Chapter 4: Problem 9
Consider the given initial value problem \(\mathbf{y}^{\prime}=A \mathbf{y}, \mathbf{y}\left(t_{0}\right)=\mathbf{y}_{0}\). (a) Find the eigenvalues and eigenvectors of the coefficient matrix \(A\). (b) Construct a fundamental set of solutions. (c) Solve the initial value problem.\(\mathbf{y}^{\prime}=\left[\begin{array}{lll}2 & 1 & 0 \\ 0 & 2 & 0 \\\ 0 & 0 & 1\end{array}\right] \mathbf{y}, \quad \mathbf{y}(0)=\left[\begin{array}{r}1 \\ 3 \\ -2\end{array}\right]\)
Short Answer
Step by step solution
Find the Eigenvalues and Eigenvectors of Matrix A
Construct a Fundamental Set of Solutions
Solve the Initial Value Problem
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Key Concepts
These are the key concepts you need to understand to accurately answer the question.
Eigenvalues and Eigenvectors
In the example provided, the eigenvalues are \(\lambda_1 = 1\) and \(\lambda_2 = \lambda_3 = 2\). Notice \(\lambda_2\) and \(\lambda_3\) are repeated, having implications for the eigenvectors.
Eigenvectors, linked to each eigenvalue, show directions in which the transformation only stretches. These are derived by solving \((A - \lambda I)\mathbf{v} = 0\). If an eigenvalue is repeated, you might need to find generalized eigenvectors as well. This involves additional computations to ensure enough linearly independent solutions.
Initial Value Problem
In the exercise, the initial value condition is \(\mathbf{y}(0) = \left[\begin{array}{r}1 \ 3 \ -2\end{array}\right]\). By using this information, you can determine constants in the general solution to make sure the solution exactly matches the initial condition at \(t = 0\). This ensures that your solution isn't just any solution, but the one that starts at your specified initial point.
Fundamental Set of Solutions
In this case, solutions derived from eigenvectors \(\mathbf{y}_1(t)\), \(\mathbf{y}_2(t)\), and \(\mathbf{y}_3(t)\) form this set. They are:
- \(\mathbf{y}_1(t) = \left[\begin{array}{r}-1 \ 1 \ 0\end{array}\right]e^{t}\)
- \(\mathbf{y}_2(t) = \left[\begin{array}{r}1 \ 0 \ 0\end{array}\right]e^{2t}\)
- \(\mathbf{y}_3(t) = \left[\begin{array}{r}t \ 1 \ 0\end{array}\right]e^{2t}\)
General Solution of Differential Equations
The formula \( \mathbf{y}(t) = c_1\mathbf{y}_1(t) + c_2\mathbf{y}_2(t) + c_3\mathbf{y}_3(t) \) is a perfect example. The constants \(c_1, c_2,\) and \(c_3\) are determined by initial conditions or boundary values.
In the solution, these constants were computed using the given initial condition \(\mathbf{y}(0) = \left[\begin{array}{r}1 \ 3 \ -2\end{array}\right]\). By setting time \(t = 0\), equations involving \(c_1, c_2, \) and \(c_3\) were solved to fit the starting point exactly. The outcome is a specific solution that both matches the fundamental solutions and satisfies the initial condition.