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Heat Equation
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Initial condition given by a delta function
For an initial heat distribution localized at a point, use a Green's function approach, where the solution is built up from the fundamental solution corresponding to that point heat source.
Mixed boundary conditions
Solving the heat equation with one end held at a constant temperature (Dirichlet) and the other insulated (Neumann), leads to a mixed series solution, often involving sine and cosine functions or modified sine series.
Robin (third type) boundary conditions
Robin boundary conditions which involve a linear combination of temperature and flux can lead to solutions that use eigenfunctions satisfying associated Sturm-Liouville problems.
Initial condition as a Fourier sine series
The initial condition must be expanded as a Fourier sine series to match the eigenfunctions derived from the homogeneous boundary conditions.
Initial condition as a Fourier cosine series
If Neumann boundary conditions are used, then the initial condition can often be represented by a Fourier cosine series consistent with these boundary conditions.
Periodic boundary conditions
Periodic conditions assume the ends of the domain are connected, leading to a continuous and differentiable temperature profile that calls for a Fourier series solution involving both sines and cosines.
Homogeneous Neumann boundary conditions
Solution involves cosine series as the eigenfunctions, reflecting no heat flux at the ends, implying .
Non-homogeneous Neumann boundary conditions
A non-trivial flux at the boundaries complicates the problem. Just like with Dirichlet conditions, seek a steady solution plus a transient solution with homogeneous Neumann conditions.
Non-homogeneous Dirichlet boundary conditions
Non-zero boundary conditions mean we may need to split the solution into a steady part and a transient part, where the steady part satisfies the static heat equation.
Homogeneous boundary conditions at both ends of a rod
Solution form assumes , and the boundary conditions lead to a sine series solution for . The time-dependent part is an exponential decay.
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