Problems 2

Part II ✎ Problems Phillips pp. 31–34 · ~16 min read

  • dispersion relation
  • group velocity
  • Schrödinger equation
  • Klein-Gordon equation

Four of these six problems attack the same equation from different sides, and the interesting answers are the ones where a plausible wave turns out not to solve it.

Six problems, each with Phillips’ own hint and a full worked solution, both collapsed so the page still works as practice.


1 Capillary waves — the ratio flips derivation

Waves on the surface of water are dispersive. If the wavelength is short enough that surface tension rather than gravity provides the restoring force, the dispersion relation is

ω=Tk3ρ\omega = \sqrt{\frac{Tk^3}{\rho}}

where TT is the surface tension and ρ\rho the density of water.

Find the phase velocity of a sinusoidal wave with wave number kk, and the group velocity of a packet with wave numbers near kk.

💡 Phillips' own hint

Use vphase=ω/kv_{\text{phase}} = \omega/k and vgroup=dω/dkv_{\text{group}} = d\omega/dk. Verify that vgroup=32vphasev_{\text{group}} = \tfrac32 v_{\text{phase}}.

✓ Worked solution

Write the dispersion relation as ω=(T/ρ)1/2k3/2\omega = (T/\rho)^{1/2}k^{3/2} so the kk-dependence is explicit. Then

vphase=ωk=Tkρv_{\text{phase}} = \frac{\omega}{k} = \sqrt{\frac{Tk}{\rho}}vgroup=dωdk=32(Tρ)1/2k1/2=32Tkρ=32vphasev_{\text{group}} = \frac{d\omega}{dk} = \frac{3}{2}\left(\frac{T}{\rho}\right)^{1/2}k^{1/2} = \frac{3}{2}\sqrt{\frac{Tk}{\rho}} = \frac{3}{2}\,v_{\text{phase}}

The general rule is worth extracting: for any power law ωkn\omega \propto k^n, vgroup=nvphasev_{\text{group}} = n\,v_{\text{phase}}. Gravity waves have n=12n = \tfrac12 (ratio 12\tfrac12), capillary waves n=32n = \tfrac32, light n=1n = 1, and a free quantum particle n=2n = 2.

2 A packet that keeps its shape derivation

Consider the wave packet

Ψ(x,t)=kΔkk+ΔkAcos(kxωt)dk\Psi(x,t) = \int_{k-\Delta k}^{k+\Delta k} A\cos(k'x - \omega' t)\,dk'

with the non-dispersive relation ω=ck\omega' = ck'. By integrating over kk', show that

Ψ(x,t)=S(xct)cosk(xct),S(xct)=2AΔksin[Δk(xct)][Δk(xct)]\Psi(x,t) = S(x-ct)\cos k(x-ct), \qquad S(x-ct) = 2A\Delta k\,\frac{\sin[\Delta k(x-ct)]}{[\Delta k(x-ct)]}

and describe how this packet propagates.

💡 Phillips' own hint

Use

cosk(xct)dk=sink(xct)(xct)\int\cos k'(x-ct)\,dk' = \frac{\sin k'(x-ct)}{(x-ct)}

and sinAsinB=2cos ⁣(A+B2)sin ⁣(AB2)\sin A - \sin B = 2\cos\!\big(\tfrac{A+B}{2}\big)\sin\!\big(\tfrac{A-B}{2}\big).

✓ Worked solution

The whole trick is that ω=ck\omega' = ck' lets you write the integrand’s phase as kxckt=k(xct)k'x - ck't = k'(x-ct) — a single variable u=xctu = x - ct. Substituting:

Ψ=kΔkk+ΔkAcos(ku)dk=Au[sin(ku)]kΔkk+Δk=Au[sin((k+Δk)u)sin((kΔk)u)]\Psi = \int_{k-\Delta k}^{k+\Delta k} A\cos(k'u)\,dk' = \frac{A}{u}\Big[\sin(k'u)\Big]_{k-\Delta k}^{k+\Delta k} = \frac{A}{u}\big[\sin((k{+}\Delta k)u) - \sin((k{-}\Delta k)u)\big]

