Example – Photon momentum of green light (\(\lambda = 550\;\text{nm}\)):
\[
p = \frac{h}{\lambda}= \frac{6.626\times10^{-34}\;\text{J·s}}{5.5\times10^{-7}\;\text{m}}
= 1.20\times10^{-27}\;\text{kg·m s}^{-1}
\]
Note: because photons travel at \(c\), the same result follows from \(p=E/c\).
The experiment shows that electrons are emitted only when the incident light frequency exceeds a material‑specific threshold.
\[
hf = \Phi + \tfrac12 mv^{2}\qquad\text{or}\qquad K_{\max}=hf-\Phi
\]
Worked example (A‑level style):
\[
E_{\text{photon}}=\frac{hc}{\lambda}= \frac{1240\;\text{eV·nm}}{400\;\text{nm}}=3.10\;\text{eV}
\]
\[
K{\max}=E{\text{photon}}-\Phi = 3.10-2.0 = 1.10\;\text{eV}
\]
Any particle with momentum \(p\) is associated with a wavelength
\[
\boxed{\lambda = \frac{h}{p}}
\]
\[
p = \sqrt{2m_{e}K}\qquad\Longrightarrow\qquad
\lambda = \frac{h}{\sqrt{2m_{e}K}}
\]
\[
p = \frac{1}{c}\sqrt{K^{2}+2K\,m_{e}c^{2}}\qquad\Longrightarrow\qquad
\lambda = \frac{h}{p}
\]
When to use the relativistic formula
For \(K = 200\;\text{keV}\):
Non‑relativistic \(\lambda_{\text{NR}} = 2.74\times10^{-12}\;\text{m}\)
Relativistic \(\lambda_{\text{R}} = 2.48\times10^{-12}\;\text{m}\) (≈ 9 % shorter).
The difference is measurable in high‑energy electron diffraction.
\[
\lambda = \frac{h}{\sqrt{2m_{e}eV}}
\]

Sharp intensity maxima appear at angles satisfying Bragg’s law
\[
2d\sin\theta = n\lambda \qquad (n=1,2,\dots)
\]
Using the measured \(\theta\) and the known lattice spacing \(d\) (Ni (111) planes, \(d=0.215\;\text{nm}\)), the calculated \(\lambda\) matches the de Broglie value – a direct confirmation of matter‑wave behaviour.
When a coherent electron beam passes through two narrow slits (separation \(s\)), an interference pattern of bright and dark fringes appears on a distant screen.
Fringe‑spacing example (A‑level style):
\[
y_1 = \frac{L\lambda}{s}= \frac{0.5\times1.00\times10^{-10}}{1.0\times10^{-6}} = 5.0\times10^{-5}\;\text{m}=50\;\mu\text{m}
\]
When X‑rays scatter from loosely bound electrons, their wavelength increases by
\[
\Delta\lambda = \lambda' - \lambda = \frac{h}{m_{e}c}\,(1-\cos\theta)
\]
where \(\theta\) is the scattering angle.
Worked example:
\[
\Delta\lambda = 2.43\times10^{-12}\,\text{m}\;(1-\cos60^{\circ}) = 1.22\times10^{-12}\;\text{m}
\]
Thermal neutrons (\(\lambda\approx 0.18\;\text{nm}\)) are diffracted by crystal lattices in the same way as X‑rays, providing a powerful tool for studying magnetic structures. Mentioned here to show that wave‑particle duality is not limited to electrons or photons.
If electrons were purely particles, the angular distribution would be smooth and roughly isotropic (Rutherford‑type scattering). The discrete, angle‑dependent peaks are therefore a hallmark of wave behaviour.
When an electron in an atom moves between two discrete energy levels \(Ei\) and \(Ef\), a photon of frequency \(f\) is emitted or absorbed:
\[
\boxed{hf = \Delta E = |Ei - Ef|}
\]
\[
\frac{1}{\lambda}=R_{\!H}\!\left(\frac{1}{2^{2}}-\frac{1}{n^{2}}\right),\qquad n=3,4,5,\dots
\]
\[
\frac{1}{\lambda}=R_{\!H}\!\left(\frac{1}{1^{2}}-\frac{1}{n^{2}}\right),\qquad n=2,3,4,\dots
\]
Example: \(n=2\to1\) (Lyman‑α) gives \(\lambda = 121.6\;\text{nm}\).
| Aspect | Particle‑only model | Wave model (observed) |
|---|---|---|
| Angular distribution | Continuous, roughly isotropic (modulo geometric factors) | Discrete Bragg peaks at specific \(\theta\) |
| Dependence on crystal plane spacing \(d\) | None | Peak angles obey \(2d\sin\theta = n\lambda\) |
| Effect of electron kinetic energy | Higher energy → more forward‑scattering | Higher energy → shorter \(\lambda\); peaks shift according to Bragg law |
| Origin of intensity pattern | Random collisions | Coherent interference of matter waves |
Given: electrons accelerated through \(V = 150\;\text{V}\); Ni crystal plane spacing \(d = 0.215\;\text{nm}\).
Outline a modification of the Davisson–Germer set‑up to test the relativistic correction for electrons accelerated to \(200\;\text{keV}\).
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