Colloidal Stability: DLVO Theory
2026-03-16
After this lecture, you will be able to:
Last lecture, we introduced a kinetic barrier through the external potential \(V_T\):
\[\begin{align} F = 4\pi r^2 D_{11} \left( \frac{dN}{dr} + \frac{N}{k_B T}\frac{dV_T}{dr} \right) \end{align}\]and the Fuchs stability ratio
\[\begin{align} W = \frac{\beta_{11}^{\mathrm{DLCA}}}{\beta_{11}^{\mathrm{RLCA}}} \end{align}\]When we introduce the external potential \(V_T\) (and \(W\)) we show the RLCA rate is slower, but why?
Derjaguin, Landau, Verwey, and Overbeek (DLVO) theory: For charged colloids, the total interaction potential comes from two competing effects:
DLVO theory combines them into one total potential.
\[\begin{align} V_T(h) = V_{\mathrm{vdW}}(h) + V_{\mathrm{el}}(h) \end{align}\]
where \(h\) is the surface-to-surface separation.
From Lecture 18, a lyophobic colloid remains only metastable. The dispersed state has higher free energy than the aggregated state, but aggregation may be delayed if particles must overcome a barrier.
Key idea:

A typical interaction curve contains (how do they come)?
A charged solid surface in electrolyte attracts counterions and repels coions. This creates the electrical double layer:
The potential field \(\psi\) in a dielectric medium satisfies Poisson equation (one of Maxwell’s equations)
For ion species \(i\) with valence \(z_i\), the equilibrium concentration follows
\[\begin{align} n_i = n_{i,\infty} \exp \left( -\frac{z_i e \psi}{k_B T} \right) \end{align}\]Hence the charge density \(\rho\) in Poisson equation is
\[\begin{align} \rho = \sum_i z_i e n_i = \sum_i z_i e n_{i,\infty} \exp \left( -\frac{z_i e \psi}{k_B T} \right) \end{align}\]Linking this to the Poisson equation gives the Poisson-Boltzmann (PB) equation
Combining Poisson and Boltzmann gives the nonlinear PB equation
\[\begin{align} \nabla^2 \psi = -\frac{1}{\varepsilon_r \varepsilon_0} \sum_i z_i e n_{i,\infty} \exp \left( -\frac{z_i e \psi}{k_B T} \right) \end{align}\]For a symmetric electrolyte and planar geometry, this becomes the standard 1D form.
Take \(x\) normal to a flat charged surface. Far from the surface, the solution must recover bulk electroneutrality:
\[\begin{align} \psi(x \rightarrow \infty) &= 0 \\ \frac{d\psi}{dx}(x \rightarrow \infty) &= 0 \end{align}\]At the surface, two common boundary conditions are used.
If the surface potential can be predetermined (like zeta-potential measurements), then
\[\begin{align} \psi(0) = \psi_0 \end{align}\]This is often used when adsorption or surface chemistry keeps the interfacial potential nearly fixed.
Using Gauss law, the electric field at the surface satisfies
\[\begin{align} \sigma = -\varepsilon_r \varepsilon_0 \frac{d\psi}{dx}\Big|_{x=0} \end{align}\]This is the constant-charge description, applicable to:
If the potential is not too large,
\[\begin{align} \left| \frac{z_i e \psi}{k_B T} \right| \ll 1 \end{align}\]then the PB equation can be linearized, often called the Debye-Hückel (DH) approximation
\[\begin{align} \exp \left( -\frac{z_i e \psi}{k_B T} \right) \approx 1 - \frac{z_i e \psi}{k_B T} \end{align}\]The linearized equation in DH approximation becomes
\[\begin{align} \frac{d^2 \psi}{dx^2} = \kappa^2 \psi \end{align}\]We know from the diffusion concepts it is like a steady-state Fick’s second law, but with external potential. The solution is a nice exponential decay of potential \(\psi\)
\[\begin{align} \psi(x) = \psi_0 e^{-\kappa x} \end{align}\]One consequence of the DH approximation is that the electrostatic screening is related with the charge concentrations in the liquid:
\[\begin{align} \kappa^{-1} &= \left( \frac{\varepsilon_r \varepsilon_0 k_B T} {e^2 \sum n_{i, 0} z_i^2} \right)^{1/2} \\ &= \left( \frac{\varepsilon_r \varepsilon_0 k_B T} {2 e^2 N_a I} \right)^{1/2} \end{align}\]where \(N_a\) is the Avogadro number, and \(I = 1/2 \sum_{i} z_{i}^{2} c_{i, 0}\) is the ionic strength.
From the Debye-Hückel Approximation, we typically can use the following handy rule:
\[ \kappa = 3.29 \sqrt{I} = 3.29 \sqrt{\frac{1}{2}\sum c_{i, 0} z_i^2}\qquad \text{[nm]}^{-1} \]
when the solute concentration \(c_{i, 0}\) is in mol/L. For example, for a \(10^{−3}\) M, 1:1 electrolyte, \(1/\kappa = 9.6\) nm.
Where can I find the screening length \(\kappa^{-1}\)?
