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4.2.2 Discretization of the Thermal Equation
For convenience, the thermal equation (3.72) is rewritten here as
|
(4.33) |
where the notation
is used.
Following the same procedure as for Laplace's equation, one multiplies (4.33) by
and integrates over the domain
, which together with Green's formula (4.26) and a Neumann boundary condition yields the weak formulation
|
(4.34) |
The thermal equation (4.33) corresponds to a parabolic problem. Besides the spatial discretization, a discretization in time has also to be performed. A simple choice is the backward Euler method
|
(4.35) |
where
is the time step. Applying now the spatial discretization for the temperature variable
|
(4.36) |
and the electric potential discretization (4.29), equation (4.34) is written for a single element as
|
|
|
|
|
(4.37) |
Using the integral notations (4.31),
|
(4.38) |
and
(4.37) can be expressed as
|
|
|
(4.40) |
This is the discrete system of equations, which has to be solved each time step in order to obtain the temperature at each node of the element.
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Up: 4.2 Discretization of the
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R. L. de Orio: Electromigration Modeling and Simulation