10.3 Modern Physics
Key Takeaways
- The photoelectric effect was discovered by Heinrich Hertz in 1887 and explained by Einstein in 1905 using light quanta (photons)
- Einstein's photoelectric equation KE_max = hf − Φ defines a threshold frequency f₀ = Φ/h below which no electrons are emitted, regardless of intensity
- Bohr's 1913 model quantized electron orbits; the nucleus (Rutherford, 1911) and Bohr's quantization underpin atomic structure questions
- Mass–energy equivalence E = mc² relates the energy released in fission (splitting a heavy nucleus) and fusion (joining light nuclei) to the mass defect
The Photoelectric Effect
The photoelectric effect is the emission of electrons from a metal surface when light of sufficiently high frequency falls on it. It was discovered by Heinrich Hertz in 1887 during his experiments with spark-gap transmitters, and explained by Albert Einstein in 1905 using the idea that light delivers energy in discrete packets called photons, each carrying energy E = hf (h = Planck's constant ≈ 6.63 × 10⁻³⁴ J·s).
Einstein's photoelectric equation is:
KE_max = hf − Φ
where Φ (the work function) is the minimum energy needed to eject an electron from the metal, and f is the frequency of the incident light. The threshold frequency is:
f₀ = Φ / h
Below f₀, no electrons are emitted no matter how intense the light — a result classical wave theory could not explain and which established the quantum (particle) nature of light.
Worked example 1. A metal has a work function of 2.0 eV. Find the threshold frequency. (1 eV = 1.6 × 10⁻¹⁹ J, h = 6.63 × 10⁻³⁴ J·s.)
Φ = 2.0 × 1.6 × 10⁻¹⁹ = 3.2 × 10⁻¹⁹ J. f₀ = Φ / h = 3.2 × 10⁻¹⁹ / 6.63 × 10⁻³⁴ ≈ 4.8 × 10¹⁴ Hz (red/orange light).
Dual Nature of Light
Light exhibits wave–particle duality: it propagates as a wave (interference, diffraction, polarization) but interacts with matter in discrete quanta (photons). The photoelectric effect and the Compton effect demonstrate the particle side; Young's double-slit experiment demonstrates the wave side. de Broglie extended duality to matter: λ = h/p for any particle with momentum p.
Atomic Models
The evolution of atomic theory is a common PAF topic:
- Dalton (1808) — solid, indivisible sphere.
- J.J. Thomson (1897) — discovered the electron; 'plum-pudding' model with electrons embedded in a positive sphere.
- Rutherford (1911) — gold-foil experiment; dense, positively charged nucleus with electrons orbiting at a distance.
- Bohr (1913) — electrons in quantized circular orbits; photons emitted/absorbed on transitions: ΔE = hf.
- Quantum mechanical model — electrons described by probability clouds (orbitals), not fixed paths.
Bohr's model successfully explained the hydrogen spectrum and introduced the idea of quantized energy levels — a concept that underpins lasers, LEDs, and many cockpit display technologies.
Nuclear Physics: Fission, Fusion, and E = mc²
Einstein's mass–energy equivalence:
E = mc²
states that mass and energy are interchangeable. In any nuclear reaction, the mass defect Δm is released as energy:
- Nuclear fission — a heavy nucleus (e.g., U-235, Pu-239) splits into smaller nuclei when struck by a neutron, releasing ~200 MeV per fission and additional neutrons that sustain a chain reaction. Basis of nuclear power plants and atomic bombs.
- Nuclear fusion — light nuclei (e.g., hydrogen isotopes deuterium + tritium) combine into a heavier nucleus (helium), releasing even more energy per unit mass. Powers the Sun and hydrogen bombs; the goal of controlled fusion research.
Worked example 2. A reaction has a mass defect of 1.0 × 10⁻²⁸ kg. How much energy is released? (c = 3.0 × 10⁸ m/s.)
E = mc² = 1.0 × 10⁻²⁸ × (3.0 × 10⁸)² = 1.0 × 10⁻²⁸ × 9.0 × 10¹⁶ = 9.0 × 10⁻¹² J.
