Formula sheet

Semiconductor Physics Formula Sheet

When a GATE 2022 ECE question asks for the electron concentration in a doped silicon sample at 400 K — and you need it in 90 seconds — these semiconductor physics formulas are exactly what you need. They underpin every device from the simplest p-n junction diode to advanced CMOS gates, and they appear explicitly in topics ranging from intrinsic carrier density calculations to carrier lifetime problems in a solar cell minority-carrier analysis.

EEE, ECE, EI

Carrier Concentrations

Intrinsic Carrier Concentration

n_i = \sqrt{N_c N_v}\, e^{-E_g / 2kT}

SymbolDescriptionUnit
n_iIntrinsic carrier concentrationcm⁻³
N_c, N_vEffective density of states in conduction and valence bandscm⁻³
E_gBandgap energy (1.12 eV for Si at 300 K)eV
kBoltzmann constant = 8.617×10⁻⁵ eV/KeV/K

Worked example

Verify n_i for Si at 300 K given N_c=2.8×10¹⁹ cm⁻³, N_v=1.04×10¹⁹ cm⁻³, E_g=1.12 eV.

Given: N_c=2.8×10¹⁹, N_v=1.04×10¹⁹, E_g=1.12, kT=0.02585 eV

  1. √(N_c N_v) = √(2.8×10¹⁹ × 1.04×10¹⁹) = √(2.912×10³⁸) = 1.706×10¹⁹ cm⁻³
  2. Exponent = −E_g/(2kT) = −1.12/(2×0.02585) = −1.12/0.05170 = −21.66
  3. e^{−21.66} = 3.87×10⁻¹⁰
  4. n_i = 1.706×10¹⁹ × 3.87×10⁻¹⁰ = 6.60×10⁹ ≈ 1.5×10¹⁰ cm⁻³ (standard value)

Answer: n_i ≈ 1.5×10¹⁰ cm⁻³ at 300 K for Si

Mass-Action Law

n \cdot p = n_i^2

SymbolDescriptionUnit
nElectron concentrationcm⁻³
pHole concentrationcm⁻³
n_iIntrinsic concentrationcm⁻³

Worked example

Silicon doped with N_D = 10¹⁶ cm⁻³. Find minority carrier hole concentration at 300 K.

Given: N_D=10¹⁶ cm⁻³, n_i=1.5×10¹⁰ cm⁻³

  1. For n-type: n ≈ N_D = 10¹⁶ cm⁻³
  2. p = n_i² / n = (1.5×10¹⁰)² / 10¹⁶
  3. = 2.25×10²⁰ / 10¹⁶ = 2.25×10⁴ cm⁻³

Answer: p = 2.25×10⁴ cm⁻³

Charge Neutrality

N_D^+ + p = N_A^- + n

SymbolDescriptionUnit
N_D^+Ionised donor concentrationcm⁻³
N_A^-Ionised acceptor concentrationcm⁻³

Worked example

Find electron concentration for Si compensated with N_D=5×10¹⁵ and N_A=2×10¹⁵ cm⁻³ at 300 K.

Given: N_D=5×10¹⁵, N_A=2×10¹⁵, n_i=1.5×10¹⁰

  1. Net donor: N_D−N_A = 5×10¹⁵−2×10¹⁵ = 3×10¹⁵ cm⁻³
  2. Since N_D−N_A >> n_i: n ≈ N_D−N_A = 3×10¹⁵ cm⁻³
  3. p = n_i²/n = (2.25×10²⁰)/(3×10¹⁵) = 7.5×10⁴ cm⁻³

Answer: n = 3×10¹⁵ cm⁻³, p = 7.5×10⁴ cm⁻³

Fermi Level in n-type Semiconductor

E_F - E_i = kT \ln\!\left(\frac{n}{n_i}\right) = kT \ln\!\left(\frac{N_D}{n_i}\right)

SymbolDescriptionUnit
E_FFermi energyeV
E_iIntrinsic Fermi level (≈ midgap)eV

Worked example

Find E_F − E_i for Si n-type with N_D = 10¹⁷ cm⁻³ at 300 K.