Apply the sine difference identity with A=(k+Δk)uA' = (k+\Delta k)u and B=(kΔk)uB' = (k-\Delta k)u, so A+B2=ku\tfrac{A'+B'}{2} = ku and AB2=Δku\tfrac{A'-B'}{2} = \Delta k\,u:

Ψ=Au2cos(ku)sin(Δku)=2AΔksin(Δku)(Δku)cos(ku)\Psi = \frac{A}{u}\cdot 2\cos(ku)\sin(\Delta k\,u) = 2A\Delta k\,\frac{\sin(\Delta k\,u)}{(\Delta k\,u)}\,\cos(ku)

which is the required form with u=xctu = x - ct.

How it propagates. Both the carrier and the envelope depend on xx and tt only through the single combination xctx - ct. So the entire packet — shape and all — translates rigidly to the right at speed cc, without any change of form, for ever.

Non-dispersive vs dispersive — press propagate on each

-20-1001020-1.0-0.500.51.0position xΨ
  • Ψ(x,t)
  • envelope S(x), Eq. (2.5)
  • a crest — moves at ω/k
  • envelope peak — moves at dω/dk
ω(k)
ω = ck
length 2π/Δk
8.4
ω/k
1.00
dω/dk
1.00(1.00×)

Non-dispersive: every component travels at the same speed, so the packet keeps its shape forever and the two markers never separate. This is the one case the classical wave equation describes.

3 Real functions are not solutions verification

Verify by direct substitution that the real functions

Ψ=Acos(kxωt)andΨ=Asin(kxωt)\Psi = A\cos(kx-\omega t) \qquad\text{and}\qquad \Psi = A\sin(kx-\omega t)

are not solutions of the Schrödinger equation for a free particle.

💡 Phillips' own hint

Use relations like

cos(kxωt)t=ωsin(kxωt),2cos(kxωt)x2=k2cos(kxωt)\frac{\partial\cos(kx-\omega t)}{\partial t} = \omega\sin(kx-\omega t), \qquad \frac{\partial^2\cos(kx-\omega t)}{\partial x^2} = -k^2\cos(kx-\omega t)
✓ Worked solution

Take the cosine and put each side of Eq. (2.14) together separately.

Left side.

iΨt=iAωsin(kxωt)i\hbar\frac{\partial\Psi}{\partial t} = i\hbar A\omega\sin(kx-\omega t)

Right side.

22m2Ψx2=22m(k2Acos(kxωt))=2k22mAcos(kxωt)-\frac{\hbar^2}{2m}\frac{\partial^2\Psi}{\partial x^2} = -\frac{\hbar^2}{2m}\big(-k^2A\cos(kx-\omega t)\big) = \frac{\hbar^2k^2}{2m}A\cos(kx-\omega t)

Now look at what they are. The left side is ii times a real quantity — purely imaginary. The right side is purely real. Two complex numbers are equal only if their real and imaginary parts match separately, so we would need

ωAsin(kxωt)=0and2k22mAcos(kxωt)=0\hbar\omega A\sin(kx-\omega t) = 0 \quad\text{and}\quad \frac{\hbar^2k^2}{2m}A\cos(kx-\omega t) = 0

for all xx and tt — which forces A=0A = 0. The only “solution” is no wave at all.

The sine works out identically: the time derivative produces a cosine and the second space derivative reproduces the sine, so the two sides again land on perpendicular axes.

Confirm it for yourself — try every real option and drag ω\omega across its whole range:

Does this Ψ solve the free-particle Schrödinger equation? Plot both sides and look.

left side: iħ ∂Ψ/∂t

-6-4-20246-2-1012x

right side: −(ħ²/2m) ∂²Ψ/∂x²

-6-4-20246-2-1012x
  • real part
  • imaginary part

✗ not a solutionmismatch 100.0%

The left side is purely IMAGINARY and the right side purely REAL. No choice of ω can reconcile them — the failure is structural.

