Home Knowledge Base Mathematical Modeling of Epitaxy in Semiconductor Front-End Processing (FEP)

Mathematical Modeling of Epitaxy in Semiconductor Front-End Processing (FEP)

Keywords: epi, epitaxy, epitaxial, epitaxial layer, epi layer, epi process


Mathematical Modeling of Epitaxy in Semiconductor Front-End Processing (FEP)

1. Overview

Epitaxy is a critical Front-End Process (FEP) step where crystalline films are grown on crystalline substrates with precise control of:

Mathematical modeling enables:

1.1 Types of Epitaxy

1.2 Epitaxy Methods

2. Fundamental Thermodynamic Framework

2.1 Driving Force for Growth

The supersaturation provides the thermodynamic driving force:

$$ \Delta \mu = k_B T \ln\left(\frac{P}{P_{eq}}\right) $$

Where:

2.2 Free Energy of Mixing (Multi-component Systems)

For systems like SiGe alloys:

$$ \Delta G_{mix} = RT\left(x \ln x + (1-x) \ln(1-x)\right) + \Omega x(1-x) $$

Where:

2.3 Gibbs Free Energy of Formation

$$ \Delta G = \Delta H - T\Delta S $$

For spontaneous growth: $\Delta G < 0$

3. Growth Rate Kinetics

3.1 The Two-Regime Model

Epitaxial growth rate is governed by two competing mechanisms:

Overall growth rate equation:

$$ G = \frac{k_s \cdot h_g \cdot C_g}{k_s + h_g} $$

Where:

3.2 Temperature Dependence

The surface reaction rate follows Arrhenius behavior:

$$ k_s = A \exp\left(-\frac{E_a}{k_B T}\right) $$

Where:

3.3 Growth Rate Regimes

Temperature RegimeLimiting FactorGrowth Rate ExpressionTemperature Dependence
Low TSurface reaction$G \approx k_s \cdot C_g$Strong (exponential)
High TMass transport$G \approx h_g \cdot C_g$Weak (~$T^{1.5-2}$)

3.4 Boundary Layer Analysis

For horizontal CVD reactors, the boundary layer thickness evolves as:

$$ \delta(x) = \sqrt{\frac{ u \cdot x}{v_{\infty}}} $$

Where:

u$ = kinematic viscosity (m²/s)

The mass transfer coefficient:

$$ h_g = \frac{D_{gas}}{\delta} $$

Where $D_{gas}$ is the gas-phase diffusion coefficient.

4. Surface Kinetics: BCF Theory

The Burton-Cabrera-Frank (BCF) model describes atomic-scale growth mechanisms.

4.1 Surface Diffusion Equation

$$ D_s abla^2 n_s - \frac{n_s - n_{eq}}{\tau_s} + J_{ads} = 0 $$

Where:

4.2 Characteristic Diffusion Length

$$ \lambda_s = \sqrt{D_s \tau_s} $$

This parameter determines the growth mode:

4.3 Surface Diffusion Coefficient

$$ D_s = D_0 \exp\left(-\frac{E_m}{k_B T}\right) $$

Where:

4.4 Step Velocity

$$ v_{step} = \frac{2 D_s (n_s - n_{eq})}{\lambda_s} \tanh\left(\frac{L}{2\lambda_s}\right) $$

Where $L$ is the inter-step spacing (terrace width).

4.5 Growth Rate from Step Flow

$$ G = \frac{v_{step} \cdot h_{step}}{L} $$

Where $h_{step}$ is the step height (monolayer thickness).

5. Heteroepitaxy and Strain Modeling

5.1 Lattice Mismatch

$$ f = \frac{a_{film} - a_{substrate}}{a_{substrate}} $$

Where:

Example values:

SystemLattice Mismatch
Si₀.₇Ge₀.₃ on Si~1.2%
Ge on Si~4.2%
GaAs on Si~4.0%
InAs on GaAs~7.2%
GaN on Sapphire~16%

5.2 Strain Components

For biaxial strain in (001) films:

$$ \varepsilon_{xx} = \varepsilon_{yy} = \varepsilon_{\parallel} = \frac{a_s - a_f}{a_f} \approx -f $$

$$ \varepsilon_{zz} = \varepsilon_{\perp} = -\frac{2C_{12}}{C_{11}} \varepsilon_{\parallel} $$

Where $C_{11}$ and $C_{12}$ are elastic constants.

