06-Introduction to Quantum Physics

Summary

Light shows many properties consistent with its nature as being a wave; examples being difffraction and interference. But it also shows many properties that can only be explained by considering light as being a stream of particles, photons (\(\gamma\)). This conflict can be viewed as a wave-particle duality, with a photon as a probability wave.

Particles such as electrons also show similar effects.

The wave-like properties can be interpreted using Heisenberg’s Uncertainty Principle.

Contents

  1. Wave Nature of Light
  2. Particle Nature of Light
    1. Blackbody Radiation & Planck
    2. Photoelectric Effect
      • Energy & Momentum of Photons
    3. Compton Effect
    4. Pair Production
  1. Mathematics of Wave Packets
  2. Uncertainty Principle
  3. Wave Nature of Particles
  4. Equations
  5. References

Wave Nature of Light

  • optical diffraction explained by waves
    • analogous to phenomena in water waves, sound, etc
    • \(\theta \propto \frac{\lambda}{d}\), d is aperture width

  • two-slit interference pattern (Young’s)
    • \(n\lambda = d \times sin\theta\)


  • X-ray diffraction patterns we looked at last week also explained by wave nature of light

But there are problems

  1. Blackbody Radiation

    • classical model of the spectrum of thermal radiation (Rayleigh-Jeans) gives infinities at short wavelengths
    • called ultraviolet catastrophy
    • solved by Planck’s Radiation Law
  2. photoelectric effect

  3. Compton Scattering

  4. Pair production

1. Blackbody Radiation

  • every object emits light because of its temperature
    • hot bodies are brighter (Stefan Boltzman Law)
    • hot bodies \(\implies\) more intense colours (Wien’s Displacement Law)
      • \(infrared \rightarrow crimson \rightarrow yellow \rightarrow blue \rightarrow uv\)

  • spectrum explained by Planck’s Radiation Law

\({\displaystyle u_{\lambda }(\lambda ,T)={\frac {8\pi hc}{\lambda ^{5}}}{\frac {1}{e^{hc/(\lambda k_{\mathrm {B} }T)}-1}}}\)

  • introduces Plank’s constant, \(h = 6.626 \times 10^{-34} Js\)
    • also \(\hbar = \frac{h}{2\pi} = 1.055 \times 10^{-34} Js\)
    • h is the talisman for quantum physics
  • where \(c = 2.99792458 \times 10^{8}m/s\) = speed of light
  • \(k_B = 1.380649 \times 10^{-23} J/K\) = Boltzman’s Constant

Equations for Our Photons

  • \(\omega = {2\pi}{f}\) = angular velocity
  • \(k = \frac{2\pi}{\lambda}\) = wave vector
  • \(p = \frac{h}{\lambda} = \hbar k\) = momentum
  • \(E_{\gamma} = hf = \hbar \omega\)
  • \(E_{\gamma} = \frac{hc}{\lambda} = \hbar k c = pc\)
  • also, photons are spin 1 particles \(\implies\) bosons

2. Photoelectric Effect

  • shine light on metal plate
  • electrons emitted
    • would expect the brighter the light \(\implies\) the stronger the electric field \(\implies\) the more energetic the electrons leaving plate
  • don’t see this
    • energy of electrons depends on light wavelength
    • number of electrons depends on brightness
    • \(KE_{{max}_{e^-}} = hf - \phi\)

  • adjust voltage until just strong enough to stop all electrons
    • \(eV = hf - \phi\)

3. Compton Effect


  • if light is just a wave, scattering off particles won’t effect \(\lambda\)

  • but we do see change in \(\lambda\)

    • have to look pretty carefully
    • works best for x-rays scattering off electrons
  • get \(\Delta \lambda = \lambda - \lambda_0 = \frac{h}{mc}(1-cos \theta)\)

  • energy before = energy after

\(mc^2 + E_o = E_e + E\) \(\implies E_e = E_0 + mc^2 - E\) \(\implies \sqrt{(mc^2)^2+ (p_ec)^2}\) \(= p_oc + mc^2 - pc\) \(\implies \sqrt{(mc)^2+ (p_e)^2}\) \(= p_o + mc - p\)


