What are the basic steps involved in solving a system of equations with Gauss- Seidel method?

Short Answer

Expert verified
Answer: The primary purpose of the Gauss-Seidel method is to iteratively solve systems of linear equations. The main steps involved in solving a system of linear equations using this method include: 1) understanding the given system of linear equations, 2) separating the diagonal, lower, and upper matrices, 3) forming the iterative formula, 4) initializing the starting solution estimates, 5) performing iterations, 6) checking the convergence, and 7) reporting the final solution.

Step by step solution

01

Understand the given system of linear equations

Write down the given system of linear equations in matrix form. The system will be represented as Ax=b, where A is the coefficient matrix, x is the solution vector, and b is the constant vector.
02

Separate the diagonal, lower, and upper matrices

Split the matrix A into three matrices: the diagonal matrix (D), the lower triangular matrix (L), and the upper triangular matrix (U). D contains the diagonal elements of A, L contains the elements below the diagonal, and U has the elements above the diagonal.
03

Form the iterative formula

Form the Gauss-Seidel iterative formula using the inverse of (D+L) matrix and the U matrix. The formula will be in the following format: x^{(k+1)} = (D+L)^{-1} * (b - U * x^{(k)}), where x^{(k)} is the current estimate of the solution and x^{(k+1)} is the updated estimate.
04

Initialize the starting solution estimates

Set an initial estimate for the solution vector x^{(0)}. In most cases, it is common to start with a zero vector. However, any initial guess can be used in the Gauss-Seidel method.
05

Perform iterations

Update the solution vector estimates using the iterative formula obtained in step 3: x^{(k+1)} = (D+L)^{-1} * (b - U * x^{(k)}). Continue updating the solution estimates until a specified convergence criterion is met. Common convergence criteria include a predefined number of iterations or a tolerance for the difference between consecutive estimates.
06

Check the convergence

Check if the sequence of estimates has converged to the true solution within the given tolerance or within the specified number of iterations. If the convergence criterion is not met, continue iterating using the iterative formula until convergence is achieved.
07

Report the final solution

Once the convergence criterion is met, the final estimate x^{(k+1)} of the solution vector is the approximate solution to the given system of linear equations.

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Key Concepts

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

Solving System of Linear Equations
The Gauss-Seidel method is an algorithm used for finding the solutions to a system of linear equations, which is one of the fundamental tasks in algebra and an essential tool in various scientific fields. To solve such a system, you usually need to find the values for variables that make all equations hold true simultaneously.

In mathematical terms, if you have equations with variables, the aim is to find the set of values for those variables that satisfy all the equations. This situation is often represented in matrix form as \( Ax = b \) where \( A \) is a square matrix representing the coefficients, \( x \) is a column vector of variables, and \( b \) is the result vector.

The Gauss-Seidel method dives into this matrix equation and employs an iterative approach to zero in on the solution. It starts with an initial guess and improves the solution incrementally until the results are satisfactory—an approach that is particularly useful when dealing with large systems where direct methods like matrix inversion might be computationally expensive or unfeasible.
Iterative Solution Methods
Iterative methods, such as the Gauss-Seidel method, are techniques that progressively improve estimates of the solution to a system of equations through repeated cycles or iterations. Unlike direct methods that aim to solve the system in a finite number of steps, iterative techniques refine the solution until it is close enough to the true answer within an acceptable error margin.

Each iteration of the Gauss-Seidel method involves updating the estimate of the solution vector. Starting from an initial guess, which could be as simple as a zero vector, the method applies the iteration formula derived from the matrix equation to obtain a new and improved estimate. This process is repeated, with each successive estimate hopefully closer to the true solution, demonstrating the core principle of iterative improvement.

The significant advantage of iterative methods is their ability to handle very large systems where other methods struggle due to computational or memory constraints. They are, therefore, often the go-to solution for numerical problems in engineering and computational sciences.
Convergence Criteria
An important concept when using iterative methods like Gauss-Seidel is 'convergence'. Convergence refers to the point at which successive estimates of the solution are close enough to each other and to the true solution that further iterations do not yield significant improvements.

Convergence criteria are the rules that determine whether the iterative process can be halted. This might be a maximum number of iterations allowed, or more commonly, a threshold value for the change in the solution estimates from one iteration to the next. If the difference between successive iterations is less than this threshold, we say the method has 'converged'.

Careful attention to the convergence criteria is vital for ensuring the result is accurate without exhausting computational resources. However, it is also important to note that not all systems will converge using the Gauss-Seidel method. Checking the properties of the matrix \( A \), such as its diagonally dominant nature, can give us insights into whether the method is likely to be successful or not.
Matrix Decomposition
Matrix decomposition is the process of breaking a matrix down into a set of simpler matrices whose product equals the original matrix. In the context of the Gauss-Seidel method, the matrix \( A \) is decomposed into three components: the diagonal matrix \( D \), the lower triangular matrix \( L \), and the upper triangular matrix \( U \).

