass of the element = r(dx dy dz) Time rate of mass increase = Net rate of outflow from CV = time rate of decrease of mass within CV or
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Which becomes The above is the continuity equation valid for unsteady flow Note that for steady flow and unsteady incompressible flow the first term is zero. Figure 2.6 (next slide) shows conservation and non-conservation forms of the continuity equation. Note an error in Figure 2.6: Dp/Dt should be replace with Dr/Dt.
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Computational Fluid Dynamics (AE/ME 339) K. M. Isaac
MAEEM Dept., UMR
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Momentum equation
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Summary Apply conservation equations to a control volume (CV) As the CV shrinks to infinitesimal volume, the resulting partial differential equations are the Navier-Stokes equations Taylor series can be used to write the variables The total derivative consists of local time derivative and convective derivative terms In incompressible flow, divergence of velocity is a statement of the conservation of volume Need surface and body forces to write the momentum equation Surface forces are: pressure forces, forces due to normal stresses and forces due to shear stresses Body forces are due to weight, magnetism and electrostatics Momentum equation is a vector equation. Can be written in terms of its components.
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