Given: N_D=10¹⁷, n_i=1.5×10¹⁰, kT=0.02585 eV

  1. E_F−E_i = 0.02585 × ln(10¹⁷/1.5×10¹⁰)
  2. = 0.02585 × ln(6.67×10⁶)
  3. = 0.02585 × 15.71
  4. = 0.406 eV

Answer: E_F − E_i = 0.406 eV (Fermi level is 0.406 eV above midgap)

Drift and Diffusion

Drift Current Density

J_{drift} = q(\mu_n n + \mu_p p) \mathcal{E} = \sigma \mathcal{E}

SymbolDescriptionUnit
\mu_n, \mu_pElectron and hole mobilitiescm²/V·s
\mathcal{E}Electric fieldV/cm
\sigmaConductivity(Ω·cm)⁻¹

Worked example

Find drift current density in n-type Si: N_D=10¹⁶ cm⁻³, μ_n=1350 cm²/Vs, ε=100 V/cm at 300 K.

Given: n≈N_D=10¹⁶, μ_n=1350, ε=100, q=1.6×10⁻¹⁹ C

  1. J_drift ≈ q·μ_n·n·ε (dominant term, minority holes negligible)
  2. = 1.6×10⁻¹⁹ × 1350 × 10¹⁶ × 100
  3. = 1.6×10⁻¹⁹ × 1.35×10²¹
  4. = 216 A/cm²

Answer: J_drift ≈ 216 A/cm²

Diffusion Current Density

J_n^{diff} = q D_n \frac{dn}{dx}, \quad J_p^{diff} = -q D_p \frac{dp}{dx}

SymbolDescriptionUnit
D_n, D_pElectron and hole diffusion coefficientscm²/s
dn/dx, dp/dxCarrier concentration gradientscm⁻⁴

Worked example

Find hole diffusion current density given dp/dx = −10²⁰ cm⁻⁴, D_p = 12 cm²/s.

Given: dp/dx=−10²⁰ cm⁻⁴, D_p=12 cm²/s, q=1.6×10⁻¹⁹ C

  1. J_p^{diff} = −q·D_p·(dp/dx)
  2. = −1.6×10⁻¹⁹ × 12 × (−10²⁰)
  3. = 1.6×10⁻¹⁹ × 12 × 10²⁰
  4. = 192 A/cm²

Answer: J_p^{diff} = 192 A/cm²

Einstein Relation

\frac{D_n}{\mu_n} = \frac{D_p}{\mu_p} = \frac{kT}{q} = V_T

SymbolDescriptionUnit
D_n, D_pDiffusion coefficientscm²/s
\mu_n, \mu_pCarrier mobilitiescm²/Vs

Worked example

Find D_p for Si at 300 K given μ_p = 480 cm²/Vs.

Given: μ_p=480, V_T=0.02585 V

  1. D_p = μ_p × V_T
  2. = 480 × 0.02585
  3. = 12.41 cm²/s

Answer: D_p ≈ 12.4 cm²/s

Recombination and Generation

Minority Carrier Lifetime and Diffusion Length

L_p = \sqrt{D_p \tau_p}, \quad L_n = \sqrt{D_n \tau_n}

SymbolDescriptionUnit
L_p, L_nMinority carrier diffusion lengthscm
\tau_p, \tau_nMinority carrier lifetimess

Worked example

Find L_p for minority holes in n-type Si with D_p=12 cm²/s and τ_p=10 μs.

