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CHAPTER 13

Simple Harmonic Motion

We have already learnt that when a spring is stretched or compressed by a certain amount x, it exerts a force proportional to the displacement. Moreover, the direction of the force exerted by the spring is always opposite to the displacement (and for this reason it is called a restoring force). All this can be expressed by
F = -kx
with k = spring constant. We will now study the motion of a body moving under the influence of such a restoring force. This motion, that goes under the name of Simple Harmonic Motion (or Simple Harmonic Oscillation), is encountered, either exactly or approximately, in a very large class of physical phenomena.

Suppose then you have a mass m resting on a frictionless surface and attached to a spring of constant k. To obtain the equation of motion, we write as usual Newton's second law :
F=ma

-kx(t) = m d2x(t)/dt2
this is again a differential equation, and to solve it we need to find a function which, apart from the constant factors k and m, is equal to minus its second derivative. The minus sign is essential, and if it wasn't there it would lead to a completely different situation.

Question : what would be the solution if the minus wasn't there, i.e. if you were looking for a function equal to its second derivative?

But returning to our case, we see that a good candidate is the cosine (we could also have chosen the sine), since
$d\cos = \sin,~~~d\sin = -\cos \rightarrow d^{2}\cos = -\cos $
We can then guess that the cosine is the function we are looking for, and in fact one could see that the most general expression satisfying the differential equation under study can be written as
$x(t) = A\cos(\omega t+\phi) $
with $A,\omega,\phi$ constant parameters. We can verify that this result satisfies the differential equation. One has
$v(t)=dx(t)/dt = A\omega\sin(\omega t+\phi) $

$a(t) = dv(t)/dt = -A\omega^{2}\cos(\omega t+\phi) $

But the condition we want to satisfy is
a(t) = -(k/m)x(t)
our general solution will satisfy this condition provided that $\omega^{2} = k/m$.

It is clear then that the motion of our mass will be a periodic oscillation, with the mass moving back and forth around its position of equilibrium x=0. Let us examine the physical meaning of the parameters $A,\omega,\phi$: Let us choose for simplicity $\phi=0$ The expressions
$x(t)= x_{max}\cos\omega t $

$v(t)= x_{max}\omega\sin\omega t $

$a(t) =-x_{max}\omega^{2}\cos\omega t $

allow us to determine the position, velocity and acceleration of our mass, as well as their relative values, at any instant t. In particular :

Harmonic Motion and Energy Coservation

We had learnt that the force exerted by a spring is conservative and that a spring stretched (or compressed) by an amount x carries a Potential Energy $\frac{1}{2}kx^{2}$. We can then expect that, throughout the oscillatory motion, the total mechanical energy (i.e. the sum of potential + kinetic energy) of the system is conserved :

$E = K + U = \frac{1}{2}mv^{2}(t) + \frac{1}{2}kx^{2}(t)$ = constant
Throughout the motion we have a continuous, back and forth transformation from potential to kinetic energy and viceversa. When the spring is fully stretched (x=xmax) the energy is all potential, while when the mass goes through x=0, the potential energy is zero and the energy is all kinetic. We then have
$E = K + U = \frac{1}{2}mv^{2}(t) + \frac{1}{2}kx^{2}(t) = \frac{1}{2}kx_{max}^{2} = \frac{1}{2}mv_{max}^{2} $
(and the last equality shows again that $v_{max} = x_{max}\sqrt{k/m} $). Through simple substitutions one could also see that
$v(x) = \pm\sqrt{k/m(x_{max}^{2}-x^{2})} $

Pendulum Another mechanical system moving with simple harmonic motion is the pendulum: as an immediate consequence, we can expect that the pendulum period of oscillation will be independent of the oscillation amplitude. This important property was first realized by Galileo when observing the swinging of the church chandeliers as the sexton[*] was snuffing out the candles, and led to the construction of the first reliable time-keeping devices.

The conceptual pendulum is a point-like mass m supported by a massless string of length l. The forces acting on the mass are gravity and the string tension. As usual, the string tension cancels out the radial component of gravity, so that the only unbalanced force, responsible for the motion of the mass is gravity's tangential component $F_{t} = -mg\sin\theta$. $\theta$ is the angle with respect to the vertical and the minus sign reflects the fact that the force is alwyas in the direction opposite to the displacement (therefore it is a restoring force). Newton's law will then give
$-mg\sin\theta = m~d^{2}s/dt^{2} = (m/l) d^{2}\theta/dt^{2} $
this equation is not equivalent to that of the harmonic oscillator, since it relates the second derivative of $\theta$ not to $\theta$ itself but to its sine, and its solution is not straightforward. But we can simplify it by noticing that, if $\theta$ is small enough (say less than 100), then $\sin\theta\approx\theta$(in radians, you can verify it on your calculator). The expression therefore reduces to
$-(g/l)\theta = d^{2}\theta /dt^{2} $
whose solution will then be
$\theta (t) = \theta_{max}\cos(\omega t+\phi) = \theta_{max}\cos[2\pi (t/T)+\phi] $
with $T = 2\pi\sqrt{l/g} $, showing that, for small oscillation, the period is independent of the amplitude but is determined purely by l and g .

