Note: THIS PAGE DESCRIBES THE LEGACY WORKFLOW. New features might not be compatible with the legacy workflow. For the corresponding step in the recommended workflow, see Equations You Can Solve Using Recommended Functions.
This toolbox applies to the following PDE type:
expressed in Ω, which we shall refer to as the elliptic equation, regardless of whether its coefficients and boundary conditions make the PDE problem elliptic in the mathematical sense. Analogously, we shall use the terms parabolic equation and hyperbolic equation for equations with spatial operators like the previous one, and first and second order time derivatives, respectively. Ω is a bounded domain in the plane or is a bounded 3-D region. c, a, f, and the unknown u are scalar, complex valued functions defined on Ω. c can be a matrix function on Ω (see c Coefficient for Systems). The software can also handle the parabolic PDE
the hyperbolic PDE
and the eigenvalue problem
where d is a complex valued function on Ω,
and λ is an unknown eigenvalue. For the parabolic
and hyperbolic PDE the coefficients c, a, f,
and d can depend on time, on the solution u,
and on its gradient ∇u. A nonlinear solver
pdenonlin) is available for the
nonlinear elliptic PDE
where c, a, and f are functions of the unknown solution u and of its gradient ∇u. The parabolic and hyperbolic equation solvers also solve nonlinear and time-dependent problems.
Note: Before solving a nonlinear elliptic PDE, from the Solve menu in the PDE app, select Parameters. Then, select the Use nonlinear solver check box and click OK.
For eigenvalue problems, the coefficients cannot depend on the
u or its gradient.
All solvers can handle the system case of N coupled equations. You can solve N = 1 or 2 equations using the PDE app, and any number of equations using command-line functions. For example, N = 2 elliptic equations:
For a description of N > 1 PDE systems and their coefficients, see Coefficients for Systems of PDEs.
For the elliptic problem, an adaptive mesh refinement algorithm is implemented. It can also be used in conjunction with the nonlinear solver. In addition, a fast solver for Poisson's equation on a rectangular grid is available.
The following boundary conditions are defined for scalar u:
Dirichlet: hu = r on the boundary ∂Ω.
Generalized Neumann: on ∂Ω.
is the outward unit normal. g, q, h, and r are complex-valued functions defined on ∂Ω. (The eigenvalue problem is a homogeneous problem, i.e., g = 0, r = 0.) In the nonlinear case, the coefficients g, q, h, and r can depend on u, and for the hyperbolic and parabolic PDE, the coefficients can depend on time. For the two-dimensional system case, Dirichlet boundary condition is
the generalized Neumann boundary condition is
and the mixed boundary condition is
where µ is computed such that the Dirichlet boundary condition is satisfied. Dirichlet boundary conditions are also called essential boundary conditions, and Neumann boundary conditions are also called natural boundary conditions.
For advanced, nonstandard applications you can transfer the description of domains, boundary conditions etc. to your MATLAB® workspace. From there you use Partial Differential Equation Toolbox™ functions for managing data on unstructured meshes. You have full access to the mesh generators, FEM discretizations of the PDE and boundary conditions, interpolation functions, etc. You can design your own solvers or use FEM to solve subproblems of more complex algorithms. See also Solve PDEs Programmatically.