Question 4.5.1: Consider a 2-dof system whose matrix equation of motion is g......

Consider a 2-dof system whose matrix equation of motion is given as

\begin{bmatrix} m_{11} & 0 \\ 0 & m_{22} \end{bmatrix}\begin{pmatrix} \ddot{x} _{1} \\ \ddot{x}_{2} \end{pmatrix}  + \begin{bmatrix} k_{11} & k_{12} \\ k_{21} & k_{22} \end{bmatrix} \begin{pmatrix} x_{1} \\ x_{2} \end{pmatrix} = \begin{pmatrix} 0\\ 0 \end{pmatrix} ,       (i)

where m_{11}=2m,\,m_{22}={\frac{2}{3}}m L^{2},\,k_{11}=2k,\,k_{12}=k_{21}=-{\frac{k L}{2}},\,k_{22}={\frac{25k L^{2}}{8}},\,x_{1}=x is the translational displacement, and x_{2} = θ is the angular or rotational displacement.

a. Determine the natural frequencies and mode shapes of the 2-dof system.

b. For the given system with 2m = 2000 kg, 2k = 40,000 N/m, and L = 1.0 m, find the natural frequencies and normal modes of the 2-dof system.

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a. Since the system is undamped and therefore the responses have no delay or phase difference with respect to the applied force, one can write

{\binom{x_{1}}{x_{2}}}={\binom{X_{1}}{X_{2}}}s{\mathrm{in}}\omega t={\binom{X}{\Theta}}\sin\omega t.

In this equation, X and Θ are the amplitudes of instantaneous displacements x_{i}. and symbolically not to be confused with the Laplace transform of x_{i}.

Substituting the above solution and its derivatives into Equation (i) and simplifying, one has

\begin{bmatrix}(k_{11}\!-\!m_{11}\!\omega^{2}) & k_{12} \\ k_{21} & (k_{22}\!-\!m_{22}\!\omega^{2}) \end{bmatrix}{\binom{X}{\Theta}}={\binom{0}{0}}                  (ii)

or writing it in a more concise form

[Z(\omega)]{\binom{X_{1}}{X_{2}}}={\binom{0}{0}}

where the so-called impedance matrix has been defined by Equation (4.18) as

\begin{bmatrix}(k_{11} – m_{1}\omega^{2}) & k_{12} \\ k_{21} & (k_{22} – m_{2} \omega^{2}) \end{bmatrix}{\binom{X_{1}}{X_{2}}}={\binom{F_{1}}{0}}            (4.18)

[Z(\omega)]= \begin{bmatrix}(k_{11}\!-\!m_{11}\!\omega^{2}) & k_{12} \\ k_{21} & (k_{22}\!-\!m_{22}\!\omega^{2}) \end{bmatrix}

Of course, one can determine the natural frequencies of the system by making use of Equations (A2a) and (A2b) in Appendix 4A.

\omega_{1}^{2}={\frac{-b+{\sqrt{b^{2}-4a c}}}{2a}}                (A2a)

\omega_{2}^{2}={\frac{-b-{\sqrt{b^{2}-4a c}}}{2a}}                  (A2b)

However, one can simply apply the frequency equation from Equation (ii); that is, equating the determinant of the impedance matrix [Z(ω)] to zero,

\left|{\begin{array}{ll}{k_{11}-m_{11}\omega^{2})}&{k_{12}}\\ {k_{21}}&{{}(k_{22}-m_{22}\omega^{2})}\end{array}}\right|=0.

Substituting the system parameters given above and writing λ = ω²

\left|{\begin{array}{ll}(2k− 2mλ) & -{\frac{k L}{2}} \\ -{\frac{k L}{2}} & \left({\frac{25k L^{2}}{8}}-{\frac{2}{3}}m L^{2}\lambda\right) \end{array}}\right| = 0

Operating on this equation, one has

(2k-2m\lambda)\biggl(\frac{25k L^{2}}{8}-\frac{2}{3}m L^{2}\lambda\biggr)-\biggl(\frac{k L}{2}\biggr)^{2}=0.

This quadratic equation in λ gives

\lambda_{1}=0.9498\,\frac{k}{m},~~~\lambda_{2}=4.7377\frac{k}{m}

which gives the two natural frequencies as

\omega_{1}={\sqrt{0.9498{\frac{k}{m}}}}=0.9746{\sqrt{\frac{k}{m}}},          (iiia)

\omega_{2}={\sqrt{4.7377{\frac{k}{m}}}}=2.1766{\sqrt{\frac{k}{m}}}.                (iiib)

In order to obtain the mode shapes, one substitutes {\boldsymbol{\omega}}_{1} into Equation (ii), resulting in

\left({\frac{X}{\Theta}}\right)_{(1)}={\frac{k_{12}}{m_{11}\omega_{1}^{2}-k_{11}}}={\frac{-{\frac{kL}{2}}}{2m\big(0.9498\,{\frac{k}{m}}\big)-2k}}=4.98L.            (iva)

where the subscript (1) on the lhs of Equation (iva) denotes the amplitude ratio associated with the first natural frequency. Similarly, substituting {\boldsymbol{\omega}}_{2} into Equation (ii), one has

\left({\frac{X}{\Theta}}\right)_{(2)}={\frac{k_{12}}{m_{11}\omega_{1}^{2}-k_{11}}}={\frac{-{\frac{k L}{2}}}{2m(4.7377{\frac{k}{m}})-2k}}= − 0.067L            (ivb)

Equations (iva) and (ivb) give the two mode shapes of the 2-dof system.

b. For the given system with 2m = 2000 kg, 2k = 40,000 N/m, L = 1.0 m, Equations (iiia) and (iiib) give the two natural frequencies as

\omega_{1}=4.3584\,\mathrm{rad/s},          (va)

\omega_{2}=9.7342\,\mathrm{rad/s}.      (vb)

If one assumes ΘL = 1 so that Equations (iva) and (ivb) become

\left({\frac{X}{\Theta L}}\right)_{(1)}=4.98          (via)

\left({\frac{X}{\Theta L}}\right)_{(2)}=-\,0.067.       (vib)

Thus, the required two normal modes can be written as

\Phi_{1}={\binom{4.980}{1.000}}          (viia)

\Phi_{2}={\binom{-0.067}{1.000}}             (viib)

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