Part 4 - Waves

The next chapter in our physics course is about waves, especially mechanical waves.

General about Waves

In this chapter we’ll cover mechanical waves but also electromagnetic waves, in this case only (visible) light.

There’s two types of waves we’ll be covering:

  • Transverse waves
    • They have ‘noise’ orthogonal against the wave’s propagation speed.
  • Longitudinal waves
    • They have ‘noise’ parallel with the waves’ propagation speed.

We can describe this noise with the function y(x,t)=f(x+vt)y(x, t) = f(x + vt).

Harmonic Waves

Harmonic waves are ‘idealized waves’ where the frequency is a positive integer multiple of the fundamental frequency.

This just means we can describe our waves in terms of sine and cosine functions.

A general formula for harmonic waves is:

y(x,t)=A sin[2π(xλλλ Tt)]y(x, t) = A\ sin[2\pi(\frac{x}{\lambda} - \frac{\lambda}{\lambda\ T}t)]

Let’s cover each term here and see what they mean:

A Amplitude [m]λ Wave-length [m]f Frequency [Hz][1s]v Propagation velocity [ms]ω Angular velocity [rads]T Period [s]A - \text{ Amplitude } [m] \newline \lambda - \text{ Wave-length } [m] \newline f - \text{ Frequency } [Hz] [\frac{1}{s}] \newline v - \text{ Propagation velocity } [\frac{m}{s}] \newline \omega - \text{ Angular velocity } [\frac{rad}{s}] \newline T - \text{ Period } [s] \newline

And now let’s write up some relationships between these variables:

f=1Tω=2π f=2πTv=λ fλ=v Tv=λ1Tf = \frac{1}{T} \newline \omega = 2\pi\ f = \frac{2\pi}{T} \newline v = \lambda\ f \newline \lambda = v\ T \newline v = \lambda \frac{1}{T}

Now we can rewrite our general formula to something even more general:

y(x,t)=A sin(kxωt+ϕ), wherek=2πλ[radm]ϕ= Describes our ’starting’ position.y(x, t) = A\ sin(kx - \omega t + \phi) \text{, where} \newline k = \frac{2\pi}{\lambda} [\frac{rad}{m}] \newline \phi = \text{ Describes our 'starting' position.}

Different Kind of Velocities

There’s two different kinds of velocities that we need to differentiate. We can view the entire waves velocity as VfV_f, but at the same time we could view a singular particles speed. This is noted by VpV_p

We can write VpV_p as:

Vp=dydt=ωAcos(kxωt+ϕ)V_p = \frac{dy}{dt} = -\omega A cos(kx - \omega t + \phi)

Velocities in a String

Strings, when flicked, will behave like waves - If we fixate a string on each ends, for example in a guitar.

We can calculate the propagation velocity as:

Vf=Tμ, where T Tension force [N]μ mass per length-unit [kgm]V_f = \sqrt\frac{T}{\mu} \text{, where } \newline T - \text{ Tension force } [N] \newline \mu - \text{ mass per length-unit } [\frac{kg}{m}]

Intensity

The ‘intensity’ of a wave describes it’s energy flux. But we can also describe it as:

I  A2I\ \propto\ A^2

So the intensity is proportional to the amplitude squared. This will become important once we begin to cover light waves.

Wave interference

Interference is the phenomena that occurs when two waves collide. It can either result in destructive interference where the waves ‘take each other out’, or in constructive interference, which means we ‘add’ the waves together. It’s quite a natural thing as we can see from the equations:

y1=A sin(kxωt)y2=A sin(kxωt+ϕ)y_1 = A\ sin(kx - \omega t) \newline y_2 = A\ sin(kx - \omega t + \phi) ytotal=A [sin(kxωt)+sin(kxwt+ϕ)]y_{total} = A\ [sin(kx - \omega t) + sin(kx - wt + \phi)]

Using the sine addition formula:

ytotal=2A cos(ϕ2)×sin(kxωt+ϕ2)y_{total} = 2A\ cos(\frac{\phi}{2}) \times sin(kx - \omega t + \frac{\phi}{2})

The important term is the ϕ2\frac{\phi}{2} if this is:

ϕ2=mπ,, where m= positive integer \frac{\phi}{2} = m\pi, \text{, where } \newline m = \text{ positive integer }

Then we have so called constructive interference - visually this means we have highs and lows ‘aligned’.

