Module VI: Semiconductor Physics - Question Solutions
Question 1: Fermi-Dirac Distribution Function
| Symbol | Name | Description |
|---|---|---|
| f(E) | Fermi Function | Probability that an energy state E is occupied by an electron (ranges from 0 to 1) |
| E | Energy Level | The energy of the quantum state being considered (in Joules or eV) |
| EF | Fermi Energy | The energy level at which the probability of occupation is exactly 0.5 (50%) |
| kB | Boltzmann Constant | 1.38 × 10⁻²³ J/K or 8.617 × 10⁻⁵ eV/K |
| T | Absolute Temperature | Temperature in Kelvin |
| kBT | Thermal Energy | ≈ 0.026 eV at room temperature (300K) |
- At E = EF: f(EF) = 1/[1 + e⁰] = 1/2 = 0.5 (always 50% probability)
- At T = 0K: f(E) = 1 for E < EF and f(E) = 0 for E > EF (step function)
- At T > 0K: The distribution smooths out; some electrons above EF, some empty states below EF
- For E >> EF: f(E) ≈ exp[-(E - EF)/kBT] (Maxwell-Boltzmann limit)
- For E << EF: f(E) ≈ 1 (states are almost certainly filled)
- Describes the statistical distribution of electrons in energy states at thermal equilibrium
- Essential for understanding electrical conductivity in metals and semiconductors
- Accounts for Pauli exclusion principle (fermions cannot occupy same state)
- Used to calculate carrier concentrations in semiconductors
Question 2: Fermi Level in Intrinsic Semiconductor
Step 1: Electron concentration in conduction band:
where NC is the effective density of states in conduction band:
Step 2: Hole concentration in valence band:
where NV is the effective density of states in valence band:
Step 3: For an intrinsic semiconductor, the number of electrons equals the number of holes:
Step 4: Equating the two expressions:
Step 5: Taking natural logarithm of both sides:
Step 6: Rearranging:
Step 7: Solving for EF:
Step 8: Since NC/NV = (me*/mh*)^(3/2):
Special Case: If me* = mh* (equal effective masses), then ln(1) = 0:
- For most semiconductors, me* ≈ mh*, so EF lies very close to the middle
- The second term is temperature-dependent and usually small at room temperature
- At T = 0K, Fermi level is exactly at the midpoint
- This result applies only to intrinsic (undoped) semiconductors
Question 3: Mobility of Electrons - Numerical
Units: m²/V·s or cm²/V·s
- Higher mobility means electrons move more freely through the material
- Mobility depends on: temperature, impurity concentration, crystal structure
- Related to mean free time (τ) between collisions: μ = eτ/m*
- Conductivity is directly proportional to mobility: σ = neμ
- Resistivity of Cu, ρ = 1.72 × 10⁻⁸ Ω·m
- Electron concentration, n = 10.41 × 10²⁸ m⁻³
- Charge of electron, e = 1.6 × 10⁻¹⁹ C
The relationship between conductivity, carrier concentration, and mobility:
Since σ = 1/ρ:
| Material | Electron Mobility (cm²/V·s) |
|---|---|
| Copper | ~35 |
| Silicon (intrinsic) | ~1350 |
| Germanium | ~3900 |
| GaAs | ~8500 |
Question 4: Effect of Indium Doping on Silicon
Given: Concentration of silicon atoms = 5 × 10²⁸ /m³
Intrinsic conductivity of silicon = 4.4 × 10⁻⁴ /Ω-m
Mobility of holes = 0.048 m²/V·sec
- Concentration of Si atoms, NSi = 5 × 10²⁸ m⁻³
- Doping ratio = 1 in 10⁶ (every millionth atom)
- Intrinsic conductivity, σᵢ = 4.4 × 10⁻⁴ Ω⁻¹m⁻¹
- Mobility of holes, μₕ = 0.048 m²/V·s
- Charge of electron, e = 1.6 × 10⁻¹⁹ C
At room temperature, all acceptor atoms are ionized, so:
(This is much greater than intrinsic carrier concentration ni ≈ 10¹⁶ m⁻³)
For a p-type semiconductor, conductivity is dominated by holes:
Intrinsic resistivity:
Ratio of conductivities:
| Property | Intrinsic Si | Doped Si (with In) |
|---|---|---|
| Type | Intrinsic | p-type |
| Conductivity | 4.4 × 10⁻⁴ Ω⁻¹m⁻¹ | 384 Ω⁻¹m⁻¹ |
| Resistivity | 2273 Ω·m | 2.6 × 10⁻³ Ω·m |
The doped silicon becomes a p-type semiconductor with σ = 384 Ω⁻¹m⁻¹
- Silicon becomes p-type semiconductor (majority carriers are holes)
- Conductivity increases dramatically (~10⁶ times)
- Fermi level shifts towards the valence band
- Hole concentration >> electron concentration
- Temperature dependence of conductivity changes