The derivatives are evaluated analytically, so “identical” means identical. Try every real option: none of them can be rescued by any value of ω, because one time derivative and two space derivatives put the two sides on perpendicular axes of the complex plane.

4 A complex standing wave verification

Verify that

Ψ(x,t)=Aei(kxωt)Aei(kx+ωt)\Psi(x,t) = A\,e^{i(kx-\omega t)} - A\,e^{-i(kx+\omega t)}

with AA an arbitrary complex constant, is a solution of the free-particle Schrödinger equation if ω=2k2/2m\hbar\omega = \hbar^2k^2/2m. Show it can be rewritten

Ψ(x,t)=2iAsinkx  eiωt\Psi(x,t) = 2iA\sin kx\;e^{-i\omega t}

What sort of wave is this?

💡 Phillips' own hint

The rewriting uses eiθeiθ=2isinθe^{i\theta} - e^{-i\theta} = 2i\sin\theta. It is a complex standing wave with wave number kk and angular frequency ω\omega.

✓ Worked solution

It is a solution. The first term is a plane wave with wave number +k+k; the second is a plane wave with wave number k-k, since ei(kx+ωt)=ei((k)xωt)e^{-i(kx+\omega t)} = e^{i((-k)x - \omega t)}. Both satisfy the equation when ω=2k2/2m\hbar\omega = \hbar^2k^2/2m — and crucially the same ω\omega works for both, because the dispersion relation depends on k2k^2 and is blind to the sign of kk. The equation is linear, so their difference is also a solution.

The rewriting. Factor out the common time dependence:

Ψ=Aeiωt(eikxeikx)=Aeiωt2isinkx=2iAsinkx  eiωt\Psi = A\,e^{-i\omega t}\big(e^{ikx} - e^{-ikx}\big) = A\,e^{-i\omega t}\cdot 2i\sin kx = 2iA\sin kx\;e^{-i\omega t}

What sort of wave. A standing wavexx and tt have separated into different factors, exactly as in §2.1’s classical standing wave. The nodes sit at x=nπ/kx = n\pi/k and stay there for ever.

5 Physicists on another planet conceptual

In quantum mechanics it is the convention to represent a free particle of momentum pp and energy EE by

Ψ(x,t)=Aei(pxEt)/\Psi(x,t) = A\,e^{i(px-Et)/\hbar}

Physicists on another planet may have chosen instead

Ψ(x,t)=Aei(pxEt)/\Psi(x,t) = A\,e^{-i(px-Et)/\hbar}

What is the form of the Schrödinger equation on that planet?

💡 Phillips' own hint

Verify that their wave function solves

iΨt=22m2Ψx2-i\hbar\frac{\partial\Psi}{\partial t} = -\frac{\hbar^2}{2m}\frac{\partial^2\Psi}{\partial x^2}
✓ Worked solution

Substitute their convention and see what equation it satisfies. With Ψ=Aei(pxEt)/\Psi = A e^{-i(px-Et)/\hbar}:

Ψt=iEΨ,2Ψx2=(ip)2Ψ=p22Ψ\frac{\partial\Psi}{\partial t} = \frac{iE}{\hbar}\Psi, \qquad \frac{\partial^2\Psi}{\partial x^2} = \left(\frac{-ip}{\hbar}\right)^2\Psi = -\frac{p^2}{\hbar^2}\Psi

We want an equation that reproduces E=p2/2mE = p^2/2m. Try multiplying the time derivative by i-i\hbar:

iΨt=iiEΨ=EΨ-i\hbar\frac{\partial\Psi}{\partial t} = -i\hbar\cdot\frac{iE}{\hbar}\Psi = E\Psi

and the right side is unchanged:

22m2Ψx2=p22mΨ-\frac{\hbar^2}{2m}\frac{\partial^2\Psi}{\partial x^2} = \frac{p^2}{2m}\Psi

So their Schrödinger equation is

  iΨt=22m2Ψx2  \boxed{\;-i\hbar\frac{\partial\Psi}{\partial t} = -\frac{\hbar^2}{2m}\frac{\partial^2\Psi}{\partial x^2}\;}

the complex conjugate of ours. Their wave functions are the complex conjugates of ours, and every physical prediction is identical, because Ψ2=Ψ2|\Psi|^2 = |\Psi^*|^2.