  • conservation of momentum

\(\vec{p_0} = \vec{p} + \vec{p_e}\) \(\implies \vec{p_e} = \vec{p_0} - \vec{p}\) \(\implies p_e^2 = (\vec{p_0} - \vec{p})\cdot(\vec{p_0} - \vec{p})\) \(\implies p_e^2 = p_0^2 + p^2 - 2p_0 p\; cos\theta\)

  • combining, replacing \(p_e^2\) from energy equation

\((mc)^2 + p_0^2 + p^2 - 2p p_0 cos \theta\) \(= p_0^2 + p^2 -2pp_0 + m^2c^2 + 2p_0mc - 2pmc\)

  • lots of terms cancel

\(-2pp_0 cos \theta = -2p_0p + 2mc(p_0-p)\)

\(p_0p(1-cos\theta) = mc(p_0-p)\) \(\frac{1}{mc}(1-cos\theta) = \frac{1}{p}- \frac{1}{p_0}\)

Compton Shift is Pretty Small

  • photons scattering off electrons at \(\theta = 80 ^{\circ}\)
  • \(\Delta \lambda = \frac{h}{mc} (1 - cos\theta)\)
  • \(= \frac{6.626 \times 10^{-34}}{9.11 \times 10^{-31} \;\times \; 3 \times 10^8}\; \times (1-cos 80^{\circ})\)
  • \(= 2.426 \times 10^{-12} \; \times \; (1 - 0.1736)\)
  • \(= 2.005 \times 10^{-12} m\)
  • \(= 0.002005 \; nm\)
  • gets worse if x-ray doesn’t liberate electron
    • replace \(m = 9.11 \times 10^{-31} kg\) by mass of atom

4. Pair Production

Mathematics of Waves

  • single wave \(A = A_0 sin(kx - \omega t)\)
    • (neat way of expressing this \(A = e^{i(kx - \omega t)}\))
    • solution to equation \(\frac{\partial^2A}{\partial t^2}-(\frac{\omega}{k})^2 \frac{\partial^2A}{\partial x^2} = 0\)
    • angular velocity; \(\omega = 2 \pi f\), where f is the frequency
    • wavenumber; \(k = \frac{2 \pi}{\lambda}\), where \(\lambda\) is the wavelength
    • using \(v = f\lambda\) get \(v = \frac{\omega}{k}\)
    • (this is the phase velocity, \(v_p\))

Add Two Waves of Slightly Different Frequency Together

  • \(A(x, t) = A_0 sin[(k-\Delta k)x - (\omega - \Delta \omega) t] +\) \(A_0 sin[(k+\Delta k)x - (\omega + \Delta \omega) t]\)

  • rearranging

  • \(A(x, t) = A_0 sin[(kx-\omega t) - (\Delta kx - \Delta \omega t)] +\) \(A_0 sin[(kx-\omega t) + (\Delta kx - \Delta \omega t)]\)

  • like adding two sines: \(sin(A+B) + sin(A-B) = 2sin(A)cos(B)\)

  • get: \(A(x, t) = 2 \times A_0 sin(kx - \omega t)\; cos(\Delta kx - \Delta \omega t)\)

  • a sine wave modulated by a much slower cosine wave

  • \(A(x, t) = 2 \times A_0 sin(kx - \omega t)\; cos(\Delta kx - \Delta \omega t)\)

  • The sine wave has velocity \(v_p = \omega / k\)

  • The longer cosine wave modulating it has velocity \(v_g = \Delta \omega / \Delta k\)

  • this last we call the Group Velocity

Example

  • Add the two waves \(A_0 sin(k_1x - \omega_1 t)\) and \(A_0 sin(k_2x - \omega_2 t)\) where \(k_1 = 6.4 \; rads/m\), \(\omega_1 = 9.2 \; rads/s\), \(k_2 = 6.0 \; rads/m\), and \(\omega_2 = 9.0 \; rads/s\)

  • the phase velocity is \(\omega / k\) where \(\omega = \frac{(\omega_1 + \omega_2)}{2}\) and \(k = \frac{(k_1 + k_2)}{2}\) giving \(v_p = 9.1 / 6.2 = 1.47 m/s\)

