Edpmétodo De Separacion De Variables Ejercicios

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penangjazz

Nov 28, 2025 · 11 min read

Edpmétodo De Separacion De Variables Ejercicios
Edpmétodo De Separacion De Variables Ejercicios

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    Absolutely! Here's a comprehensive article on the method of separation of variables for solving partial differential equations, complete with exercises:

    Separation of Variables: A Powerful PDE-Solving Technique

    The separation of variables is a cornerstone technique in the world of partial differential equations (PDEs). Its elegance lies in transforming a complex PDE into a set of simpler, ordinary differential equations (ODEs), which can then be solved using well-established methods. This approach has broad applications in physics, engineering, and various other fields where PDEs arise.

    When to Use Separation of Variables

    This method is most effective when dealing with linear, homogeneous PDEs in a domain where the boundary conditions are also linear and homogeneous. The basic idea is to assume that the solution of the PDE can be expressed as a product of functions, each depending on only one independent variable. This assumption, when substituted back into the PDE, hopefully leads to the separation of variables into distinct equations for each variable.

    The Essence of Separation: A Step-by-Step Guide

    Let's break down the process of solving a PDE using separation of variables into manageable steps:

    1. Assume a Product Solution:

      Suppose we have a PDE involving two independent variables, x and t, and a dependent variable u(x, t). We start by assuming that the solution u(x, t) can be written as a product of two functions, one depending only on x and the other only on t:

      u(x, t) = X(x)T(t)

      This is the critical initial assumption that enables the separation of variables.

    2. Substitute into the PDE:

      Next, substitute this assumed product solution into the original PDE. This will involve calculating the necessary partial derivatives of u(x, t) with respect to x and t and then substituting these into the PDE.

    3. Separate the Variables:

      After substitution, the goal is to manipulate the equation so that all terms involving x are on one side of the equation and all terms involving t are on the other side. This may require some algebraic manipulation. The key observation is that if you have an equation of the form:

      f(x) = g(t)

      where f(x) is a function of x only and g(t) is a function of t only, then both sides of the equation must be equal to a constant. This constant is often denoted by λ and is called the separation constant.

    4. Solve the ODEs:

      The separation process will yield two or more ODEs, each involving only one independent variable. Solve these ODEs using standard techniques. The general solutions will involve arbitrary constants.

    5. Apply Boundary Conditions:

      Apply the given boundary conditions to determine the values of the arbitrary constants in the solutions of the ODEs. This step is crucial for finding the particular solution that satisfies the specific problem.

    6. Construct the General Solution:

      The solutions obtained in the previous steps are often referred to as eigenfunctions. The general solution of the PDE is usually expressed as a linear combination (sum) of these eigenfunctions. This linear combination will involve another set of arbitrary constants.

    7. Apply Initial Conditions (if applicable):

      If the PDE is an initial value problem, apply the given initial conditions to determine the values of the remaining arbitrary constants in the general solution. This will give the final solution to the PDE that satisfies both the boundary and initial conditions.

    Exercises to Master the Technique

    Let's dive into some exercises to solidify your understanding of separation of variables.

    Exercise 1: The Heat Equation

    Consider the one-dimensional heat equation:

    u/∂t = α² ∂²u/∂x²

    where u(x, t) represents the temperature at position x and time t, and α² is the thermal diffusivity.

    • Domain: 0 < x < L, t > 0
    • Boundary Conditions: u(0, t) = 0, u(L, t) = 0 (temperature is fixed at both ends)
    • Initial Condition: u(x, 0) = f(x) (initial temperature distribution)

    Solution:

    1. Assume a Product Solution:

      u(x, t) = X(x)T(t)

    2. Substitute into the Heat Equation:

      X(x)T'(t) = α² X''(x)T(t)

    3. Separate the Variables:

      Divide both sides by X(x)T(t):

      T'(t) / T(t) = α² X''(x) / X(x)

      Since the left side depends only on t and the right side depends only on x, both sides must be equal to a constant, say −λ²:

      T'(t) / T(t) = α² X''(x) / X(x) = −λ²

      This gives us two ODEs:

      • T'(t) + λ²T(t) = 0
      • X''(x) + (λ²/α²)X(x) = 0
    4. Solve the ODEs:

      • The general solution for T(t) is T(t) = A e^(−λ²t), where A is a constant.
      • The general solution for X(x) is X(x) = B cos(λx/α) + C sin(λx/α), where B and C are constants.
    5. Apply Boundary Conditions:

      • u(0, t) = X(0)T(t) = 0 implies X(0) = 0, so B = 0.
      • u(L, t) = X(L)T(t) = 0 implies X(L) = 0, so C sin(λL/α) = 0. To avoid the trivial solution C = 0, we must have sin(λL/α) = 0, which means λL/α = nπ, where n is an integer. Thus, λ = nπα/L.

      Therefore, the solutions for X(x) are:

      X_n(x) = C_n sin(nπx/L)

      And the solutions for T(t) are:

      T_n(t) = A_n e^(−(nπα/L)²t)

    6. Construct the General Solution:

      The general solution is a linear combination of the product solutions:

      u(x, t) = Σ [C_n A_n sin(nπx/L) e^(−(nπα/L)²t)] (sum from n = 1 to infinity)

      We can combine the constants C_n and A_n into a single constant B_n:

      u(x, t) = Σ [B_n sin(nπx/L) e^(−(nπα/L)²t)] (sum from n = 1 to infinity)

    7. Apply Initial Condition:

      u(x, 0) = f(x) = Σ [B_n sin(nπx/L)] (sum from n = 1 to infinity)

      To find B_n, we use Fourier series:

      B_n = (2/L) ∫[from 0 to L] f(x) sin(nπx/L) dx

      This integral gives the coefficients B_n that determine the specific solution for the given initial condition f(x).

    Exercise 2: The Wave Equation

    Consider the one-dimensional wave equation:

    ∂²u/∂t² = c² ∂²u/∂x²

    where u(x, t) represents the displacement of a string at position x and time t, and c is the wave speed.

    • Domain: 0 < x < L, t > 0
    • Boundary Conditions: u(0, t) = 0, u(L, t) = 0 (ends of the string are fixed)
    • Initial Conditions: u(x, 0) = f(x) (initial displacement), ∂u/∂t(x, 0) = g(x) (initial velocity)

    Solution:

    1. Assume a Product Solution:

      u(x, t) = X(x)T(t)

    2. Substitute into the Wave Equation:

      X(x)T''(t) = c² X''(x)T(t)

    3. Separate the Variables:

      Divide both sides by X(x)T(t):

      T''(t) / T(t) = c² X''(x) / X(x)

      Set both sides equal to a constant, −λ²:

      T''(t) / T(t) = c² X''(x) / X(x) = −λ²

      This gives us two ODEs:

      • T''(t) + λ²T(t) = 0
      • X''(x) + (λ²/c²)X(x) = 0
    4. Solve the ODEs:

      • The general solution for T(t) is T(t) = A cos(λt) + B sin(λt), where A and B are constants.
      • The general solution for X(x) is X(x) = C cos(λx/c) + D sin(λx/c), where C and D are constants.
    5. Apply Boundary Conditions:

      • u(0, t) = X(0)T(t) = 0 implies X(0) = 0, so C = 0.
      • u(L, t) = X(L)T(t) = 0 implies X(L) = 0, so D sin(λL/c) = 0. To avoid the trivial solution D = 0, we must have sin(λL/c) = 0, which means λL/c = nπ, where n is an integer. Thus, λ = nπc/L.

      Therefore, the solutions for X(x) are:

      X_n(x) = D_n sin(nπx/L)

      And the solutions for T(t) are:

      T_n(t) = A_n cos(nπct/L) + B_n sin(nπct/L)

    6. Construct the General Solution:

      The general solution is a linear combination of the product solutions:

      *u(x, t) = Σ [sin(nπx/L) (A_n cos(nπct/L) + B_n sin(nπct/L))] * (sum from n = 1 to infinity)

    7. Apply Initial Conditions:

      • u(x, 0) = f(x) = Σ [A_n sin(nπx/L)] (sum from n = 1 to infinity)

        This is a Fourier sine series for f(x), so

        A_n = (2/L) ∫[from 0 to L] f(x) sin(nπx/L) dx

      • u/∂t(x, 0) = g(x) = Σ [B_n (nπc/L) sin(nπx/L)] (sum from n = 1 to infinity)

        This is a Fourier sine series for g(x), so

        B_n (nπc/L) = (2/L) ∫[from 0 to L] g(x) sin(nπx/L) dx

        B_n = (2/(nπc)) ∫[from 0 to L] g(x) sin(nπx/L) dx

      The integrals for A_n and B_n give the coefficients that determine the specific solution for the given initial displacement f(x) and initial velocity g(x).