Select e^{−i(kx − ωt)} in the widget in problem 3 above: the two sides have the right shape but the wrong sign, which is exactly the statement that it needs the other planet’s equation.

6 Trying it relativistically — the Klein–Gordon equation derivation

According to relativity, the momentum pp and energy EE of a particle of mass mm satisfy

E2p2c2=m2c4E^2 - p^2c^2 = m^2c^4

and the velocity of the particle is u=pc2/Eu = pc^2/E.

(a) Assume the motion is described by a wave packet with E=ωE = \hbar\omega and p=kp = \hbar k. Derive the group velocity of the packet and show it equals the particle velocity.

(b) Show that the wave equation

2Ψt2c22Ψx2+m2c42Ψ=0\frac{\partial^2\Psi}{\partial t^2} - c^2\frac{\partial^2\Psi}{\partial x^2} + \frac{m^2c^4}{\hbar^2}\Psi = 0

has solutions Ψ=Aei(ωtkx)\Psi = A\,e^{-i(\omega t - kx)} which could describe a relativistic particle of energy E=ωE = \hbar\omega and momentum p=kp = \hbar k.

💡 Phillips' own hint

(a) Use vgroup=dω/dkv_{\text{group}} = d\omega/dk. (b) Show that Ψ=Aei(ωtkx)\Psi = A e^{-i(\omega t - kx)} is a solution if E2p2c2=m2c4E^2 - p^2c^2 = m^2c^4.

✓ Worked solution

(a) Write the energy–momentum relation in wave variables using E=ωE = \hbar\omega, p=kp = \hbar k:

2ω22k2c2=m2c4\hbar^2\omega^2 - \hbar^2k^2c^2 = m^2c^4

Differentiate both sides with respect to kk, treating ω\omega as ω(k)\omega(k):

22ωdωdk22kc2=0dωdk=kc2ω=kc2ω=pc2E=u2\hbar^2\omega\frac{d\omega}{dk} - 2\hbar^2kc^2 = 0 \quad\Longrightarrow\quad \frac{d\omega}{dk} = \frac{kc^2}{\omega} = \frac{\hbar k c^2}{\hbar\omega} = \frac{pc^2}{E} = u

The group velocity is the particle velocity — exactly as in the non-relativistic case, and by the same reasoning. The requirement that fixed §2.2’s equation is not special to non-relativistic physics.

(b) With Ψ=Aei(ωtkx)\Psi = A e^{-i(\omega t - kx)},

2Ψt2=ω2Ψ,2Ψx2=k2Ψ\frac{\partial^2\Psi}{\partial t^2} = -\omega^2\Psi, \qquad \frac{\partial^2\Psi}{\partial x^2} = -k^2\Psi

Substituting into the equation:

ω2Ψ+c2k2Ψ+m2c42Ψ=0-\omega^2\Psi + c^2k^2\Psi + \frac{m^2c^4}{\hbar^2}\Psi = 0

Divide by Ψ\Psi and multiply by 2\hbar^2:

2ω22c2k2=m2c4E2p2c2=m2c4\hbar^2\omega^2 - \hbar^2c^2k^2 = m^2c^4 \quad\Longleftrightarrow\quad E^2 - p^2c^2 = m^2c^4

which is exactly the relativistic energy–momentum relation. So the plane wave is a solution precisely when it describes a relativistic particle.

Check yourself

0 / 6 answered

  1. 1.For a dispersion relation , what is the ratio ?

  2. 2.In problem 2, why does the packet keep its shape exactly?

  3. 3.Problem 3 shows fails. What exactly goes wrong?

  4. 4.Problem 4's wave is . Why is it worth more than the algebra suggests?

  5. 5.The other planet writes . Which of these is genuinely a convention?

  6. 6.The Klein–Gordon equation reproduces correctly, yet Phillips says its solutions cannot be treated as wave functions. Why?