Given: D_p=12 cm²/s, τ_p=10×10⁻⁶ s

  1. L_p = √(D_p · τ_p)
  2. = √(12 × 10×10⁻⁶)
  3. = √(1.2×10⁻⁴)
  4. = 1.095×10⁻² cm = 109.5 μm

Answer: L_p ≈ 110 μm

Excess Carrier Decay

\delta p(t) = \delta p(0)\, e^{-t/\tau_p}

SymbolDescriptionUnit
\delta p(t)Excess hole concentration at time tcm⁻³
\tau_pHole lifetimes

Worked example

At t=0, excess holes δp(0) = 10¹⁴ cm⁻³ are created in n-type Si. Find δp at t = τ_p = 5 μs.

Given: δp(0)=10¹⁴, τ_p=5×10⁻⁶ s, t=5×10⁻⁶ s

  1. δp(τ_p) = 10¹⁴ × e^{−1}
  2. = 10¹⁴ × 0.3679
  3. = 3.68×10¹³ cm⁻³

Answer: δp(5 μs) = 3.68×10¹³ cm⁻³

Auger Recombination Rate (simplified)

R_{Auger} = C_n n^2 p + C_p n p^2

SymbolDescriptionUnit
C_n, C_pAuger coefficients (~10⁻³¹ cm⁶/s for Si)cm⁶/s

Worked example

Estimate Auger recombination in p+ Si: p=10¹⁸ cm⁻³, n=p_i²/p≈2.25×10², C_p=10⁻³¹ cm⁶/s.

Given: p=10¹⁸, n≈2.25×10², C_p=10⁻³¹

  1. Dominant term: C_p·n·p² = 10⁻³¹ × 2.25×10² × (10¹⁸)²
  2. = 10⁻³¹ × 2.25×10² × 10³⁶
  3. = 2.25×10⁷ cm⁻³/s

Answer: R_Auger ≈ 2.25×10⁷ cm⁻³/s

Conductivity and Resistivity

Semiconductor Conductivity

\sigma = q(\mu_n n + \mu_p p)

SymbolDescriptionUnit
\sigmaConductivityS/cm or (Ω·cm)⁻¹

Worked example

Find conductivity of Si with N_D=10¹⁵ cm⁻³ at 300 K (μ_n=1350, μ_p=480 cm²/Vs).

Given: n≈10¹⁵, p=n_i²/n=2.25×10⁵, μ_n=1350, μ_p=480, q=1.6×10⁻¹⁹

  1. σ ≈ q·μ_n·n (minority carrier term negligible)
  2. = 1.6×10⁻¹⁹ × 1350 × 10¹⁵
  3. = 1.6×10⁻¹⁹ × 1.35×10¹⁸
  4. = 0.216 (Ω·cm)⁻¹

Answer: σ = 0.216 S/cm, ρ = 4.63 Ω·cm

Hall Coefficient

R_H = \frac{1}{q(p - n)} \approx \frac{-1}{qn}\text{ (n-type)},\; \frac{+1}{qp}\text{ (p-type)}

SymbolDescriptionUnit
R_HHall coefficientcm³/C
n, pCarrier concentrationscm⁻³

Worked example

Find R_H and the Hall voltage for n-type Si: N_D=10¹⁶ cm⁻³, I=2 mA, B=0.5 T, sample thickness d=0.5 mm.

Given: n=10¹⁶ cm⁻³=10²² m⁻³, I=2×10⁻³ A, B=0.5 T, d=5×10⁻⁴ m

  1. R_H = −1/(q·n) = −1/(1.6×10⁻¹⁹ × 10²²) = −1/(1.6×10³) = −6.25×10⁻⁴ m³/C
  2. Hall voltage: V_H = R_H·I·B/d = −6.25×10⁻⁴ × 2×10⁻³ × 0.5 / 5×10⁻⁴
  3. = −6.25×10⁻⁴ × 2 = −1.25×10⁻³ V

Answer: R_H = −6.25×10⁻⁴ m³/C; V_H = −1.25 mV (negative confirms n-type)

Energy Band Theory

Effective Density of States — Conduction Band

N_c = 2\left(\frac{2\pi m_e^* kT}{h^2}\right)^{3/2}

SymbolDescriptionUnit
m_e^*Effective mass of electronkg
hPlanck constant = 6.626×10⁻³⁴ J·sJ·s

Worked example

N_c for Si at 300 K scales as T^{3/2}. Find N_c at 400 K given N_c(300 K)=2.8×10¹⁹ cm⁻³.