5.3 Elastic Energy

For a coherently strained film:

$$ E_{elastic} = \frac{2G(1+ u)}{1- u} f^2 h = M f^2 h $$

Where:

u$ = Poisson's ratio

u)}{1- u}$

5.4 Critical Thickness (Matthews-Blakeslee)

$$ h_c = \frac{b}{8\pi f(1+ u)} \left[\ln\left(\frac{h_c}{b}\right) + 1\right] $$

Where:

u$ = Poisson's ratio

5.5 People-Bean Approximation (for SiGe)

Empirical formula:

$$ h_c \approx \frac{0.55}{f^2} \text{ (nm, with } f \text{ as a decimal)} $$

Or equivalently:

$$ h_c \approx \frac{5500}{x^2} \text{ (nm, for Si}_{1-x}\text{Ge}_x\text{)} $$

5.6 Threading Dislocation Density

Above critical thickness, dislocation density evolves:

$$ \rho_{TD}(h) = \rho_0 \exp\left(-\frac{h}{h_0}\right) + \rho_{\infty} $$

Where:

6. Reactor-Scale Modeling

6.1 Coupled Transport Equations

6.1.1 Momentum Conservation (Navier-Stokes)

$$ \rho\left(\frac{\partial \mathbf{v}}{\partial t} + \mathbf{v} \cdot abla \mathbf{v}\right) = - abla p + \mu abla^2 \mathbf{v} + \rho \mathbf{g} $$

Where:

6.1.2 Continuity Equation

$$ \frac{\partial \rho}{\partial t} + abla \cdot (\rho \mathbf{v}) = 0 $$

6.1.3 Species Transport

$$ \frac{\partial C_i}{\partial t} + \mathbf{v} \cdot abla C_i = D_i abla^2 C_i + R_i $$

Where:

6.1.4 Energy Conservation

$$ \rho c_p \left(\frac{\partial T}{\partial t} + \mathbf{v} \cdot abla T\right) = k abla^2 T + \sum_j \Delta H_j r_j $$

Where:

6.2 Silicon CVD Chemistry

6.2.1 From Silane (SiH₄)

Gas phase decomposition:

$$ \text{SiH}_4 \xrightarrow{k_1} \text{SiH}_2 + \text{H}_2 $$

Surface reaction:

$$ \text{SiH}_2(g) + * \xrightarrow{k_2} \text{Si}(s) + \text{H}_2(g) $$

Where $*$ denotes a surface site.

6.2.2 From Dichlorosilane (DCS)

$$ \text{SiH}_2\text{Cl}_2 \rightarrow \text{SiCl}_2 + \text{H}_2 $$

$$ \text{SiCl}_2 + \text{H}_2 \rightarrow \text{Si}(s) + 2\text{HCl} $$

6.2.3 Rate Law

$$ r_{dep} = k_2 P_{SiH_2} (1 - \theta) $$

Where:

6.3 Dimensionless Numbers

NumberDefinitionPhysical Meaning
Reynolds$Re = \frac{\rho v L}{\mu}$Inertia vs. viscous forces
Prandtl$Pr = \frac{\mu c_p}{k}$Momentum vs. thermal diffusivity
Schmidt$Sc = \frac{\mu}{\rho D}$Momentum vs. mass diffusivity
Damköhler$Da = \frac{k_s L}{D}$Reaction rate vs. diffusion rate
Grashof

u^2}$ | Buoyancy vs. viscous forces |

7. Selective Epitaxial Growth (SEG) Modeling

7.1 Overview

In SEG, growth occurs on exposed Si but not on dielectric (SiO₂/Si₃N₄).

7.2 Loading Effect Model

$$ G_{local} = G_0 \left(1 + \alpha \cdot \frac{A_{mask}}{A_{Si}}\right) $$

Where:

7.3 Pattern-Dependent Growth

Sources of non-uniformity:

7.4 Selectivity Condition

For selective growth on Si vs. oxide:

$$ r_{deposition,Si} > 0 \quad \text{and} \quad r_{deposition,oxide} < r_{etching,oxide} $$

Achieved by adding HCl:

$$ \text{Si}(nuclei) + 2\text{HCl} \rightarrow \text{SiCl}_2 + \text{H}_2 $$

Nuclei on oxide are etched before they can grow, maintaining selectivity.

