Find the law of motion of a physical pendulum: a rigid body…
Find the law of motion of a physical pendulum: a rigid body of mass $m$ rotating freely about a fixed horizontal axis $O$ that does not pass through the center of mass $G$. Let $I$ be the moment of inertia about $O$, $l$ the distance from $O$ to $G$, $\varphi$ the angle of deflection from vertical equilibrium, and $g$ the acceleration due to gravity.
Explanation of Method
Newton's second law for rotation, linearized for small angles, reduces the physical pendulum to the harmonic oscillator φ″+ω²φ=0 with ω²=mgl/I.
Step 1: Equation of motion
Gravity exerts a restoring torque about $O$ equal to $-mgl\sin\varphi$. By Newton's second law for rotation, $I\ddot\varphi$ equals this torque: $I\ddot\varphi = -mgl\sin\varphi.$
Step 2: Linearize for small oscillations
For small $\varphi$, $\sin\varphi\approx\varphi$, so: $I\ddot\varphi + mgl\,\varphi = 0.$
Dividing by $I$ and introducing $\omega^2 = \dfrac{mgl}{I}$ gives the standard harmonic-oscillator equation: $\ddot\varphi + \omega^2\varphi = 0.$
Step 3: Characteristic equation and general solution
\[ \lambda^2+\omega^2=0 \implies \lambda=\pm i\omega. \]
\[ \varphi(t) = C_1\cos\omega t + C_2\sin\omega t = \Phi\cos(\omega t-\varphi_0), \] where $\Phi=\sqrt{C_1^2+C_2^2}$ is the amplitude and $\varphi_0=\arctan(C_2/C_1)$ is the initial phase.
Step 4: Initial conditions
Suppose the pendulum is released from rest at deflection $\varphi_0^*$: $\varphi(0)=\varphi_0^*$, $\dot\varphi(0)=0$. Then: \[C_1 = \varphi_0^*, \qquad C_2\omega = 0 \implies C_2=0.\]
Step 5: Period and reduced length
\[ T = \frac{2\pi}{\omega} = 2\pi\sqrt{\frac{I}{mgl}}. \]
Defining a reduced (equivalent simple-pendulum) length $L$ so that $T=2\pi\sqrt{L/g}$: $L = \frac{I}{ml}.$
Step 6: Special case: mathematical pendulum
For a point mass on a massless rod, $I=ml^2$, so $\omega^2=g/l$ and $T=2\pi\sqrt{l/g}$: \[\ddot\varphi+\frac{g}{l}\varphi=0, \qquad \varphi(t)=\varphi_0^*\cos\!\left(\sqrt{\frac{g}{l}}\,t\right).\]
Step 7: Energy
Mechanical energy is conserved; in the small-angle approximation: \[E = \frac{1}{2}I\dot\varphi^2 + mgl(1-\cos\varphi) \approx \frac{1}{2}I\dot\varphi^2 + \frac{1}{2}mgl\,\varphi^2 = \frac{1}{2}I\omega^2\Phi^2 = \mathrm{const}.\]
Step 8: Verify
With $\varphi(t)=\varphi_0^*\cos\omega t$: $\dot\varphi=-\varphi_0^*\omega\sin\omega t$, $\ddot\varphi=-\varphi_0^*\omega^2\cos\omega t=-\omega^2\varphi$, so $\ddot\varphi+\omega^2\varphi=0\ \checkmark$. Also $\varphi(0)=\varphi_0^*\ \checkmark$ and $\dot\varphi(0)=0\ \checkmark$.
Step 9: Law of motion
The solution is recorded in the result below.
Result
Final answer:
\[\boxed{\,\varphi(t) = \varphi_0^*\cos\omega t, \qquad \omega=\sqrt{\frac{mgl}{I}}, \qquad T=2\pi\sqrt{\frac{I}{mgl}}\,}\]