Difference between revisions of "Eigenfunctions for a Uniform Free Beam"
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Having obtained eigenvalues <math>\lambda_n</math>, natural requency can be readily calculated : | Having obtained eigenvalues <math>\lambda_n</math>, natural requency can be readily calculated : | ||
<center> | <center> | ||
− | <math>\omega_n = \frac{(\lambda_n l)^2}{l^2}\sqrt\frac{EI}{m} | + | <math>\omega_n = \frac{(\lambda_n l)^2}{l^2}\sqrt\frac{EI}{m}</math> |
</center> | </center> | ||
− | Symmetrical natural modes can be written in normalized form | + | Symmetrical natural modes can be written in normalized form as : |
+ | <center> | ||
+ | <math>w_n = \frac{1}{2}(\frac{\cos(\lambda_n x)}{\cos(\lamda_n l)}+\frac{\cosh(\lambda_n x)}{\cosh(\lambda_n l)}) | ||
+ | </math> | ||
+ | </center> |
Revision as of 22:52, 6 November 2008
We can find a the eigenfunction which satisfy
[math]\displaystyle{ \partial_x^4 w_n = \lambda_n^4 w_n }[/math]
plus the edge conditions.
This solution is discussed further in Eigenfunctions for a Free Beam.
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.
General solution of the above stated 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]
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]
Having obtained eigenvalues [math]\displaystyle{ \lambda_n }[/math], natural requency can be readily calculated :
[math]\displaystyle{ \omega_n = \frac{(\lambda_n l)^2}{l^2}\sqrt\frac{EI}{m} }[/math]
Symmetrical natural modes can be written in normalized form as :
[math]\displaystyle{ w_n = \frac{1}{2}(\frac{\cos(\lambda_n x)}{\cos(\lamda_n l)}+\frac{\cosh(\lambda_n x)}{\cosh(\lambda_n l)}) }[/math]