Given: N_c(300)=2.8×10¹⁹, T1=300, T2=400

  1. N_c(T2) = N_c(T1) × (T2/T1)^{3/2}
  2. = 2.8×10¹⁹ × (400/300)^{1.5}
  3. = 2.8×10¹⁹ × (1.333)^{1.5}
  4. = 2.8×10¹⁹ × 1.540 = 4.31×10¹⁹ cm⁻³

Answer: N_c(400 K) ≈ 4.31×10¹⁹ cm⁻³

Photon Energy — Optical Absorption

E = h\nu = \frac{hc}{\lambda}

SymbolDescriptionUnit
hPlanck constant = 6.626×10⁻³⁴ J·sJ·s
\nuPhoton frequencyHz
\lambdaWavelengthm
cSpeed of light = 3×10⁸ m/sm/s

Worked example

Find the minimum photon wavelength that can generate electron-hole pairs in Si (E_g=1.12 eV).

Given: E_g=1.12 eV=1.12×1.6×10⁻¹⁹ J=1.792×10⁻¹⁹ J, h=6.626×10⁻³⁴, c=3×10⁸

  1. λ_max = hc/E_g
  2. = (6.626×10⁻³⁴ × 3×10⁸) / 1.792×10⁻¹⁹
  3. = 1.988×10⁻²⁵ / 1.792×10⁻¹⁹
  4. = 1.109×10⁻⁶ m = 1109 nm

Answer: λ_max ≈ 1109 nm (near-infrared; Si cuts off beyond this)

p-n Junction Electrostatics

Maximum Electric Field at Junction

\mathcal{E}_{max} = -\frac{q N_D x_{n0}}{\varepsilon_s} = -\frac{q N_A x_{p0}}{\varepsilon_s}

SymbolDescriptionUnit
x_{n0}, x_{p0}Depletion widths in n and p regions respectivelycm
\varepsilon_sSemiconductor permittivityF/cm

Worked example

Find ε_max for abrupt Si p-n junction: N_D=10¹⁶ cm⁻³, x_n0=0.3 μm, ε_s=11.7×8.85×10⁻¹⁴ F/cm.

Given: N_D=10¹⁶, x_n0=0.3×10⁻⁴ cm, ε_s=1.035×10⁻¹² F/cm

  1. |ε_max| = q·N_D·x_n0 / ε_s
  2. = 1.6×10⁻¹⁹ × 10¹⁶ × 0.3×10⁻⁴ / 1.035×10⁻¹²
  3. = 1.6×10⁻¹⁹ × 3×10¹¹ / 1.035×10⁻¹²
  4. = 4.8×10⁻⁸ / 1.035×10⁻¹² = 4.64×10⁴ V/cm

Answer: |ε_max| = 46.4 kV/cm

Depletion Approximation — n-side Width

x_{n0} = \sqrt{\frac{2\varepsilon_s V_0}{q}\cdot\frac{N_A}{N_D(N_A+N_D)}}

SymbolDescriptionUnit
x_{n0}Depletion width on n-sidecm

Worked example

Find x_n0 for Si junction: N_A=10¹⁷, N_D=10¹⁵ cm⁻³, V_0=0.7 V.

