Stabilization The stabilization of foam is caused by
van der Waals forces between the molecules in the foam,
electrical double layers created by
dipolar surfactants, and the
Marangoni effect, which acts as a restoring force to the lamellae. The Marangoni effect depends on the liquid that is foaming being impure. Generally, surfactants in the solution decrease the surface tension. The surfactants also clump together on the surface and form a layer as shown below. For the Marangoni effect to occur, the foam must be indented as shown in the first picture. This indentation increases the local surface area. Surfactants have a larger diffusion time than the bulk of the solution—so the surfactants are less concentrated in the indentation. Also, surface stretching makes the surface tension of the indented spot greater than the surrounding area. Consequentially—since the diffusion time for the surfactants is large—the Marangoni effect has time to take place. The difference in surface tension creates a gradient, which instigates fluid flow from areas of lower surface tension to areas of higher surface tension. The second picture shows the film at equilibrium after the Marangoni effect has taken place.
Curing a foam solidifies it, making it indefinitely stable at STP.
Destabilization Witold Rybczynski and
Jacques Hadamard developed an equation to calculate the velocity of bubbles that rise in foam with the assumption that the bubbles are spherical with a radius r. : u=\frac{2gr^2}{9\eta_2}(\rho_2-\rho_1)\left (\frac{3\eta_1+3\eta_2}{3\eta_1+2\eta_2}\right)\! with velocity in units of centimeters per second. ρ1 and ρ2 is the density for a gas and liquid respectively in units of g/cm3 and ῃ1 and ῃ2 is the
dynamic viscosity of the gas and liquid respectively in units of g/cm·s and g is the
acceleration of gravity in units of cm/s2. However, since the density and viscosity of a liquid is much greater than the gas, the density and viscosity of the gas can be neglected, which yields the new equation for velocity of bubbles rising as: : u=\frac{gr^2}{3\eta_2}(\rho_2)\! However, through experiments it has been shown that a more accurate model for bubbles rising is: : u=\frac{2gr^2}{9\eta_2}(\rho_2-\rho_1)\! Deviations are due to the
Marangoni effect and capillary pressure, which affect the assumption that the bubbles are spherical. For laplace pressure of a curved gas liquid interface, the two principal radii of curvature at a point are R1 and R2. With a curved interface, the pressure in one phase is greater than the pressure in another phase. The capillary pressure Pc is given by the equation of: : P_c=\gamma\left (\frac{1}{R_1}+\frac{1}{R_2}\right)\!, where \gamma is the surface tension. The bubble shown below is a gas (phase 1) in a liquid (phase 2) and point A designates the top of the bubble while point B designates the bottom of the bubble. At the top of the bubble at point A, the pressure in the liquid is assumed to be p0 as well as in the gas. At the bottom of the bubble at point B, the hydrostatic pressure is: : P_B,1=p_0+g\rho_1z\! : P_B,2=p_0+g\rho_2z\! where ρ1 and ρ2 is the density for a gas and liquid respectively. The difference in hydrostatic pressure at the top of the bubble is 0, while the difference in hydrostatic pressure at the bottom of the bubble across the interface is
gz(
ρ2 −
ρ1). Assuming that the radii of curvature at point A are equal and denoted by RA and that the radii of curvature at point B are equal and denoted by RB, then the difference in capillary pressure between point A and point B is: : P_c=2\gamma\left (\frac{1}{R_A}-\frac{1}{R_B}\right)\! At equilibrium, the difference in capillary pressure must be balanced by the difference in hydrostatic pressure. Hence, : gz(\rho_2-\rho_1)=2\gamma\left (\frac{1}{R_A}-\frac{1}{R_B}\right)\! Since, the density of the gas is less than the density of the liquid the left hand side of the equation is always positive. Therefore, the inverse of RA must be larger than the RB. Meaning that from the top of the bubble to the bottom of the bubble the radius of curvature increases. Therefore, without neglecting gravity the bubbles cannot be spherical. In addition, as z increases, this causes the difference in RA and RB too, which means the bubble deviates more from its shape the larger it grows. Foam destabilization occurs for several reasons. First,
gravitation causes drainage of liquid to the foam base, which Rybczynski and Hadamar include in their theory; however, foam also destabilizes due to
osmotic pressure causes drainage from the lamellas to the Plateau borders due to internal concentration differences in the foam, and
Laplace pressure causes diffusion of gas from small to large bubbles due to pressure difference. In addition, films can break under
disjoining pressure, These effects can lead to rearrangement of the foam structure at scales larger than the bubbles, which may be individual (
T1 process) or collective (even of the "avalanche" type). ==Mechanical properties==