Difference between revisions of "Dispersion Relation for a Floating Elastic Plate"

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-\omega^2 \cosh(kH)  \, </math>
 
-\omega^2 \cosh(kH)  \, </math>
  
where <math>\beta = D/\rho</math>
+
where <math>\beta = D/(\rho g L^5)\,</math> and <math>\gamma = \rho_i h/(\rho L)\,</math>.
 +
Often the additional notation <math>\alpha = \omega^2\,</math> is used. This notation
 +
is based on [[Tayler_1986a|Tayler 1986]]
  
This reduces to the following form in the length parameter is set to  
+
This reduces to the following form if the length parameter is set to  
  
 
which is the method used in Chung and Fox.
 
which is the method used in Chung and Fox.

Revision as of 08:14, 16 May 2006

Separation of Variables

The dispersion equation arises when separating variables subject to the boundary conditions for a Floating Elastic Plate of infinite extent. The same equation arises when separating variables in two or three dimensions and we present here the two-dimensional version. The equations are described in detail in the Floating Elastic Plate page and we begin with the equations The equations of motion for the Frequency Domain Problem with radial frequency [math]\displaystyle{ \,\omega }[/math] in terms of the potential alone is

[math]\displaystyle{ D\frac{\partial^4}{\partial x^4} \frac{\partial \phi}{\partial z} + \left(\rho g - \omega^2 \rho_i h \right) \frac{\partial \phi}{\partial z} = - \rho \omega^2 \phi, \, z=0 }[/math]

plus the equations within the fluid

[math]\displaystyle{ \nabla^2\phi =0 }[/math]

[math]\displaystyle{ \frac{\partial \phi}{\partial z} = 0, \, z=-H }[/math]

where [math]\displaystyle{ \,g }[/math] is the acceleration due to gravity, [math]\displaystyle{ \,\rho_i }[/math] and [math]\displaystyle{ \,\rho }[/math] are the densities of the plate and the water respectively, [math]\displaystyle{ \,h }[/math] and [math]\displaystyle{ \,D }[/math] are the thickness and flexural rigidity of the plate.

We then look for a separation of variables solution to Laplace's Equation and obtain the following expression for the velocity potential

[math]\displaystyle{ \phi(x,z) = e^{ikx} \cosh k(z+H) \, }[/math]

If we then apply the condition at [math]\displaystyle{ z=0 }[/math] we see that the constant [math]\displaystyle{ \,k }[/math] (which corresponds to the wavenumber) is given by

[math]\displaystyle{ -D k^5 \sinh(kH) - k \left(\rho g - \omega^2 \rho_i h \right) \sinh(kH) = -\rho \omega^2 \cosh(kH) \, }[/math]

Solution of the dispersion equation

The dispersion equation was first solved by Fox and Squire 1994 and they determined that the solution consists of one real, two complex, and infinite number of imaginary roots plus their negatives. Interestingly the eigenfunctions form an over complete set for [math]\displaystyle{ L_2[-H,0]\, }[/math]. Also, there are some circumstances (non-physical) in which the complex roots become purely imaginary. The solution of this dispersion equation is far from trivial and the optimal solution method has been developed by Tim Williams and is described below.

Non-dimensional form

The dispersion equation is often given in non-dimensional form. The form used by Michael Meylan in many of his papers is to scale length with respect to [math]\displaystyle{ L\, }[/math] and time with respect to [math]\displaystyle{ \sqrt{L/g}\, }[/math]. The non-dimensional equations then become

[math]\displaystyle{ -\beta k^5 \sinh(kH) - k \left(1 - \omega^2 \gamma \right) \sinh(kH) = -\omega^2 \cosh(kH) \, }[/math]

where [math]\displaystyle{ \beta = D/(\rho g L^5)\, }[/math] and [math]\displaystyle{ \gamma = \rho_i h/(\rho L)\, }[/math]. Often the additional notation [math]\displaystyle{ \alpha = \omega^2\, }[/math] is used. This notation is based on Tayler 1986

This reduces to the following form if the length parameter is set to

which is the method used in Chung and Fox.

The most sophisticated form, which is due to Tim Williams and has certain theoretical and practical advantages, is the following,

[math]\displaystyle{ f(\gamma)=\cosh(\gamma H)-(\gamma^4+\varpi)\gamma\sinh(\gamma H)=0, }[/math]

where [math]\displaystyle{ H }[/math] is the nodimensional water depth, and

[math]\displaystyle{ \varpi=(1-k_\infty\sigma)/(k_\infty L),\quad k_\infty=\omega^2/g,\quad\sigma=\rho_ih/\rho,\quad L^5=D/(\rho\omega^2). }[/math]

[math]\displaystyle{ k_\infty }[/math] is the wave number for a wave traveling in open water of infinite depth, and [math]\displaystyle{ L\, }[/math] is the natural length that we have scaled length variables by. The dispersion relation relates the wavenumber [math]\displaystyle{ \gamma/L\, }[/math] and thus wave speed to the above parameters.