If instead this term is:

ϕ2=(2m+1) π2,, where m= positive integer \frac{\phi}{2} = (2m + 1)\ \frac{\pi}{2}, \text{, where } \newline m = \text{ positive integer }

Then we have destructive interference, or visually, opposites will be aligned (highs with lows, and lows with higs of the other).

More Ways to Write Wave Equation

One we can rewrite our original wave equation is:

A sin(ω(txv))A\ sin(\omega(t - \frac{x}{v}))

Which can be useful sometimes!

Reflection and Transmission of Waves

If we have a wave that propagates from one medium to another, we will have so called reflection and transmission of the wave.

If we just visualize what will happen is that - the reflection of the wave will go in the other direction - whilst the transmission will have the same direction as the wave before.

By doing some math we get:

Ai+Ar=AtA_i + A_r = A_t

Which seems logical, the initial wave added with the reflection wave should have the same amplitude as the new transmission wave.

We can also get the following:

ddx (yi+yr)=ddx yt\frac{d}{dx}\ (y_i + y_r) = \frac{d}{dx}\ y_t 1V1 (AiAr)=1V2 At\frac{1}{V_1}\ (A_i - A_r) = \frac{1}{V_2}\ A_t

Which finally gives us the relation:

At=2 V2V2+V1 AiA_t = \frac{2\ V_2}{V_2 + V_1}\ A_i Ar=V2V1V2+V1AiA_r = \frac{V_2 - V_1}{V_2 + V_1} A_i

Standing Waves

Standing waves is the phenomena when interference occurs but the waves have opposite direction.

y1=A sin(kxωt)y2=A sin(kx+ωt)ytotal==2A sin(kx) cos(ωt)y_1 = A\ sin(kx - \omega t) \newline y_2 = A\ sin(kx + \omega t) \newline y_{total} = \dots = 2A\ sin(kx)\ cos(\omega t)

From this we can see that in some points, we will always have some points that are 0. We call these points ‘nodes’. The peaks are therefore called antinodes.

Fixated Wave

Let’s apply our knowledge about standing waves to this example - we have a string which is fixated at both ends. So therefore:

y(0,t)=0y(L,t)=0y(0, t) = 0 \newline y(L, t) = 0

So at x = 0 (the start of the string) and x = L (the end of the string).

We get:

y=2A sin(0) cos(ωt)=0y = 2A\ sin(0)\ cos(\omega t) = 0

Which is what we wanted, now for x=Lx = L:

y=2A sin(kL) cos(omegat)=0y = 2A\ sin(kL)\ cos(omega t) = 0

For this to be equal to 0 - sin(kL)sin(kL) needs to be 0. So:

sin(kL)=0k=2πλkL=mπλ=2Lmsin(kL) = 0 \newline k = \frac{2\pi}{\lambda} \newline kL = m\pi \newline \lambda = \frac{2L}{m}

This means we only have a subset of all possible Wave-lengths that we can use so that our initial conditions are fullfilled.

λ=2L,L,23 L,\lambda = 2L, L, \frac{2}{3}\ L, \dots

Beats

This phenomena occurs when we have two frequencies which are really close, there isn’t really that much to say, we can look at the formula and derive what happens from there:

y=y1+y2=2A cos[2π (f1f22) t]×cos[2π (f1+f22) t]y = y_1 + y_2 = 2A\ cos[2\pi\ (\frac{f_1 - f_2}{2})\ t] \times cos[2\pi\ (\frac{f_1 + f_2}{2})\ t]

So from this we can see that if f1,f2f_1, f_2 are really close, we will have a really low frequency and a high frequency that is close to f1f_1.

The Doppler Effect

Is the effect that happens when we have a sound source which moves, or both the listener and sound source move.

If only the listener moves

If the listener moves then we can write the frequency which the listener hears as:

fL=V+VLλ=V+VLVfS=(1+VLV) fSf_L = \frac{V + V_L}{\lambda} = \frac{V + V_L}{\frac{V}{f_S}} = (1 + \frac{V_L}{V})\ f_S

If both are moving

fL=V+VLV+VS fSf_L = \frac{V + V_L}{V + V_S}\ f_S

Conclusion

This was it for this part - quite short, waves are a quite natural phenomena so a lot of things comes from intuition. In the next part we’ll begin to cover light waves!