Photoelectric KE_max — Worked Example
Worked example 3. Light of frequency 8.0 × 10¹⁴ Hz falls on a metal whose work function is 2.0 eV. Find the maximum kinetic energy of the emitted electrons (in eV). (h = 6.63 × 10⁻³⁴ J·s, 1 eV = 1.6 × 10⁻¹⁹ J.)
Photon energy E = hf = 6.63 × 10⁻³⁴ × 8.0 × 10¹⁴ = 5.30 × 10⁻¹⁹ J = 5.30 × 10⁻¹⁹ / 1.6 × 10⁻¹⁹ ≈ 3.31 eV. Work function Φ = 2.0 eV. So KE_max = 3.31 − 2.0 = 1.31 eV. The surplus (1.31 eV) appears as the electron's kinetic energy; the threshold frequency for this metal is f₀ = Φ/h ≈ 4.8 × 10¹⁴ Hz, and since 8.0 × 10¹⁴ Hz > f₀, emission occurs.
de Broglie Wavelength — Worked Example
Worked example 4. Find the de Broglie wavelength of an electron moving at 1.0 × 10⁷ m/s. (m_e = 9.11 × 10⁻³¹ kg, h = 6.63 × 10⁻³⁴ J·s.)
p = m v = 9.11 × 10⁻³¹ × 1.0 × 10⁷ = 9.11 × 10⁻²⁴ kg·m/s. λ = h/p = 6.63 × 10⁻³⁴ / 9.11 × 10⁻²⁴ ≈ 7.28 × 10⁻¹¹ m (about 0.073 nm, comparable to atomic spacing — which is why electron microscopes resolve atoms).
Threshold Frequency vs Intensity — The Key Trap
The single most-tested modern-physics trap: below threshold frequency, no emission occurs, no matter how large the intensity. Classical wave theory predicted that increasing intensity should always eventually eject electrons; experiment showed it does not. Only increasing the frequency (or shortening the wavelength) beyond f₀ helps. Once above threshold, increasing intensity ejects more electrons per second (larger photocurrent) but does not change their maximum kinetic energy — only increasing frequency raises KE_max.
Fission vs Fusion — Quick Comparison
| Feature | Fission | Fusion |
|---|---|---|
| Reaction | Heavy nucleus splits | Light nuclei combine |
| Fuel | U-235, Pu-239 | D + T (hydrogen isotopes) |
| Energy per kg | Lower | Higher |
| By-products | Radioactive fragments, neutrons | Helium (clean) |
| Application | Nuclear reactors, atom bombs | Stars, hydrogen bombs, fusion research |
| Chain reaction | Self-sustaining (neutron-multiplying) | Requires extreme T and pressure |
Both release energy because the products have higher binding energy per nucleon — the mass defect Δm is converted via E = mc².
Key Discoveries Timeline
| Year | Scientist | Discovery |
|---|---|---|
| 1897 | J.J. Thomson | Electron |
| 1905 | Einstein | Photoelectric explanation; special relativity (E = mc²) |
| 1911 | Rutherford | Atomic nucleus (gold-foil experiment) |
| 1913 | Bohr | Quantized atomic model |
| 1887 | Hertz | Photoelectric effect (discovery) |
| 1939 | Hahn/Strassmann | Nuclear fission of uranium |
| 1924 | de Broglie | Wave nature of matter (λ = h/p) |
Aviation & Defence Links
- Photoelectric sensors and lidar — used in terrain-following and obstacle-avoidance systems.
- Radar relies on photon (electromagnetic wave) reflection — the same wave–particle duality at radio frequencies.
- Nuclear propulsion and weapons — Pakistan's deterrent relies on fission and boosted-fission designs; understanding E = mc² is therefore operationally relevant for PAF officers.
Who discovered the photoelectric effect, and who explained it theoretically?
In the photoelectric effect, what happens if light below the threshold frequency is shone on a metal, but with very high intensity?
A nuclear reaction has a mass defect of 2.0 × 10⁻²⁹ kg. Using E = mc² with c = 3.0 × 10⁸ m/s, the energy released is:
Which atomic model first introduced quantized electron orbits to explain the hydrogen spectrum?