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In many engineering applications variation in thermal properties is significant especially when there are large temperature gradients or the material is not homogeneous. To account for these variations in thermal properties, develop a finite difference formulation for an internal node in case of a three dimensional steady state heat conduction equation with variable thermal conductivity.

Short Answer

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Question: Develop a finite difference formulation for an internal node in a three-dimensional steady-state heat conduction equation with variable thermal conductivity. Answer: The finite difference formulation for an internal node (i,j,k) in a three-dimensional steady-state heat conduction problem with variable thermal conductivity can be expressed as: 0 ≈ k(i+1/2,j,k) * (∇^2T)_x + k(i,j+1/2,k) * (∇^2T)_y + k(i,j,k+1/2) * (∇^2T)_z where k(i+1/2,j,k) = (k(i+1,j,k) + k(i,j,k)) / 2, and the second derivatives of temperature (∇^2T)_x, (∇^2T)_y, and (∇^2T)_z are obtained using the central difference method. This equation, along with similar equations for all internal nodes, forms a system of linear equations that can be solved using numerical methods such as Gauss-Seidel or Conjugate Gradient.

Step by step solution

01

Discretize the spatial domain

Divide the three-dimensional domain into small elements or finite differences, using uniform grid-spacing in all three directions: x, y, and z. Denote the increments with Δx, Δy, and Δz, respectively. The Cartesian coordinates of an internal node will be (i*Δx, j*Δy, k*Δz), where i, j, and k are integer indices for the nodes.
02

Approximate the derivatives with central differences

First, calculate the partial derivatives of the variable thermal conductivity with respect to x, y, and z. Then, approximate them with central differences. For example, the partial derivative with respect to x is: (∇k)_x = (k(i+1,j,k) - k(i-1,j,k)) / (2*Δx) Do the same for y and z directions. Next, approximate the second derivatives of the temperature with respect to x, y, and z using the central difference method. For example, the second derivative with respect to x is: (∇^2T)_x = (T(i+1,j,k) - 2*T(i,j,k) + T(i-1,j,k)) / (Δx^2) Repeat this process for the y and z directions as well.
03

Combine the derivatives into the finite difference equation

Substitute the approximated derivatives (Step 2) into the 3D steady-state heat conduction equation: (∇(k(x,y,z)∇T(x,y,z))) ≈ ( (∇k)_x * (∇T)_x + (∇k)_y * (∇T)_y + (∇k)_z * (∇T)_z
04

Incorporate the variable thermal conductivity

Multiply the thermal conductivity with the second derivatives of the temperature in each direction, and sum these terms: 0 ≈ k(i+1/2,j,k) * (∇^2T)_x + k(i,j+1/2,k) * (∇^2T)_y + k(i,j,k+1/2) * (∇^2T)_z Here, we use interpolated values of the thermal conductivity at the cell faces, e.g., k(i+1/2,j,k) = (k(i+1,j,k) + k(i,j,k)) / 2.
05

Simplify and solve for the internal temperature node

Rearrange the equation from Step 4 to express T(i, j, k) - the internal node temperature - as a function of its neighboring nodes' temperatures and thermal conductivities. This equation will become a part of the system of linear equations that can be solved with methods such as Gauss-Seidel or Conjugate Gradient.

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Key Concepts

These are the key concepts you need to understand to accurately answer the question.