7.5 Faceting Model

Growth rate depends on crystallographic orientation:

$$ G_{(hkl)} = G_0 \cdot f(hkl) \cdot \exp\left(-\frac{E_{a,(hkl)}}{k_B T}\right) $$

Typical growth rate hierarchy:

$$ G_{(100)} > G_{(110)} > G_{(111)} $$

8. Dopant Incorporation

8.1 Segregation Coefficient

Equilibrium segregation coefficient:

$$ k_0 = \frac{C_{solid}}{C_{liquid/gas}} $$

Effective segregation coefficient:

$$ k_{eff} = \frac{k_0}{k_0 + (1-k_0)\exp\left(-\frac{G\delta}{D_l}\right)} $$

Where:

8.2 Dopant Concentration in Film

$$ C_{film} = k_{eff} \cdot C_{gas} $$

8.3 Dopant Profile Abruptness

The transition width is limited by:

$$ \Delta z_{transition} \approx \sqrt{\lambda_{seg}^2 + L_D^2} $$

8.4 Common Dopants for Si Epitaxy

DopantTypePrecursorSegregation Behavior
Bp-typeB₂H₆, BCl₃Low segregation
Pn-typePH₃, PCl₃Moderate segregation
Asn-typeAsH₃Strong segregation
Sbn-typeSbH₃Very strong segregation

9. Atomistic Simulation Methods

9.1 Kinetic Monte Carlo (KMC)

9.1.1 Event Rates

Each atomic event has a rate following Arrhenius:

$$ \Gamma_i = u_0 \exp\left(-\frac{E_i}{k_B T}\right) $$

Where:

u_0$ = attempt frequency (~10¹²-10¹³ s⁻¹)

9.1.2 Events Modeled

u_0 \exp(-E_{des}/k_B T)$

u_0 \exp(-E_m/k_B T)$

9.1.3 Time Advancement

$$ \Delta t = -\frac{\ln(r)}{\Gamma_{total}} = -\frac{\ln(r)}{\sum_i \Gamma_i} $$

Where $r$ is a uniform random number in $(0,1]$.

9.2 Density Functional Theory (DFT)

Provides input parameters for KMC:

Kohn-Sham equation:

$$ \left[-\frac{\hbar^2}{2m} abla^2 + V_{eff}(\mathbf{r})\right]\psi_i(\mathbf{r}) = \varepsilon_i \psi_i(\mathbf{r}) $$

9.3 Molecular Dynamics (MD)

Newton's equations:

$$ m_i \frac{d^2 \mathbf{r}_i}{dt^2} = - abla_i U(\mathbf{r}_1, \mathbf{r}_2, ..., \mathbf{r}_N) $$

Where $U$ is the interatomic potential (e.g., Stillinger-Weber, Tersoff for Si).

10. Nucleation Theory

10.1 Classical Nucleation Theory (CNT)

10.1.1 Gibbs Free Energy Change

$$ \Delta G(r) = -\frac{4}{3}\pi r^3 \cdot \frac{\Delta \mu}{\Omega} + 4\pi r^2 \gamma $$

Where:

10.1.2 Critical Nucleus Radius

Setting $\frac{d(\Delta G)}{dr} = 0$:

$$ r^* = \frac{2\gamma \Omega}{\Delta \mu} $$

10.1.3 Free Energy Barrier

$$ \Delta G^* = \frac{16 \pi \gamma^3 \Omega^2}{3 (\Delta \mu)^2} $$

10.1.4 Nucleation Rate

$$ J = Z \beta^ N_s \exp\left(-\frac{\Delta G^}{k_B T}\right) $$

Where:

10.2 Growth Modes

ModeSurface Energy ConditionGrowth BehaviorExample
Frank-van der Merwe$\gamma_s \geq \gamma_f + \gamma_{int}$Layer-by-layer (2D)Si on Si
Volmer-Weber$\gamma_s < \gamma_f + \gamma_{int}$Island (3D)Metals on oxides
Stranski-KrastanovIntermediate2D then 3D islandsInAs/GaAs QDs