  • the group velocity is \(\Delta \omega / \Delta k\) where \(\Delta \omega = \frac{(\omega_1 - \omega_2)}{2}\) and \(\Delta k = \frac{(k_1 - k_2)}{2}\) giving \(v_g = 0.2 / 0.4 = 0.50 m/s\)

Adding More than Two Waves

  • the two wave example above gives the general principle, but in practice many more waves combine to form a wave packet

    • they’ll all have closely spaced frequencies (\(\frac{\omega}{2\pi}\))

    • and closely spaced wavenumbers, k

  • the average values for \(\omega\) and k will generate the phase velocity

  • the way in which \(\omega\) and k change across the wavepacket, \(d \omega / dk\), will give the group velocity

  • the group velocity is of greater physical significance

Wavepacket of 500 Sine Waves

Credit: Institute of Sound and Vibration Research

Heisenberg’s Uncertainty Principle

  • light diffraction can be though of as an illustration of the uncertainty principle
  • slit width \(d\) so therefore uncertainty in photon position of \(\Delta x = d\)
  • width of diffraction pattern = \(\Delta \theta = \frac{\lambda}{d}\)
    • range of momentum values = \(\Delta p = p \Delta \theta = p \frac{\lambda}{d}\)
    • but \(p = \frac{h}{\lambda}\)
    • substituting we get \(\Delta p = \frac{h}{\lambda} \frac{\lambda}{d} = \frac{h}{d}\)
    • but \(\Delta x = d\), so \(\Delta p = \frac{h}{\Delta x}\)
    • \(\implies \Delta x \Delta p \ge h\)

Wave Nature of Other Stuff

  • electrons fired through a double slit apparatus also show a diffraction / interference pattern

    • Davison Germer experiment with beam of electrons at nickel plate
    • even when we dial the intensity way down, one electron at a time, we see the same pattern
    • and this is also true for light, one photon at a time

  • we have \(E = \hbar \omega\)
  • for mass particles we have \(E = \frac{1}{2} m v^2 = \frac{p^2}{2m}\)
  • We need a differential equation that can work with the equation for a plane wave and yet give us the correct for the relation between energy and momentum
    • Need to be proportional to \(k^2\), not \(k\)
    • How about differentiating twice on t but just once on x?

  • something like \(\frac{\partial A}{\partial t} = \propto \frac{\partial^2A}{\partial x^2}\)
  • or, replacing \(A\) with \(\Psi\): \(\frac{\partial \Psi}{\partial t} = \propto \frac{\partial^2 \Psi}{\partial x^2}\)
  • if we put in the plan wave solution, \(\Psi = e^{i(kx-\omega t)}\) get
  • \(-k^2 = i \propto \omega\)
  • if we use \(p = \hbar k\) and \(E = \frac{p^2}{2m}\) get:
    • \(\propto = -2mi/\hbar\)
    • feed this back in to our equation and rearrange to get:

\(i \hbar \frac{\partial \Psi}{\partial t} = - \frac{\hbar^2}{2m} \frac{\partial ^2 \Psi}{\partial x^2}\)

  • this is in free space, no forces
  • if we add a potential, \(V\), we get

\(\; \; i \hbar \frac{\partial \Psi}{\partial t} = - \frac{\hbar^2}{2m} \frac{\partial ^2 \Psi}{\partial x^2} + V\Psi\)

Equations

  • \(A = A_0 sin(kx - \omega t)\)
  • \(A = e^{i(kx - \omega t)}\))
  • \(\frac{\partial^2A}{\partial t^2}-(\frac{\omega}{k})^2 \frac{\partial^2A}{\partial x^2} = 0\)
  • \(\omega = 2 \pi f\)
  • \(k = \frac{2 \pi}{\lambda}\)
  • \(v = \frac{\omega}{k}\)
  • \(p = \frac{h}{\lambda} = \hbar k\)
  • \(E = hf = \frac{hc}{\lambda}= \hbar c k\)
  • \(v_p = \omega / k\)
  • \(v_g = \partial \omega / \partial k\)
  • \(\Delta \lambda = \frac{h}{mc} (1 - cos \theta)\)

References