Three-Dimensional Heat Conduction
Three-dimensional heat conduction involves the transfer of thermal energy in space within a material across three dimensions: length, width, and height. The main goal is to understand how heat moves through a 3D object given certain boundary conditions.
  • Think of heat conduction like the diffusion of heat. Heat flows from regions of high temperature to regions of low temperature.
  • In 3D, this means heat can spread out in multiple directions, making it more complex than one-dimensional cases.
  • We model this process using the heat equation, which is a form of the diffusion equation.
This concept is crucial in various engineering applications, like designing thermal systems in vehicles or electronic devices, where materials need to distribute heat evenly.
Variable Thermal Conductivity
Thermal conductivity refers to a material's ability to conduct heat, which can vary within the same material depending on temperature or other factors. When working with variable thermal conductivity:
  • It's essential because realistic materials often do not have constant properties due to non-homogeneity or temperature gradients.
  • Mathematically, the thermal conductivity becomes a function of space and possibly temperature, represented as \(k(x, y, z)\).
  • To tackle this in calculations, you use interpolated values such as \(k(i+1/2,j,k)\), which represents thermal conductivity at the midpoint between nodes.
Considering variable thermal conductivity provides more accurate results, especially for simulations involving high precision thermal management.
Central Difference Approximation
The central difference approximation is a mathematical technique used to estimate derivatives, a key part of solving differential equations numerically. Let’s explore why it's useful in heat conduction problems:
  • It provides a way to calculate the rate of change of a function by considering the function's values at two adjacent points.
  • In a grid, for a function defined on discrete points, the central difference formula for the first derivative \((∇f)_x\) is \((f(i+1) - f(i-1))/(2 \Delta x)\).
  • Similarly, the central difference approximation for the second derivative \((∇^2f)_x\) is \((f(i+1) - 2f(i) + f(i-1))/(\Delta x^2)\).
This method is favored because it is generally more accurate than forward or backward difference approximations.
Steady-State Heat Equation
The steady-state heat equation describes a condition where the temperature in the system does not change with time. Understanding this can simplify the analysis greatly:
  • This implies that any heat entering a specific area of the material is equal to the heat leaving it, resulting in a stable temperature.
  • The equation for a steady state in three dimensions is \(∇(k(x,y,z)∇T(x,y,z)) = 0\), where \(T\) is the temperature.
  • The finite difference method is used for discretizing this equation to handle complex shapes and boundary conditions more easily.
Understanding and applying the steady-state heat equation helps in optimizing thermal systems for efficiency and effectiveness in maintaining desired temperature conditions.

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Most popular questions from this chapter

The unsteady forward-difference heat conduction for a constant area, \(A\), pin fin with perimeter, \(p\), exposed to air whose temperature is \(T_{0}\) with a convection heat transfer coefficient of \(h\) is $$ \begin{aligned} T_{m}^{*+1}=& \frac{k}{\rho c_{p} \Delta x^{2}}\left[T_{m-1}^{*}+T_{m+1}^{*}+\frac{h p \Delta x^{2}}{A} T_{0}\right] \\\ &-\left[1-\frac{2 k}{\rho c_{p} \Delta x^{2}}-\frac{h p}{\rho c_{p} A}\right] T_{m}^{*} \end{aligned} $$ In order for this equation to produce a stable solution, the quantity \(\frac{2 k}{\rho c_{p} \Delta x^{2}}+\frac{h p}{\rho c_{p} A}\) must be (a) negative (b) zero (c) positive (d) greater than 1 (e) less than 1

Consider one-dimensional transient heat conduction in a plane wall with variable heat generation and variable thermal conductivity. The nodal network of the medium consists of nodes 0,1 , and 2 with a uniform nodal spacing of \(\Delta x\). Using the energy balance approach, obtain the explicit finite difference formulation of this problem for the case of specified heat flux \(\dot{q}_{0}\) and convection at the left boundary (node 0 ) with a convection coefficient of \(h\) and ambient temperature of \(T_{\infty}\), and radiation at the right boundary (node 2 ) with an emissivity of \(\varepsilon\) and surrounding temperature of \(T_{\text {surr }}\).

Define these terms used in the finite difference formulation: node, nodal network, volume element, nodal spacing, and difference equation.

How is the finite difference formulation for the first derivative related to the Taylor series expansion of the solution function?

Consider a medium in which the finite difference formulation of a general interior node is given in its simplest form as $$ T_{\text {node }}=\left(T_{\text {left }}+T_{\text {top }}+T_{\text {right }}+T_{\text {bottom }}\right) / 4 $$ (a) Is heat transfer in this medium steady or transient? (b) Is heat transfer one-, two-, or three-dimensional? (c) Is there heat generation in the medium? (d) Is the nodal spacing constant or variable? (e) Is the thermal conductivity of the medium constant or variable?

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