A simple pendulum consists of a point mass \(m\) suspended by a (weightless) cord or rod of length \(l,\) as shown, and swinging in a vertical plane under the action of gravity. Show that for small oscillations (small \(\theta\) ), both \(\theta\) and \(x\) are sinusoidal functions of time, that is, the motion is simple harmonic. Hint: Write the differential equation \(\mathbf{F}=m \mathbf{a}\) for the particle \(m .\) Use the approximation \(\sin \theta=\theta\) for small \(\theta,\) and show that \(\theta=A \sin \omega t\) is a solution of your equation. What are \(A\) and \(\omega ?\)

Newton's Second Law is a fundamental principle in physics that states that the force acting on an object is equal to the mass of the object multiplied by its acceleration. For the simple pendulum, the force acting on the point mass is the restoring force due to gravity. This force can be expressed as \[F = -mg \sin(\theta)\], where \(-mg \sin(\theta)\) represents the component of the gravitational force pulling the mass back towards its equilibrium point. By Newton's Second Law, this force is also equal to the mass of the pendulum bob times its acceleration along the arc, which gives us the equation: \[m \ddot{x} = -mg \sin(\theta)\]. Since \[x = l \theta\], we can write the equation as: \[m \ddot{(l \theta)} = -mg \sin(\theta)\]. Simplifying this expression leads us to the differential equation that describes the motion of the pendulum.

The Small-Angle Approximation is a key concept when analyzing the motion of a simple pendulum. It assumes that for small angles (measured in radians), the sine of the angle is approximately equal to the angle itself. This simplifies the mathematical analysis of the pendulum's motion. In other words, for small oscillations of the pendulum, we can use: \[ \sin(\theta) \approx \theta \]. This approximation is valid when \( \theta \) is in the range of a few degrees. By applying the small-angle approximation to our differential equation, we can replace \[ \sin(\theta) \] with \[\theta\]. This results in a simplified differential equation: \[ m l \ddot{\theta} = -mg \theta \]. Dividing both sides by \( ml \), we get: \[ \ddot{\theta} + \frac{g}{l} \theta = 0 \]. This is a key step towards understanding the simple harmonic motion of the pendulum.

A Differential Equation is an equation that involves the derivatives of a function. For the simple pendulum, we form a differential equation to describe its motion. From Newton's Second Law and applying the small-angle approximation, we obtained the equation: \[ m l \ddot{\theta} = -mg \theta \]. After simplification, this becomes: \[ \ddot{\theta} + \frac{g}{l} \theta = 0 \]. This is a second-order linear differential equation, which is characteristic of simple harmonic motion (SHM). The general form of SHM differential equation is: \[ \ddot{x} + \omega^2 x = 0 \], where \(\omega \) is the angular frequency. By comparing our pendulum's differential equation with the SHM equation, we can identify \( \omega \) and confirm that the motion of the pendulum is indeed simple harmonic for small angles.

Angular Frequency (\( \omega \)) is a measure of how quickly something oscillates in simple harmonic motion. For the simple pendulum, we derived the differential equation: \[ \ddot{\theta} + \frac{g}{l} \theta = 0 \]. Comparing this with the standard form of the simple harmonic motion equation: \[ \ddot{x} + \omega^2 x = 0 \], we can see that \[ \omega^2 = \frac{g}{l} \]. Therefore, the angular frequency \( \omega \) of the pendulum is: \[ \omega = \sqrt{\frac{g}{l}} \]. This shows how the length \( l \) of the pendulum and the acceleration due to gravity \( g \) influence the frequency of its oscillations. The period of the pendulum, which is the time it takes to complete one full oscillation, is related to the angular frequency by: \[ T = \frac{2\pi}{\omega} = 2\pi \sqrt{\frac{l}{g}} \]. This gives us a complete understanding of how the pendulum behaves over time.