When dealing with a physical pendulum rather than an ideal one, the length l is obviously given by the distance between the point of suspension and the pendulum center of mass (since there is where the force of gravity is applied). With a given pendulum therefore one can either
1.
measure g if l is known, or
2.
given g, determine the center of mass of the swinging body (if you want to locate your own center of mass, you can ask a friend to hang you by your feet and time the period of your oscillations)
In terms of angular variables, the pendulum equation can be written as
$\tau = I\alpha $

$-mgd\sin\theta\approx -mgd\theta = Id^{2}\theta/dt^{2} $
which represents an oscillation of period $T = 2\pi\sqrt{I/(mgd})$. This would allow to determine the moment of inertia of any object, provided the location of its center of mass is known.

Torsional Pendulum Grandfather clocks are awkward to be worn on your wrist or kept in your pocket. To build a (mechanical) watch you need to rely on torsional elasticity : if you twist an elastic material (e.g. a wire) by an angle $\theta$, the restoring force creates a torque which is proportional to the angle of twist, $\tau = \kappa\theta$. If allowed to oscillate, a body attached to a twisted wire will oscillate with period $T = 2\pi\sqrt{I/\kappa}$ .

Harmonic Motion as Projection of Circular Motion In describing the harmonic motion, we have used the symbol $\omega$, which is normally associated with an angular velocity. So far we can just assume that the quantity $\omega$ was used for convenience, to avoid the $2\pi$ factors that would appear if we were to express the harmonic motion in terms of period T or frequency f. But we'll see that one can conceptually associate a harmonic motion with a uniform circular motion. Consider a body in uniform circular motion with constant angular velocity $\omega$. As the body moves around the circle, its projection on the x-axis is
$x(t)=R\cos\theta = R\cos\omega t$
where, for simplicity, we have chosen $\phi=0$. We then see that the projection of a uniform circular motion on any axis moves with simple harmonic motion. If we also look at the projection on the y-axis, its motion will be given by $y(t) = R\sin\omega t$. Since the global motion is given by the combined motion along the x and y direction, we can then state that any uniform circular motion can be considered as the combination of two simple harmonic motions along orthogonal directions and out of phase by 900.

Damped Oscillations In any real life situation, a harmonic oscillation will not go on forever, but it will gradually come to a stop, since the original mechanical energy gets eaten away by friction, air resistance etc. We have already seen that, under certain condtions, motion through a fluid encounters a resistance R which is proportional to the velocity of the moving object R = -bv . To study the motion of a harmonic oscillator under these more realistic conditions, we must include this resistive forcce in the equation of motion :
-kx-b dx/dt=m d2x/dt2
this differential equation is slightly more complicated than the one we encountered before, and so is its solution, which turns out to be
$x(t) = x_{max}e^{-bt/(2m)}\cos (\omega t+\phi)$,

with $\omega = \sqrt{k/m-(b/2m)^{2}} $
telling us that It could be shown that the condition (b/2m)2=k/m corresponds to the shortest time for returning to equilbrium. This condition is called critical damping. If b is smaller than the critical value the system is underdamped, if larger overdamped.

Forced Oscillations Another interesting case is when a force is applied to a system in order to keep it oscillating.

Note : so far we have dealt with the ideal case of a mass m attached to a spring k, leading to a natural angular frequency $\omega = k/m$. In reality, practically every object has some elasticity and, if some energy is applied to it, it will tend to vibrate at a well defined frequency. In other words, every object has some well defined natural frequency of vibration $\omega_{0}$ (and in fact complex objects can have several natural frequencies)

If now we want to transfer some energy to a system to keep it vibrating even in the presence of some resistive force, it is intuitive that the most efficient situation is encountered when a periodic force is applied with a period close to the natural period of the oscillating system. Think of maximizing the amplitude of a swing: if you give it random pushes, sometime you will increase its velocity but sometime you will decrease it. But you will reach optimum performance if you push it in synchronism with the swing oscillating motion.

Solution of the appropriate diferential equation, including restoring force -kx, damping force -bv and periodic applied force $F=F_{0}\cos\omega t$ leads to a sustained oscillation of amplitude
$A = F_{0}/(m\sqrt{(\omega^{2}-\omega_{0}^{2})^{2}+(b\omega /m)^{2}}) $
showing that the largest amplitude is obtained when $\omega\approx\omega_{0}$. In fact, if the damping is small, amplitude can become infinitely large.... The condition $\omega =\omega_{0}$ is called resonance, and it is encountered in several fields of physics (acoustics, electric circuits, subatomic physics, etc.)



 
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Sergio Conetti
10/31/2000