Instance Models
This section transforms the problem defined in the problem description into one which is expressed in mathematical terms. It uses concrete symbols defined in the data definitions to replace the abstract symbols in the models identified in theoretical models and general definitions.
Refname | IM:calOfAngularDisplacement |
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Label | Calculation of angular displacement |
Input | \({L_{\text{rod}}}\), \({θ_{i}}\), \(\boldsymbol{g}\) |
Output | \({θ_{p}}\) |
Input Constraints | \[{L_{\text{rod}}}\gt{}0\]\[{θ_{i}}\gt{}0\]\[\boldsymbol{g}\gt{}0\] |
Output Constraints | \[{θ_{p}}\gt{}0\] |
Equation | \[{θ_{p}}\left(t\right)={θ_{i}}\,\cos\left(Ω\,t\right)\] |
Description |
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Notes |
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Source | – |
RefBy | FR:Output-Values and FR:Calculate-Angular-Position-Of-Mass |
Detailed derivation of angular displacement:
When the pendulum is displaced to an initial angle and released, the pendulum swings back and forth with periodic motion. By applying Newton’s second law for rotational motion, the equation of motion for the pendulum may be obtained:
\[\boldsymbol{τ}=\boldsymbol{I}\,α\]
Where \(\boldsymbol{τ}\) denotes the torque, \(\boldsymbol{I}\) denotes the moment of inertia and \(α\) denotes the angular acceleration. This implies:
\[-m\,\boldsymbol{g}\,\sin\left({θ_{p}}\right)\,{L_{\text{rod}}}=m\,{L_{\text{rod}}}^{2}\,\frac{\,d\frac{\,d{θ_{p}}}{\,dt}}{\,dt}\]
And rearranged as:
\[\frac{\,d\frac{\,d{θ_{p}}}{\,dt}}{\,dt}+\frac{\boldsymbol{g}}{{L_{\text{rod}}}}\,\sin\left({θ_{p}}\right)=0\]
If the amplitude of angular displacement is small enough, we can approximate \(\sin\left({θ_{p}}\right)={θ_{p}}\) for the purpose of a simple pendulum at very small angles. Then the equation of motion reduces to the equation of simple harmonic motion:
\[\frac{\,d\frac{\,d{θ_{p}}}{\,dt}}{\,dt}+\frac{\boldsymbol{g}}{{L_{\text{rod}}}}\,{θ_{p}}=0\]
Thus the simple harmonic motion is:
\[{θ_{p}}\left(t\right)={θ_{i}}\,\cos\left(Ω\,t\right)\]