    Exercise 3: Laplace's Equation in a Rectangle

    Consider Laplace's equation:

    ∂²u/∂x² + ∂²u/∂y² = 0

    where u(x, y) represents the potential in a two-dimensional region.

    • Domain: 0 < x < a, 0 < y < b
    • Boundary Conditions:
      • u(0, y) = 0
      • u(a, y) = 0
      • u(x, 0) = 0
      • u(x, b) = f(x)

    Solution:

    1. Assume a Product Solution:

      u(x, y) = X(x)Y(y)

    2. Substitute into Laplace's Equation:

      X''(x)Y(y) + X(x)Y''(y) = 0

    3. Separate the Variables:

      Divide by X(x)Y(y):

      X''(x) / X(x) + Y''(y) / Y(y) = 0

      X''(x) / X(x) = −Y''(y) / Y(y) = −λ²

      This gives us two ODEs:

      • X''(x) + λ²X(x) = 0
      • Y''(y) - λ²Y(y) = 0
    4. Solve the ODEs:

      • The general solution for X(x) is X(x) = A cos(λx) + B sin(λx), where A and B are constants.
      • The general solution for Y(y) is Y(y) = C cosh(λy) + D sinh(λy), where C and D are constants.
    5. Apply Boundary Conditions:

      • u(0, y) = X(0)Y(y) = 0 implies X(0) = 0, so A = 0.
      • u(a, y) = X(a)Y(y) = 0 implies X(a) = 0, so B sin(λa) = 0. To avoid the trivial solution B = 0, we must have sin(λa) = 0, which means λa = nπ, where n is an integer. Thus, λ = nπ/a.
      • u(x, 0) = X(x)Y(0) = 0 implies Y(0) = 0, so C = 0.

      Therefore, the solutions for X(x) are:

      X_n(x) = B_n sin(nπx/a)

      And the solutions for Y(y) are:

      Y_n(y) = D_n sinh(nπy/a)

    6. Construct the General Solution:

      The general solution is a linear combination of the product solutions:

      *u(x, y) = Σ [sin(nπx/a) sinh(nπy/a)] * (sum from n = 1 to infinity)

    7. Apply the Remaining Boundary Condition:

      u(x, b) = f(x) = Σ [E_n sin(nπx/a) sinh(nπb/a)] (sum from n = 1 to infinity), where E_n = B_n * D_n.

      Then

      E_n = (2/a) ∫[from 0 to a] f(x) sin(nπx/a) dx

      The final solution is:

      u(x, y) = Σ [(2/a) ∫[from 0 to a] f(x) sin(nπx/a) dx sin(nπx/a) sinh(nπy/a)] (sum from n = 1 to infinity)

    Key Considerations and Challenges

    While separation of variables is a powerful technique, it's essential to be aware of its limitations:

    • Linearity and Homogeneity: The method typically applies to linear, homogeneous PDEs with linear, homogeneous boundary conditions.
    • Domain Geometry: The method is most effective for PDEs defined on rectangular or circular domains where the boundaries align with the coordinate system.
    • Superposition: The general solution is often constructed by superposing (adding) a series of product solutions. Convergence of this series must be verified.
    • Non-constant Coefficients: If the coefficients in the PDE are not constant, separation of variables may not be possible.

    Conclusion

    Separation of variables is a fundamental and versatile technique for solving PDEs. By transforming a PDE into a set of ODEs, it provides a systematic approach to finding solutions for a wide range of problems in science and engineering. With practice and a clear understanding of the underlying principles, you can master this powerful tool and unlock the solutions to many complex PDE problems. Remember to always carefully consider the boundary conditions and initial conditions, as they play a critical role in determining the specific solution to the problem.

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