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Symmetries of the Helmholtz Equations

It is easy to see that if

$\displaystyle (\nabla^2+k^2)\psi =0
$

then

$\displaystyle X_{a\ast}\psi\,,~~Y_{b\ast}\psi~~\textrm{and}~~R_{\gamma\ast}\psi
$

are also solutions to the Hermholtz equation. In other words,

$\displaystyle (\nabla^2+k^2)(X_a\psi )=0\,,~~\textrm{etc.}
$

This is because the partial derivative can be interchanged and the coefficient of $ \nabla^2$ are independent of $ x$ , $ y$ , and $ \theta $ . One refers to this independence by saying that $ x$ , $ y$ and $ \theta $ are cyclic coordinates, or equivalently, that $ X_{a\ast}$ , $ Y_{b\ast}$ , and $ R_{\gamma\ast}$ are symmetries of $ \nabla^2$ .

This independence implies that the eigenspace of $ \nabla^2$ is invariant under $ X_{a*}$ , $ Y_{b*}$ , and also $ R_{\gamma*}$ . This is a very powerful result. It says that if $ \psi $ is a solution, then one obtains the additional solutions

$\displaystyle X_{a*}\psi,~~Y_{b*}\psi, ~~\textrm{and}~~R_{\gamma*}\psi~~,
$

which are parametrized by the translation parameter $ a$ and $ b$ , and by the angle $ \gamma$ respectively.


next up previous contents index
Next: Wanted: Rotation Invariant Solutions Up: The Helmholtz Equation Previous: Translations and Rotations in   Contents   Index
Ulrich Gerlach 2007-04-05