Difference between revisions of "Example Calculations for the KdV and IST"
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where <math>\nu</math> is an appropriate constant to make the function increase in value | where <math>\nu</math> is an appropriate constant to make the function increase in value | ||
sufficiently rapidly but not too rapidly. | sufficiently rapidly but not too rapidly. | ||
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+ | {| class="wikitable" | ||
+ | |- | ||
+ | ! Animation | ||
+ | ! Three-dimensional plot. | ||
+ | |- | ||
+ | | [[Image:Wide_function.gif|thumb|right|500px|Evolution of <math>u(x,t)</math>.]] | ||
+ | | [[Image:Widefunction.jpg|thumb|right|500px|Evolution of <math>u(x,t)</math> ]] | ||
+ | |||
+ | |} |
Revision as of 10:57, 23 September 2010
Nonlinear PDE's Course | |
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Current Topic | Example Calculations for the KdV and IST |
Next Topic | Connection betwen KdV and the Schrodinger Equation |
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Example1 Delta function potential.
We have already calculated the scattering data for the delta function potential. The scattering data is
The spectral data evolves as
so that
Example 2 A Hat Function
We solve for the case when
For this case we need to solve
which has solution and
which has solution.
Recall that the solitons have amplitude [math]\displaystyle{ 2k_{n}^{2} }[/math] or [math]\displaystyle{ -2\lambda_{n} }[/math]. This can be seen in the height of the solitary waves.
We cannot work with a hat function numerically, because the jump in [math]\displaystyle{ u }[/math] leads to high frequencies which dominate the response.. We can smooth our function by a number of methods. We use here the function [math]\displaystyle{ \tanh\left( x\right) }[/math] so we write
where [math]\displaystyle{ \nu }[/math] is an appropriate constant to make the function increase in value sufficiently rapidly but not too rapidly.
Animation | Three-dimensional plot. |
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