🧮Physical Sciences Math Tools Unit 11 – PDEs and Separation of Variables
Partial Differential Equations (PDEs) are mathematical models describing systems that change with respect to multiple variables, like space and time. They're essential in physics, engineering, and other sciences for modeling complex phenomena such as heat transfer, fluid dynamics, and quantum mechanics.
This unit covers the types of PDEs, boundary and initial conditions, and the separation of variables method for solving linear PDEs. It also explores applications in physical sciences, common challenges, and practical problem-solving techniques for various PDE scenarios.
Require initial conditions and boundary conditions
Linear PDEs: Coefficients and unknown function appear linearly (e.g., a∂x2∂2u+b∂y2∂2u=f(x,y))
Nonlinear PDEs: Coefficients or unknown function appear nonlinearly (e.g., ∂t∂u+u∂x∂u=0)
Boundary and Initial Conditions
Boundary conditions specify the behavior of the solution at the edges of the domain
Dirichlet boundary condition: Prescribes the value of the function on the boundary (e.g., u(0,t)=0)
Neumann boundary condition: Prescribes the value of the normal derivative on the boundary (e.g., ∂x∂u(L,t)=0)
Robin (mixed) boundary condition: Linear combination of function value and normal derivative (e.g., αu+β∂x∂u=γ)
Initial conditions specify the state of the system at the initial time (e.g., u(x,0)=f(x))
Well-posed problems require sufficient boundary and initial conditions to ensure existence, uniqueness, and stability of the solution
Homogeneous boundary conditions: Zero function value or zero normal derivative on the boundary
Inhomogeneous boundary conditions: Non-zero function value or non-zero normal derivative on the boundary
Separation of Variables Method
Powerful technique for solving linear, homogeneous PDEs with homogeneous boundary conditions
Assumes the solution can be written as a product of functions, each depending on a single variable (e.g., u(x,t)=X(x)T(t))
Substituting the separated solution into the PDE leads to ordinary differential equations (ODEs) for each variable
ODEs are solved using standard techniques (integration, eigenvalue problems) and combined to obtain the general solution
Boundary and initial conditions are applied to determine the specific solution and arbitrary constants
Suitable for various geometries (rectangular, cylindrical, spherical) and coordinate systems (Cartesian, polar, spherical)
Eigenfunctions obtained from the separation of variables form a complete orthogonal basis for the solution space
Solving PDEs Step-by-Step
Identify the type of PDE (elliptic, parabolic, hyperbolic) and its order
Determine the domain and boundary conditions
If applicable, identify the initial condition(s)
Assume a separated solution in the form u(x1,x2,…,t)=X1(x1)X2(x2)…T(t)
Substitute the separated solution into the PDE and divide by the product of functions
Separate the equation into terms, each depending on a single variable
Equate each term to a separation constant (eigenvalue) to obtain ODEs
Solve the ODEs using appropriate techniques (integration, eigenvalue problems)
Apply boundary conditions to the spatial solutions to determine eigenfunctions and eigenvalues
Apply initial conditions to determine the time-dependent solution and arbitrary constants
Combine the spatial and temporal solutions to obtain the general solution
Verify that the solution satisfies the PDE, boundary conditions, and initial conditions
Applications in Physical Sciences
Heat transfer: Modeling temperature distribution in solids, fluids, and gases
Steady-state heat conduction (Laplace's equation)
Transient heat conduction (heat equation)
Fluid dynamics: Describing the motion of fluids and gases
Potential flow (Laplace's equation)
Navier-Stokes equations (momentum conservation)
Quantum mechanics: Modeling the behavior of particles at the atomic and subatomic scales
Schrödinger equation (wave function, energy states)
Dirac equation (relativistic quantum mechanics)
Electromagnetism: Describing electric and magnetic fields and their interactions
Poisson's equation (electrostatic potential)
Maxwell's equations (electromagnetic waves)
Elasticity: Modeling deformation and stress in solid materials
Navier-Cauchy equations (displacement, stress)
Plate and shell equations (thin structures)
Common Challenges and Tips
Identifying the appropriate coordinate system and separation of variables based on the geometry of the problem
Dealing with inhomogeneous boundary conditions or source terms
Use superposition principle for linear PDEs
Apply change of variables or Green's functions
Solving eigenvalue problems and determining eigenfunctions
Sturm-Liouville theory for self-adjoint operators
Orthogonality and completeness of eigenfunctions
Convergence and stability of numerical methods for PDEs
Courant-Friedrichs-Lewy (CFL) condition for explicit schemes
Implicit schemes for improved stability
Verifying the solution and checking for physical plausibility
Dimensional analysis and scaling arguments
Asymptotic behavior and limiting cases
Practice Problems and Examples
Solve the one-dimensional heat equation ∂t∂u=α∂x2∂2u with boundary conditions u(0,t)=0, u(L,t)=0, and initial condition u(x,0)=sin(Lπx).
Find the steady-state temperature distribution in a rectangular plate with dimensions a×b, governed by Laplace's equation ∂x2∂2u+∂y2∂2u=0, and boundary conditions u(0,y)=0, u(a,y)=100, ∂y∂u(x,0)=0, ∂y∂u(x,b)=0.
Solve the wave equation ∂t2∂2u=c2∂x2∂2u for a vibrating string of length L with boundary conditions u(0,t)=0, u(L,t)=0, and initial conditions u(x,0)=sin(Lπx), ∂t∂u(x,0)=0.
Determine the electrostatic potential V(r,θ) inside a hollow conducting sphere of radius R with a charge distribution ρ(r,θ)=ρ0cos(θ), governed by Poisson's equation r21∂r∂(r2∂r∂V)+r2sin(θ)1∂θ∂(sin(θ)∂θ∂V)=−ε0ρ(r,θ) and boundary condition V(R,θ)=0.