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5.2 Heat Equation: Derivation and Solutions

3 min readjuly 22, 2024

The is a crucial tool in mathematical physics, describing how temperature changes over time in a material. It's derived from energy conservation and , connecting heat flux to temperature gradients.

Solving the heat equation involves techniques like and Fourier series. These methods allow us to find solutions for different geometries and boundary conditions, helping us understand heat transfer in various real-world scenarios.

Derivation and Fundamental Concepts

Derivation of heat equation

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  • Conservation of energy principle states change in internal energy of a system equals heat added minus work done by the system
    • In , work term is negligible since no significant mechanical work is performed
  • Fourier's law relates heat flux to negative temperature gradient
    • q=kTxq = -k \frac{\partial T}{\partial x}, where qq is heat flux (W/m²), kk is thermal conductivity (W/m·K), and Tx\frac{\partial T}{\partial x} is temperature gradient (K/m)
  • Continuity equation describes rate of change of temperature in terms of divergence of heat flux
    • ρcTt=q\rho c \frac{\partial T}{\partial t} = -\nabla \cdot q, where ρ\rho is density (kg/m³), cc is specific heat capacity (J/kg·K), and Tt\frac{\partial T}{\partial t} is rate of change of temperature (K/s)
  • Combining Fourier's law and continuity equation yields the heat equation
    • Tt=α2T\frac{\partial T}{\partial t} = \alpha \nabla^2 T, where α=kρc\alpha = \frac{k}{\rho c} is thermal diffusivity (m²/s) and 2\nabla^2 is the Laplacian operator

Solution Methods

Separation of variables for heat equation

  • Assume solution is a product of two functions: T(x,t)=X(x)τ(t)T(x, t) = X(x) \cdot \tau(t)
    • X(x)X(x) depends only on spatial variable xx
    • τ(t)\tau(t) depends only on time variable tt
  • Substituting this form into heat equation leads to two ordinary differential equations (ODEs)
    • XX=1αττ=λ\frac{X''}{X} = \frac{1}{\alpha} \frac{\tau'}{\tau} = -\lambda, where λ\lambda is separation constant (eigenvalue)
  • Spatial ODE X+λX=0X'' + \lambda X = 0 has solutions depending on sign of λ\lambda and boundary conditions
    • For λ>0\lambda > 0, solutions are sines and cosines (oscillatory)
    • For λ<0\lambda < 0, solutions are exponentials (growth or decay)
  • Temporal ODE τ+αλτ=0\tau' + \alpha \lambda \tau = 0 has exponential decay solution: τ(t)=eαλt\tau(t) = e^{-\alpha \lambda t}
  • General solution is linear combination of products of spatial and temporal solutions
    • T(x,t)=n=1CneαλntXn(x)T(x, t) = \sum_{n=1}^{\infty} C_n e^{-\alpha \lambda_n t} X_n(x), where CnC_n are constants determined by initial conditions and Xn(x)X_n(x) are eigenfunctions

Solutions in different geometries

  • Infinite domain (unbounded): Solution is Gaussian function that spreads and decays with time
    • T(x,t)=14παtex24αtT(x, t) = \frac{1}{\sqrt{4 \pi \alpha t}} e^{-\frac{x^2}{4 \alpha t}}, representing diffusion of initial heat distribution
  • Semi-infinite domain (bounded on one side): Solution combines infinite domain solution and its mirror image
    • Boundary condition at x=0x = 0 (fixed temperature or insulated) determines sign of mirror image
    • Represents heat transfer in a half-space (ground, thick wall)
  • Finite domain (bounded on both sides): Solution is Fourier series with coefficients determined by boundary conditions
    • : T(x)=C1x+C2T(x) = C_1 x + C_2, where C1C_1 and C2C_2 are constants (linear temperature profile)
    • : Exponential decay of Fourier modes with time (approach to steady-state)

Fourier series for boundary conditions

  • Fourier series represents periodic function as infinite sum of sines and cosines
    • f(x)=a02+n=1(ancos(nπxL)+bnsin(nπxL))f(x) = \frac{a_0}{2} + \sum_{n=1}^{\infty} \left(a_n \cos\left(\frac{n \pi x}{L}\right) + b_n \sin\left(\frac{n \pi x}{L}\right)\right), where LL is period and ana_n, bnb_n are Fourier coefficients
  • Fourier coefficients depend on boundary conditions
    • Dirichlet (fixed temperature): T(0,t)=T0T(0, t) = T_0, T(L,t)=TLT(L, t) = T_L lead to cosine series
    • Neumann (fixed heat flux): Tx(0,t)=q0\frac{\partial T}{\partial x}(0, t) = q_0, Tx(L,t)=qL\frac{\partial T}{\partial x}(L, t) = q_L lead to sine series
    • Mixed (combination of Dirichlet and Neumann) lead to mixed series
  • Substituting Fourier series into heat equation and solving for time-dependent coefficients yields
    • T(x,t)=n=1Cneαλntsin(nπxL)T(x, t) = \sum_{n=1}^{\infty} C_n e^{-\alpha \lambda_n t} \sin\left(\frac{n \pi x}{L}\right), where λn=(nπL)2\lambda_n = \left(\frac{n \pi}{L}\right)^2 are eigenvalues
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AP® and SAT® are trademarks registered by the College Board, which is not affiliated with, and does not endorse this website.

© 2024 Fiveable Inc. All rights reserved.
AP® and SAT® are trademarks registered by the College Board, which is not affiliated with, and does not endorse this website.
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