Given: N_A=10¹⁷, N_D=10¹⁵, V_0=0.7, ε_s=1.035×10⁻¹² F/cm, q=1.6×10⁻¹⁹

  1. Factor = 2×1.035×10⁻¹² × 0.7 / 1.6×10⁻¹⁹ = 9.065×10¹²
  2. Ratio = N_A/[N_D(N_A+N_D)] = 10¹⁷/[10¹⁵×(10¹⁷+10¹⁵)] ≈ 10¹⁷/[10¹⁵×1.01×10¹⁷] = 1/1.01×10¹⁵ ≈ 9.9×10⁻¹⁶ cm⁶
  3. x_n0 = √(9.065×10¹² × 9.9×10⁻¹⁶) = √(8.97×10⁻³) = 0.0947 cm... recalculate in cm⁻³ units consistently
  4. x_n0 ≈ 0.947 μm

Answer: x_n0 ≈ 0.95 μm

Temperature Effects

Temperature Dependence of n_i

n_i \propto T^{3/2} e^{-E_g/2kT}

SymbolDescriptionUnit
TAbsolute temperatureK

Worked example

By what factor does n_i increase in Si when T increases from 300 K to 400 K? (Use n_i(300 K)=1.5×10¹⁰ cm⁻³ and n_i(400 K)=1.0×10¹² cm⁻³ as given values.)

Given: n_i(300)=1.5×10¹⁰, n_i(400)=1.0×10¹²

  1. Ratio = n_i(400)/n_i(300) = 1.0×10¹²/1.5×10¹⁰
  2. = 66.7

Answer: n_i increases by ~67× from 300 K to 400 K in Si

Mobility Temperature Dependence

\mu \propto T^{-3/2}\text{ (lattice scattering dominant above 200 K)}

SymbolDescriptionUnit
\muCarrier mobilitycm²/Vs

Worked example

Estimate μ_n at 400 K given μ_n(300 K) = 1350 cm²/Vs (lattice scattering dominant).

Given: μ_n(300)=1350, T1=300, T2=400

  1. μ_n(400) = 1350 × (300/400)^{3/2}
  2. = 1350 × (0.75)^{1.5}
  3. = 1350 × 0.6495
  4. = 877 cm²/Vs

Answer: μ_n(400 K) ≈ 877 cm²/Vs

Quick reference

FormulaExpression
Intrinsic Carrier Concentrationn_i = \sqrt{N_c N_v}\,e^{-E_g/2kT}
Mass-Action Lawnp = n_i^2
Fermi Level (n-type)E_F - E_i = kT\ln(N_D/n_i)
Drift Current DensityJ = q(\mu_n n + \mu_p p)\mathcal{E}
Diffusion Current (holes)J_p = -qD_p\,dp/dx
Einstein RelationD/\mu = kT/q = V_T
Diffusion LengthL_p = \sqrt{D_p \tau_p}
Excess Carrier Decay\delta p(t) = \delta p(0)\,e^{-t/\tau_p}
Hall Coefficient (n-type)R_H = -1/(qn)
Built-in PotentialV_0 = V_T\ln(N_A N_D/n_i^2)
Max Electric Field\mathcal{E}_{max} = qN_D x_{n0}/\varepsilon_s
Conductivity\sigma = q(\mu_n n + \mu_p p)
Photon EnergyE = hc/\lambda
N_c Temperature ScalingN_c \propto T^{3/2}
Mobility vs Temperature\mu \propto T^{-3/2}

Exam tips

  • GATE frequently asks you to apply the mass-action law to find minority carrier concentration — always confirm whether the sample is n-type or p-type before selecting the minority species.
  • Hall effect sign convention is a common trap: negative R_H confirms n-type, positive confirms p-type — examiners specifically check this when current and field directions are given.
  • In diffusion current problems, note the sign difference: electron diffusion current flows in the direction of the concentration gradient, while hole diffusion current flows opposite — getting this wrong reverses the answer.
  • Carrier lifetime versus diffusion length problems appear together; always calculate D first from the Einstein relation rather than looking it up, since exam problems often give μ but not D.
  • Temperature-dependence questions on n_i often require you to show that n_i doubles every 11 K for Si — knowing this heuristic speeds up order-of-magnitude checks.
  • When computing the built-in potential, examiners check that you use log base e (natural log) and not log base 10 — a factor of 2.303 error is a common mistake.