10.3 2D Nucleation

Critical island size (atoms):

$$ i^* = \frac{\pi \gamma_{step}^2 \Omega}{(\Delta \mu)^2 k_B T} $$

11. TCAD Process Simulation

11.1 Overview

Tools: Synopsys Sentaurus Process, Silvaco Victory Process

11.2 Diffusion-Reaction System

$$ \frac{\partial C_i}{\partial t} = abla \cdot (D_i abla C_i - \mu_i C_i abla \phi) + G_i - R_i $$

Where:

11.3 Point Defect Dynamics

Vacancy concentration:

$$ \frac{\partial C_V}{\partial t} = D_V abla^2 C_V + G_V - k_{IV} C_I C_V $$

Interstitial concentration:

$$ \frac{\partial C_I}{\partial t} = D_I abla^2 C_I + G_I - k_{IV} C_I C_V $$

Where $k_{IV}$ is the recombination rate constant.

11.4 Stress Evolution

Equilibrium equation:

$$

abla \cdot \boldsymbol{\sigma} = 0 $$

Constitutive relation:

$$ \boldsymbol{\sigma} = \mathbf{C} : (\boldsymbol{\varepsilon} - \boldsymbol{\varepsilon}^{thermal} - \boldsymbol{\varepsilon}^{intrinsic}) $$

Where:

11.5 Level Set Method for Interface Tracking

$$ \frac{\partial \phi}{\partial t} + v_n | abla \phi| = 0 $$

Where:

12. Advanced Topics

12.1 Atomic Layer Epitaxy (ALE) / Atomic Layer Deposition (ALD)

Self-limiting surface reactions modeled as Langmuir kinetics:

$$ \theta = \frac{K \cdot P \cdot t}{1 + K \cdot P \cdot t} \rightarrow 1 \quad \text{as } t \rightarrow \infty $$

Growth per cycle (GPC):

$$ GPC = \theta_{sat} \cdot d_{monolayer} $$

Typical GPC values: 0.5-1.5 Å/cycle

12.2 III-V on Silicon Integration

Challenges and models:

u}$

12.3 Quantum Dot Formation (Stranski-Krastanov)

Critical thickness for islanding:

$$ h_{SK} \approx \frac{\gamma}{M f^2} $$

Island density:

$$ n_{island} \propto \exp\left(-\frac{E_{island}}{k_B T}\right) \cdot F^{1/3} $$

Where $F$ is the deposition flux.

12.4 Machine Learning in Epitaxy Modeling

Physics-Informed Neural Networks (PINNs):

$$ \mathcal{L}_{total} = \mathcal{L}_{data} + \lambda_{PDE}\mathcal{L}_{physics} + \lambda_{BC}\mathcal{L}_{boundary} $$

Where:

Applications:

13. Key Equations

PhenomenonKey EquationPrimary Parameters
Growth rate (dual regime)$G = \frac{k_s h_g C_g}{k_s + h_g}$Temperature, pressure, flow
Surface diffusion length$\lambda_s = \sqrt{D_s \tau_s}$Temperature
Lattice mismatch$f = \frac{a_f - a_s}{a_s}$Material system
Critical thickness

u)}\left[\ln\frac{h_c}{b}+1\right]$ | Mismatch, Burgers vector |

Elastic strain energy$E = M f^2 h$Mismatch, thickness, modulus
Nucleation rate$J \propto \exp(-\Delta G^*/k_BT)$Supersaturation, surface energy
Species transport

abla C = D abla^2 C + R$ | Diffusivity, velocity, reactions |

KMC event rate

u_0 \exp(-E_a/k_BT)$ | Activation energy, temperature |

Physical Constants

ConstantSymbolValue
Boltzmann constant$k_B$$1.38 \times 10^{-23}$ J/K
Gas constant$R$8.314 J/mol$\cdot$K
Planck constant$h$$6.63 \times 10^{-34}$ J$\cdot$s
Electron charge$e$$1.60 \times 10^{-19}$ C
Si lattice constant$a_{Si}$5.431 Å
Ge lattice constant$a_{Ge}$5.658 Å
GaAs lattice constant$a_{GaAs}$5.653 Å

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