The Debye–Hückel approximation assumes small potential
\[\begin{align} \left|\frac{ze\psi}{k_B T}\right| \ll 1 \end{align}\]For a higher surface potential, the Gouy-Chapman (GC) equation is more accurate (exact solution for symmetric electrolyte.
\[\begin{align} \frac{d^{2} \psi}{dx^{2}} &= -\frac{zc_{0}e}{\varepsilon_{o} \varepsilon_{r}} \left[ \exp(-\frac{ze\psi}{k_{\mathrm{B}}T}) - \exp(\frac{ze\psi}{k_{\mathrm{B}}T})\right]\\ &= \frac{2zc_{0}e}{\varepsilon_{o} \varepsilon_{r}} \sinh\left(\frac{ze\psi}{k_{\mathrm{B}}T}\right) \end{align}\]Solution to the GC equation is:
\[ \frac{\tanh(ze\psi/4k_{\mathrm{B}}T)}{\tanh(ze\psi_{0}/4k_{\mathrm{B}}T)} = \exp(-\kappa x) \]
When two charged surfaces approach, their diffuse layers overlap. You can imagine the charge-redistribution occurs between the two surfaces. Let’s first assume the charged surfaces are flat surfaces, the overlay will cause osmotic pressure.
In an ideal electrolyte solution, the local osmotic pressure follows the Donnan equation
\[ P_{\mathrm{osmotic}}(x) = k_B T \left(c_{+}(x) + c_{-}(x)\right) \]
Consider a differential volume element \(dV\) located at position \(x\).
The differential osmotic force acting on the element is
\[\begin{align} dF_{\mathrm{osmotic}} = \frac{dP_{\mathrm{osmotic}}}{dx} dV \end{align}\]The equilibrium requires the electrostatic force and osmotic force must balance at every position.
\[\begin{align} \frac{dP_{\mathrm{osmotic}}}{dx} &= \varepsilon_0\varepsilon_r \frac{d^2\psi}{dx^2} \frac{d\psi}{dx} \\ &= \frac{\varepsilon_0\varepsilon_r}{2} \frac{d}{dx} \left[ \left(\frac{d\psi}{dx}\right)^2 \right] \end{align}\]Since we know the solution to the Poisson-Boltzmann equation, integrating this will give us the total interaction energy.
The repulsive potential energy \(W_{\mathrm{R}}\) per unit area between two charged particles at distance \(h\) is then calculated as:
\[\begin{align} W_{\mathrm{R}}(h) &= -\int_{\infty}^{h} \frac{F_{\mathrm{R}}}{A} \mathrm{d} h' \\ &= 64 k T c_{0} \kappa^{-1} \Lambda_{0}^{2} e^{-\kappa h} \end{align}\]where \(\Lambda_{0} = \tanh(\frac{z e \psi_{0}}{4k_{\mathrm{B}}T})\). Note we need to adjust for the particle curvature if they are spheres.
The plate result is not yet the particle result. Real colloids are spherical, so we must convert planar interaction into curved-particle interaction. Derjaguin approximation calculates the electrostatic repulsion between sphere particles by:
\[\begin{align} V(h) = 2\pi R_{\mathrm{eff}} W(h) \end{align}\]where \(W(h)\) is the interaction free energy per unit area between plates. This is our final solution
For two particles of radii \(a_1\) and \(a_2\),
\[\begin{align} R_{\mathrm{eff}} = \frac{a_1 a_2}{a_1+a_2} \end{align}\]For equal particles, \(a_1=a_2=a\):
\[\begin{align} R_{\mathrm{eff}} = \frac{a}{2} \end{align}\]The repulsion between two spherical particles separated by \(h\) under the Derjarguin approximation is
\[ V_{\mathrm{R}}^{\mathrm{ss}}(h) = 64 \pi k_B T c_{0} R \kappa^{-2} \Lambda_{0}^{2} e^{-\kappa h} \]
Such approximation is valid when:
The attractive branch comes from fluctuating dipoles. At the molecular level, we have interaction between two particles following the \(r^{-6}\) rule
\[\begin{align} u(r) = -\frac{C}{r^6} \end{align}\]Summing over all pair interactions between two bodies gives the macroscopic van der Waals interaction. The material dependence is collected into the Hamaker constant \(A_H\).
For two spheres at small separation \(h \ll a_1, a_2\),
\[\begin{align} V_{\mathrm{vdW}}(h) = -\frac{A_H R_{\mathrm{eff}}}{6h} \end{align}\]For equal particles with radius \(a\),
\[\begin{align} V_{\mathrm{vdW}}(h) = -\frac{A_H a}{12h} \end{align}\]Putting both parts from repulsive electrostatics and attractive vdW together gives the central DLVO expression:
\[\begin{align} V_T(h) = -\frac{A_H R_{\mathrm{eff}}}{6h} + B R_{\mathrm{eff}} e^{-\kappa h} \end{align}\]This single curve explains both stabilization and aggregation.
The key quantity is the maximum barrier height \(V_{T,\max}\) in the DLVO curve.
particle collisions usually do not lead to sticking.
then particles can cross the barrier and aggregate.
This is the physical origin of RLCA.
Increasing salt compresses the double layer:
\[\begin{align} \kappa \propto I^{1/2} \end{align}\]Consequences:
At a sufficiently high salt level, the barrier vanishes. This defines the critical coagulation concentration.
In Lecture 18 we wrote
\[\begin{align} \beta_{11}^{\mathrm{RLCA}} = \frac{\beta_{11}^{\mathrm{DLCA}}}{W} \end{align}\]and
\[\begin{align} W \approx \frac{1}{2\kappa a} \exp \left( \frac{V_{T,\max}}{k_B T} \right) \end{align}\]Now we can interpret this clearly:
It is the simplest quantitative framework for charged colloidal stability.
DLVO is powerful, but not complete. Missing effects include:
These extensions are often needed in real polymer and ceramic systems.