Problem 5
Question
As in Example 1 in the text we have \(R(r)=c_{3} r^{n}+c_{4} r^{-n}\). In order that the solution be bounded as \(r \rightarrow \infty\) we must define \(c_{3}=0 .\) Hence $$u(r, \theta)=A_{0}+\sum_{n=1}^{\infty} r^{-n}\left(A_{n} \cos n \theta+B_{n} \sin n \theta\right)$$ where $$\begin{array}{l} A_{0}=\frac{1}{2 \pi} \int_{0}^{2 \pi} f(\theta) d \theta \\ A_{n}=\frac{c^{n}}{\pi} \int_{0}^{2 \pi} f(\theta) \cos n \theta d \theta \\ B_{n}=\frac{c^{n}}{\pi} \int_{0}^{2 \pi} f(\theta) \sin n \theta d \theta \end{array}$$.
Step-by-Step Solution
Verified Answer
Set \( c_{3}=0 \) for boundedness; express \( u(r, \theta) \) using \( A_n \) and \( B_n \) coefficients, derived as Fourier coefficients.
1Step 1: Analyze Given Functions
We have the function \( R(r) = c_{3} r^{n} + c_{4} r^{-n} \) that needs to be bounded as \( r \rightarrow \infty \). This implies we must eliminate terms that grow as \( r \) becomes large, which means setting \( c_{3} = 0 \). Thus, for a bounded solution we focus on \( c_{4} r^{-n} \).
2Step 2: Analyze Solution Series
Given that \( c_{3} = 0 \) for a bounded solution, the function simplifies to:\[ u(r, \theta) = A_{0} + \sum_{n=1}^{\infty} r^{-n} \left( A_{n} \cos n \theta + B_{n} \sin n \theta \right) \]Here, each term \( r^{-n} \) ensures the boundedness of the solution as \( r \to \infty \).
3Step 3: Define Coefficient \(A_0\)
The coefficient \( A_{0} \) is given by the formula:\[ A_{0} = \frac{1}{2 \pi} \int_{0}^{2 \pi} f(\theta) \, d\theta \]This represents the average value of the function \( f(\theta) \) over the interval from 0 to \( 2\pi \).
4Step 4: Define Coefficient \(A_n\)
The coefficient \( A_{n} \) is calculated using:\[ A_{n} = \frac{c^{n}}{\pi} \int_{0}^{2 \pi} f(\theta) \cos n \theta \, d\theta \]This integral projects \( f(\theta) \) onto \( \cos n \theta \), scaled by \( c^n \) and the factor \( \frac{1}{\pi} \).
5Step 5: Define Coefficient \(B_n\)
The coefficient \( B_{n} \) is given by:\[ B_{n} = \frac{c^{n}}{\pi} \int_{0}^{2 \pi} f(\theta) \sin n \theta \, d\theta \]This integrates \( f(\theta) \) onto \( \sin n \theta \), also scaled by \( c^n \) and \( \frac{1}{\pi} \). These coefficients are part of the Fourier series representation of \( f(\theta) \).
6Step 6: Formulate the Solution
The complete solution for \( u(r, \theta) \) is determined by combining the constant term \( A_0 \) and the series terms involving \( A_n \) and \( B_n \), each multiplied by \( r^{-n} \). The final expression for \( u(r, \theta) \) is:\[ u(r, \theta) = A_{0} + \sum_{n=1}^{\infty} r^{-n} \left( A_{n} \cos n \theta + B_{n} \sin n \theta \right) \]
Key Concepts
Boundary ConditionsHarmonic FunctionsIntegral Calculus
Boundary Conditions
Boundary conditions are essential constraints applied to differential equations or systems to determine a unique solution. In our exercise, we're dealing with the function \( R(r) = c_{3} r^{n} + c_{4} r^{-n} \). Boundary conditions help us ensure the solution behaves in a specific way as the variable approaches certain values, particularly at endpoints or along boundaries of a defined region. When dealing with infinite domains like \( r \rightarrow \infty \), it's crucial to control the behavior of the function.
- For the function to remain bounded as \( r \rightarrow \infty \), we need to remove any terms that grow unbounded. For instance, the term \( c_{3} r^{n} \) increases without bound as \( r \) becomes large unless \( c_{3} \) is set to zero.
- By setting \( c_{3} = 0 \), we eliminate these terms, ensuring the solution only includes diminishing terms \( c_{4} r^{-n} \), which shrink as \( r \) grows.
Harmonic Functions
Harmonic functions are solutions to Laplace's equation \( abla^{2} u = 0 \) and arise naturally in various physical settings, including fluid flow and electrostatics. In the context of Fourier series, harmonic functions have periodic properties which are significant in simplifying complex phenomena:
- A harmonic function like \( u(r, \theta) \) can be separated into radial and angular components, which often simplifies our task by breaking down complex problems into more manageable parts.
- The exercise employs Fourier series expansion to express \( u(r, \theta) \) in terms of sine and cosine functions. These trigonometric components \( \cos n \theta \) and \( \sin n \theta \) play the crucial role of harmonics, resembling waves that exhibit the property of harmonicity.
- In simpler terms, when solving problems that involve variations in space and periodic boundary conditions, harmonic functions help represent solutions that can be easily manipulated and understood.
Integral Calculus
Integral calculus, a key area of mathematics, deals with integration and its applications. In this exercise, integration is essential for determining coefficients in the Fourier series representation of \( f(\theta) \):
\( A_0 = \frac{1}{2 \pi} \int_{0}^{2 \pi} f(\theta) \, d\theta \) is the average value of the function over one period \( [0, 2\pi] \). This integral helps determine the constant term in the Fourier series, representing a mean level or equilibrium state of \( f(\theta) \).
\( A_n = \frac{c^{n}}{\pi} \int_{0}^{2 \pi} f(\theta) \cos n \theta \, d\theta \) and \( B_n = \frac{c^{n}}{\pi} \int_{0}^{2 \pi} f(\theta) \sin n \theta \, d\theta \) are integrals that identify how much of the function can be expressed as a combination of these harmonics. Integral calculus in Fourier analysis provides a systematic method to dissect and reconstruct periodic functions, enabling us to comprehensively describe and analyze situations characterized by repetitive patterns.
- The coefficients \( A_0, A_n, \) and \( B_n \) involve integrals which help in projecting the original function onto basis functions such as cosine and sine functions.
Other exercises in this chapter
Problem 1
Referring to the solution of Example 1 in the text we have $$ R(r)=c_{1} J_{0}\left(\alpha_{n} r\right) \quad \text { and } \quad T(t)=c_{3} \cos a \alpha_{n} t
View solution Problem 6
Referring to Example 1 in the text we have \\[R(r)=c_{1} r^{n} \quad \text { and } \quad \Theta(\theta)=P_{n}(\cos \theta)\\] Now \(\Theta(\pi / 2)=0\) implies
View solution Problem 8
Referring to Example 1 in the text we have \\[R(r)=c_{1} r^{n}+c_{2} r^{-(n-1)} \quad \text { and } \quad \Theta(\theta)=P_{n}(\cos \theta)\\] since we expect \
View solution Problem 10
Letting \(u(r, t)=u(r, t)+\psi(r)\) we obtain \(r \psi^{\prime \prime}+\psi^{\prime}=-\beta r .\) The general solution of this nonhomogeneous CauchyEuler equati
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