Now that we have established the theory and equations behind harmonic motion, we will examine various physical situations in which objects move in simple harmonic motion. Previously, we worked with a mass-spring system, and will examine other harmonic oscillators in a similar manner. Finally, after establishing these applications, we can examine the similarity between simple harmonic motion and uniform circular motion.

### The Torsional Oscillator

Consider a circular disk suspended from a wire fixed to a ceiling. If the disk is rotated, the wire will twist. When the disk is released, the twisted wire exerts a restoring force on the disk, causing it to rotate past its equilibrium point, twisting the wire the other direction, as shown below. This system is called a torsional oscillator.

It has been found experimentally that the torque exerted on the disk is proportional to the angular displacement of the disk, or:τ = - κθ |

where

*κ*is a proportionality constant, a property of the wire. Note the similarity to our spring equation

*F*= -

*kx*. Since

*τ*=

*Iα*for any rotational motion we can state that

*κθ*=

*Iα*=

*I*

*m*for

*I*,

*k*for

*κ*, and

*x*for

*θ*we can see that this is the exact same differential equation we had for our spring system. Thus we may skip to the final solution, describing the angular displacement of the disk as a function of time:

θ = θ_{m}cos(σt) |

where

*θ*

_{m}is defined as the maximum angular displacement and

*σ*is the angular frequency given by

*σ*= .

**Note**: It is important not to confuse angular frequency and angular velocity.

*σ*in this case refers to the angular frequency of the oscillation, and cannot be used for angular velocity.

From our expression for angular frequency we can derive that

T = 2Π |

This equation for the period of a torsional oscillator has a significant experimental use. Suppose a body of unknown moment of inertia is placed on a wire of known constant

*κ*. The period of oscillation can be measured, and the moment of inertia of the body can be determined experimentally. This is quite useful, as the rotational inertia of most bodies cannot be easily determined using the traditional calculus-based method.

From our examination of the torsional oscillator we have derived that its motion
is simple harmonic. This oscillator can almost be seen as the rotational
analogue of the mass-spring system: just as with the mass-spring we substituted
*θ* for *x*, *I* for *m* and *κ* for *k*. Not all simple harmonic oscillators
have such close correlation.

### The Pendulum

Another common oscillation is that of the simple pendulum. The classic pendulum consists of a particle suspended from a light cord. When the particle is pulled to one side and released, it swings back past the equilibrium point and oscillates between two maximum angular displacements. It is clear that the motion is periodic--we want to see if it is simple harmonic.

We do so by drawing a free body diagram and examining the forces on the pendulum at any given time.

The two forces acting on the pendulum at any given time are tension from the rope and gravity. At the equilibrium point the two are antiparallel and cancel exactly, satisfying our condition that there must be no net force at the equilibrium point. When the pendulum is displaced by an angle*θ*, the gravitational force must be resolved into radial and tangential components. The radial component,

*mg*cos

*θ*, cancels with the tension, leaving net tangential force;

F = - mg sinθ |

In this case the restoring force is

*not*proportional to the angular displacement

*θ*, but is rather proportional to the sine of the angular displacement, sin

*θ*. Strictly speaking, then, the pendulum does not engage in simple harmonic motion. However, most pendulums function at very small angles. If the angle is small we may make the approximation sin

*θ*

*θ*. With this approximation we can rewrite our force expression:

*F*= -

*mgθ*

*θ*is given by

*x*=

*Lθ*. Substituting this in, we see that:

F = - mg = - x |

Thus we have an equation in the same form as our mass-spring equation; in this case

*k*= . We can skip the calculus and simply state the period of the pendulum:

pendulum

T = 2Π = 2Π |

Note that the period, and thus the frequency, of the pendulum is independent of the mass of the particle on the cord. It only depends on the length of the pendulum and the gravitational constant. Keep in mind, also, that this is only an approximation. If the angle exceeds more than fifteen degrees or so, the approximation breaks down.