For the coupled pendulums of mass

PHYSICS · Multi-part · Fermi University Physics · Mathematical Methods for Physics · Mechanics & Dynamical Systems · Linear algebra and vector spaces

Action and Symmetry, Ch Normal modes as a generalised eigenvalue problem

Problem

For the coupled pendulums of mass m1=1.0 kgm_1=1.0\ \mathrm{kg}, m2=3.0 kgm_2=3.0\ \mathrm{kg} described above, T=diag(1.0,3.0) kg m2\mathbf T=\mathrm{diag}(1.0,3.0)\ \mathrm{kg\,m^2}, with modes a(1)=(1,1)\mathbf a^{(1)}=(1,1) at ω12=9.80 rad2 s−2\omega_1^2=9.80\ \mathrm{rad^2\,s^{-2}} and a(2)=(3,−1)\mathbf a^{(2)}=(3,-1) at ω22=26.47 rad2 s−2\omega_2^2=26.47\ \mathrm{rad^2\,s^{-2}}, satisfying a(r)TTa(s)=0\mathbf a^{(r)\mathrm T}\mathbf T\mathbf a^{(s)}=0 for r≠sr\ne s. Define normal coordinates by θ=a^(1)η1+a^(2)η2\boldsymbol\theta=\hat{\mathbf a}^{(1)}\eta_1+\hat{\mathbf a}^{(2)}\eta_2, where a^(r)\hat{\mathbf a}^{(r)} are the mode vectors normalised so that a^(r)TTa^(s)=δrs\hat{\mathbf a}^{(r)\mathrm T}\mathbf T\hat{\mathbf a}^{(s)}=\delta_{rs}. ((a)) Starting from T=12θ˙TTθ˙T=\tfrac12\dot{\boldsymbol\theta}^{\mathrm T}\mathbf T\dot{\boldsymbol\theta}, V=12θTVθV=\tfrac12\boldsymbol\theta^{\mathrm T}\mathbf V\boldsymbol\theta, and the mode equation Va(r)=ωr2Ta(r)\mathbf V\mathbf a^{(r)}=\omega_r^2\mathbf T\mathbf a^{(r)}, derive, for any number of degrees of freedom, that T=12∑rη˙r2T=\tfrac12\sum_r\dot\eta_r^2 and V=12∑rωr2ηr2V=\tfrac12\sum_r\omega_r^2\eta_r^2. ((b)) Find a^(1)\hat{\mathbf a}^{(1)} and a^(2)\hat{\mathbf a}^{(2)} for the pendulum system, and verify by direct substitution that T=12(η˙12+η˙22)T=\tfrac12(\dot\eta_1^2+\dot\eta_2^2).

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