Difference between revisions of "Eigenfunctions for a Uniform Free Beam"
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<math>C_1 = C_3 = 0 \Rightarrow w_n(x) = C_2 \cos(\lambda_n x) + C_4 \cosh(\lambda_n x)</math> | <math>C_1 = C_3 = 0 \Rightarrow w_n(x) = C_2 \cos(\lambda_n x) + C_4 \cosh(\lambda_n x)</math> | ||
</center> | </center> | ||
− | By imposing boundary conditions at <math>x = | + | By imposing boundary conditions at <math>x = L</math> : |
<center> | <center> | ||
<math> | <math> | ||
\begin{bmatrix} | \begin{bmatrix} | ||
− | - \cos(\lambda_n l)&\cosh(\lambda_n | + | - \cos(\lambda_n l)&\cosh(\lambda_n L)\\ |
− | \sin(\lambda_n l)&\sinh(\lambda_n | + | \sin(\lambda_n l)&\sinh(\lambda_n L)\\ |
\end{bmatrix} | \end{bmatrix} | ||
\begin{bmatrix} | \begin{bmatrix} | ||
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For a nontrivial solution one gets: | For a nontrivial solution one gets: | ||
<center> | <center> | ||
− | <math>\tan(\lambda_n | + | <math>\tan(\lambda_n L)+\tanh(\lambda_n L)=0\,</math> |
</center> | </center> | ||
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<center> | <center> | ||
− | <math>\lambda_0 | + | <math>\lambda_0 L = 0, \lambda_2 L = 2.365, \lambda_4 L = 5.497\,</math> |
</center> | </center> | ||
− | |||
− | |||
− | |||
− | |||
Symmetric natural modes can be written in normalized form as : | Symmetric natural modes can be written in normalized form as : | ||
<center> | <center> | ||
− | <math>w_n(x) = \frac{1}{2}\left( \frac{\cos(\lambda_n x)}{\cos(\lambda_n | + | <math>w_n(x) = \frac{1}{2}\left( \frac{\cos(\lambda_n x)}{\cos(\lambda_n L)}+\frac{\cosh(\lambda_n x)}{\cosh(\lambda_n L)} \right ) |
</math> | </math> | ||
</center> | </center> |
Revision as of 08:37, 7 November 2008
Introduction
We show here how to find the eigenfunction for a beam with free edge conditions.
Equations
We can find a the eigenfunction which satisfy
[math]\displaystyle{ \partial_x^4 w_n = \lambda_n^4 w_n \,\,\, -L \leq x \leq L }[/math]
plus the edge conditions of zero bending moment and shear stress
Solution
General solution of the differential equation is :
[math]\displaystyle{ w_n(x) = C_1 \sin(\lambda_n x) + C_2 \cos(\lambda_n x) + C_3 \sinh(\lambda_n x) + C_4 \cosh(\lambda_n x)\, }[/math]
Due to symmetry of the problem, dry natural vibrations of a free beam can be split into two different sets of modes, symmetric (even) modes and skew-symmetric (odd) modes.
Symmetric modes
[math]\displaystyle{ C_1 = C_3 = 0 \Rightarrow w_n(x) = C_2 \cos(\lambda_n x) + C_4 \cosh(\lambda_n x) }[/math]
By imposing boundary conditions at [math]\displaystyle{ x = L }[/math] :
[math]\displaystyle{ \begin{bmatrix} - \cos(\lambda_n l)&\cosh(\lambda_n L)\\ \sin(\lambda_n l)&\sinh(\lambda_n L)\\ \end{bmatrix} \begin{bmatrix} C_2\\ C_4\\ \end{bmatrix} = \begin{bmatrix} 0\\ 0\\ \end{bmatrix} }[/math]
For a nontrivial solution one gets:
[math]\displaystyle{ \tan(\lambda_n L)+\tanh(\lambda_n L)=0\, }[/math]
The first three roots are :
[math]\displaystyle{ \lambda_0 L = 0, \lambda_2 L = 2.365, \lambda_4 L = 5.497\, }[/math]
Symmetric natural modes can be written in normalized form as :
[math]\displaystyle{ w_n(x) = \frac{1}{2}\left( \frac{\cos(\lambda_n x)}{\cos(\lambda_n L)}+\frac{\cosh(\lambda_n x)}{\cosh(\lambda_n L)} \right ) }[/math]
Skew-symmetric modes
[math]\displaystyle{ C_2 = C_4 = 0 \Rightarrow w_n(x) = C_1 \sin(\lambda_n x) + C_3 \sinh(\lambda_n x) }[/math]
By imposing boundary conditions at [math]\displaystyle{ x = l }[/math] :
[math]\displaystyle{ \begin{bmatrix} - \sin(\lambda_n l)&\sinh(\lambda_n l)\\ -\cos(\lambda_n l)&\cosh(\lambda_n l)\\ \end{bmatrix} \begin{bmatrix} C_1\\ C_3\\ \end{bmatrix} = \begin{bmatrix} 0\\ 0\\ \end{bmatrix} }[/math]
For a nontrivial solution one gets:
[math]\displaystyle{ -\tan(\lambda_n l)+\tanh(\lambda_n l)=0\, }[/math]
The first three roots are :
[math]\displaystyle{ \lambda_1 l = 0, \lambda_3 l = 3.925, \lambda_5 l = 7.068\, }[/math]
Skew-symmetric natural modes can be written in normalized form as :
[math]\displaystyle{ w_n(x) = \frac{1}{2}\left( \frac{\sin(\lambda_n x)}{\sin(\lambda_n l)}+\frac{\sinh(\lambda_n x)}{\sinh(\lambda_n l)} \right ) }[/math]
Natural Frequencies
The equation in the time domain for a beam is
[math]\displaystyle{ m\partial_t^2 w + EI \partial_x^4 w }[/math]
so that, having obtained eigenvalues [math]\displaystyle{ \lambda_n }[/math], the natural frequency can be readily calculated :
[math]\displaystyle{ \omega_n = \frac{(\lambda_n l)^2}{l^2}\sqrt\frac{EI}{m} }[/math]