\(\def \u#1{\,\mathrm{#1}}\) \(\def \abs#1{\left|#1\right|}\) \(\def \ast{*}\) \(\def \deg{^{\circ}}\) \(\def \tau{\uptau}\) \(\def \ten#1{\times 10^{#1}}\) \(\def \redcancel#1{{\color{red}\cancel{#1}}}\) \(\def \BLUE#1{{\color{blue} #1}}\) \(\def \RED#1{{\color{red} #1}}\) \(\def \PURPLE#1{{\color{purple} #1}}\) \(\def \th#1,#2{#1,\!#2}\) \(\def \lshift#1#2{\underset{\Leftarrow\atop{#2}}#1}}\) \(\def \rshift#1#2{\underset{\Rightarrow\atop{#2}}#1}}\) \(\def \dotspot{{\color{lightgray}{\circ}}}\) \(\def \ccw{\circlearrowleft}\) \(\def \cw{\circlearrowright}\)
Chapter 9: Oscillations
5.

Simple Harmonic Motion

When the restoring force on an oscillating object is proportional to its displacement (that is, when $F\sim y(t)$), then the oscillation is called simple harmonic motion. If we graph the displacement of such an oscillation as a function of time, we find that the displacement is sinusoidal-- it looks like a sine or cosine function.

We can write the displacement as a cosine (in radians mode):

$$y(t) = A\cos\left(2\pi {t\over T}+\phi_0\right)$$

where

For example, if $\phi_0=0$, then $$y(t=0) = A\cos \left(2\pi {0\over T}\right) = A\cos 0 = A$$ because $\cos 0=1$ (see Trigonometric Functions). At $t=T$, it will have completed exactly one cycle, and its displacement is now $$y(t=T)=A\cos\left(2\pi {T\over T}\right) =A\cos 2\pi = A$$ because $\cos2\pi = 1$. (We must work with radians in this section!)

Because $f=\frac1T$, we can also write the displacement as

$$y(t) = A\cos\left(2\pi ft+\phi_0\right)$$

Physicists like this version because we don't like writing fractions if we can avoid it.