Problem 14
Question
Use the Laplace transform to solve the heat equation \(u_{x x}=u_{t}, x>0, t>0\) subject to the given conditions. $$ \left.\frac{\partial u}{\partial x}\right|_{x=0}=u(0, t)-50, \quad \lim _{x \rightarrow \infty} u(x, t)=0, \quad u(x, 0)=0 $$
Step-by-Step Solution
Verified Answer
The solution is \( u(x, t) = 50 e^{-(x^2/(4t))} \text{erfc} \left( \frac{x}{2\sqrt{t}} \right) \).
1Step 1: Identify the Equation and Conditions
The heat equation is given by the partial differential equation (PDE) \( u_{xx} = u_t \). We have boundary conditions: \( \frac{\partial u}{\partial x}\big|_{x=0} = u(0, t) - 50 \), \( \lim_{x \rightarrow \infty} u(x, t) = 0 \), and the initial condition \( u(x, 0) = 0 \).
2Step 2: Apply Laplace Transform in Time Domain
Take the Laplace transform of the heat equation with respect to time \( t \), which transforms \( u(x, t) \) into \( U(x, s) \). This gives us \( \mathcal{L}\{u_t\} = sU(x, s) - u(x, 0) = sU(x, s) \) because \( u(x, 0) = 0 \). So, the equation becomes \( u_{xx} = sU(x, s) \).
3Step 3: Solve the Transformed Equation
The transformed equation \( u_{xx} = sU(x, s) \) is a second-order ordinary differential equation (ODE). The general solution for this ODE is \( U(x, s) = A e^{-\sqrt{s}x} + B e^{\sqrt{s}x} \).
4Step 4: Apply Boundary Conditions at Infinity
Apply the boundary condition \( \lim_{x \rightarrow \infty} u(x, t) = 0 \). Since \( e^{\sqrt{s}x} \) grows without bound as \( x \to \infty \), we must have \( B = 0 \) to satisfy this condition. Thus \( U(x, s) = A e^{-\sqrt{s}x} \).
5Step 5: Apply Boundary Condition at x=0
Use the boundary condition \( \frac{\partial u}{\partial x}\big|_{x=0} = u(0,t) - 50 \). In the Laplace domain, \( U_x(x, s) = -A\sqrt{s}e^{-\sqrt{s}x} \). At \( x = 0 \), \( U_x(0, s) = -A\sqrt{s} = U(0, s) - \frac{50}{s} \). Since \( U(0, s) = A \), this gives: \(-A\sqrt{s} = A - \frac{50}{s} \).
6Step 6: Solve for Coefficient A
Solving the equation \(-A\sqrt{s} = A - \frac{50}{s} \) for \( A \), we have:\[ A + A\sqrt{s} = \frac{50}{s} \]\[ A(1 + \sqrt{s}) = \frac{50}{s} \]\[ A = \frac{50}{s(1 + \sqrt{s})} \].
7Step 7: Invert the Laplace Transform
Substitute \( A = \frac{50}{s(1 + \sqrt{s})} \) back into \( U(x, s) = A e^{-\sqrt{s}x} \) to get:\[ U(x, s) = \frac{50}{s(1 + \sqrt{s})} e^{-\sqrt{s}x} \]Now invert the Laplace transform to find \( u(x, t) \). Recognize \( \frac{50}{s(1 + \sqrt{s})} e^{-\sqrt{s}x} \) as a convolution which can be evaluated using standard Laplace inverse techniques and tables.
8Step 8: Compute the Inverse Transform
Recognizing \( \frac{1}{s(1 + \sqrt{s})} \) relates to a convolution involving exponential and complementary error function terms, compute \( u(x, t) \) using standard results. The inversion yields:\[ u(x, t) = 50 e^{-(x^2/(4t))} \text{erfc} \left( \frac{x}{2\sqrt{t}} \right) \], where \( \text{erfc} \) is the complementary error function.
Key Concepts
Heat EquationPartial Differential EquationBoundary ConditionsComplementary Error Function
Heat Equation
The heat equation is a classic example of a partial differential equation (PDE) used to describe how heat diffuses through a given region over time. In one dimension, it is expressed as \( u_{xx} = u_t \). This equation signifies that the second spatial derivative equals the first time derivative, reflecting how temperature changes with respect to space and time.
Heat equations are crucial in physics and engineering, modeling heat distribution, and even financial mathematics in certain contexts.
By solving the heat equation, we can predict temperature variations and understand thermal behavior.
Heat equations are crucial in physics and engineering, modeling heat distribution, and even financial mathematics in certain contexts.
By solving the heat equation, we can predict temperature variations and understand thermal behavior.
- The primary purpose: to model the conduction of heat.
- This PDE is used in various fields: physics, geometry, and beyond.
Partial Differential Equation
Partial Differential Equations (PDEs) are equations that include partial derivatives and involve functions of several variables. The heat equation, \( u_{xx} = u_t \), is a simple yet powerful PDE example.
PDEs serve as mathematical descriptions of various physical systems and phenomena. Understanding PDEs allows us to model complex behavior like temperature distribution (heat) or wave propagation (acoustics).
PDEs serve as mathematical descriptions of various physical systems and phenomena. Understanding PDEs allows us to model complex behavior like temperature distribution (heat) or wave propagation (acoustics).
- Consist of partial derivatives with respect to multiple variables.
- Applications span physics, engineering, and beyond.
- Examples include heat equation, wave equation, and Laplace's equation.
Boundary Conditions
Boundary conditions are essential in solving PDEs as they define the limits within which a solution exists. For the heat equation, we need to know what's happening at the boundaries to find a solution.
There are several types of boundary conditions:
- \( \lim_{x \rightarrow \infty} u(x, t) = 0 \) means the temperature approaches zero at infinity.
- Neumann boundary at \( x=0 \) relates to how heat flux is linked to temperature initially.
By using these conditions, solutions for the PDE can be narrowed down and determined accurately.
There are several types of boundary conditions:
- Dirichlet Conditions: Specify the function's value at the boundary, like \( u(x, 0) = 0 \).
- Neumann Conditions: Involve the derivative's value at the boundary, such as \( \frac{\partial u}{\partial x}\big|_{x=0} = u(0, t) - 50 \).
- \( \lim_{x \rightarrow \infty} u(x, t) = 0 \) means the temperature approaches zero at infinity.
- Neumann boundary at \( x=0 \) relates to how heat flux is linked to temperature initially.
By using these conditions, solutions for the PDE can be narrowed down and determined accurately.
Complementary Error Function
The complementary error function, denoted as \( \text{erfc}(x) \), is a special function related to the Gaussian error function \( \text{erf}(x) \). It's useful in probability, statistics, and partial differential equations, particularly solutions involving diffusion processes.
The complementary error function is defined as:
\[ \text{erfc}(x) = 1 - \text{erf}(x) = \frac{2}{\sqrt{\pi}} \int_{x}^{\infty} e^{-t^2} \, dt \]
In the context of the heat equation, \( \text{erfc}(x) \) often appears when solving diffusion-related PDEs using methods like the Laplace or Fourier transforms.
The complementary error function is defined as:
\[ \text{erfc}(x) = 1 - \text{erf}(x) = \frac{2}{\sqrt{\pi}} \int_{x}^{\infty} e^{-t^2} \, dt \]
In the context of the heat equation, \( \text{erfc}(x) \) often appears when solving diffusion-related PDEs using methods like the Laplace or Fourier transforms.
- It represents the tail probability of the Gaussian distribution.
- Commonly appears in solutions to the heat equation.
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