The importance of this decomposition comes into play when forming the iterative formula. The method leverages the inverted sum of the diagonal and the lower triangular matrix, \((D+L)^{-1}\), to compute the next estimate from the current one. This aspect of the Gauss-Seidel approach reflects the power of matrix decomposition; by simplifying the complex system into more manageable parts, we can employ efficient computation strategies to advance towards a solution.

Understanding matrix decomposition can also yield insights into the nature of linear systems and is a cornerstone of other numerical methods such as QR decomposition or singular value decomposition, each having their unique applications in solving linear systems or in other areas of linear algebra and beyond.

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Most popular questions from this chapter

A circular fin of uniform cross section, with diameter of \(10 \mathrm{~mm}\) and length of \(50 \mathrm{~mm}\), is attached to a wall with surface temperature of \(350^{\circ} \mathrm{C}\). The fin is made of material with thermal conductivity of \(240 \mathrm{~W} / \mathrm{m} \cdot \mathrm{K}\), and it is exposed to an ambient air condition of \(25^{\circ} \mathrm{C}\) and the convection heat transfer coefficient is \(250 \mathrm{~W} / \mathrm{m}^{2} \cdot \mathrm{K}\). Assume steady one-dimensional heat transfer along the fin and the nodal spacing to be uniformly \(10 \mathrm{~mm},(a)\) using the energy balance approach, obtain the finite difference equations to determine the nodal temperatures, \((b)\) determine the nodal temperatures along the fin by solving those equations and compare the results with the analytical solution, and (c) calculate the heat transfer rate and compare the result with the analytical solution.

Consider an aluminum alloy fin \((k=180 \mathrm{~W} / \mathrm{m} \cdot \mathrm{K})\) of triangular cross section whose length is \(L=5 \mathrm{~cm}\), base thickness is \(b=1 \mathrm{~cm}\), and width \(w\) in the direction normal to the plane of paper is very large. The base of the fin is maintained at a temperature of \(T_{0}=180^{\circ} \mathrm{C}\). The fin is losing heat by convection to the ambient air at \(T_{\infty}=25^{\circ} \mathrm{C}\) with a heat transfer coefficient of \(h=25 \mathrm{~W} / \mathrm{m}^{2} \cdot \mathrm{K}\) and by radiation to the surrounding surfaces at an average temperature of \(T_{\text {surr }}=290 \mathrm{~K}\). Using the finite difference method with six equally spaced nodes along the fin in the \(x\)-direction, determine \((a)\) the temperatures at the nodes and \((b)\) the rate of heat transfer from the fin for \(w=1 \mathrm{~m}\). Take the emissivity of the fin surface to be \(0.9\) and assume steady one-dimensional heat transfer in the fin.

Consider a 2-m-long and 0.7-m-wide stainless-steel plate whose thickness is \(0.1 \mathrm{~m}\). The left surface of the plate is exposed to a uniform heat flux of \(2000 \mathrm{~W} / \mathrm{m}^{2}\) while the right surface of the plate is exposed to a convective environment at \(0^{\circ} \mathrm{C}\) with \(h=400 \mathrm{~W} / \mathrm{m}^{2} \cdot \mathrm{K}\). The thermal conductivity of the stainless steel plate can be assumed to vary linearly with temperature range as \(k(T)=k_{o}(1+\beta T)\) where \(k_{o}=48 \mathrm{~W} / \mathrm{m} \cdot \mathrm{K}\) and \(\beta=9.21 \times 10^{-4}{ }^{\circ} \mathrm{C}^{-1}\). The stainless steel plate experiences a uniform volumetric heat generation at a rate of \(8 \times 10^{5} \mathrm{~W} / \mathrm{m}^{3}\). Assuming steady state one-dimensional heat transfer, determine the temperature distribution along the plate thickness.

Consider a medium in which the finite difference formulation of a general interior node is given in its simplest form as $$ T_{\text {left }}+T_{\text {top }}+T_{\text {right }}+T_{\text {bottom }}-4 T_{\text {node }}+\frac{\dot{e}_{\text {node }} l^{2}}{k}=0 $$ (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?

Consider steady one-dimensional heat conduction in a plane wall with variable heat generation and constant thermal conductivity. The nodal network of the medium consists of nodes \(0,1,2\), and 3 with a uniform nodal spacing of \(\Delta x\). The temperature at the left boundary (node 0 ) is specified. Using the energy balance approach, obtain the finite difference formulation of boundary node 3 at the right boundary for the case of combined convection and radiation with an emissivity of \(\varepsilon\), convection coefficient of \(h\), ambient temperature of \(T_{\circ}\), and surrounding temperature of \(T_{\text {surr }}\). Also, obtain the finite difference formulation for the rate of heat transfer at the left boundary.

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