Using Divergence theorem to find Hamaker Field (here modeled as point-wise"index_1.gif") for a Finite Body

The induced dipole—dipole interaction goes as -1/"index_2.gif", and it is this term which shows up in the Lennard-Jones potential.  This dipole-dipole interaction gives rise to the Hamaker forces between two bodies.  As a first approximation to the interaction between two bodies, one must intergrate 1/"index_3.gif" from a single point in the first body to all points in the second body.  The net interaction energy is the sum over all such points and therefore this energy produces a six-dimensional integration. There are a few cases, such a two spheres, a sphere and a seminfinite half-space, that can be worked out exactly.  However, to model the interaction energy of more complex shapes, there are no closed-form solutions and one must resort to numerical integration.

Numerical integration is a cpu-time-consuming numerical procedure—a six dimensional integration can be very expensive (time is money).  If there is a way to reduce the dimensionality of the integration, then we can reap rewards for our cleverness.  One trick is to use the divergence theorem to push the integration over a volume, to an integration over a surface. For example, we could use the divergence theorem:
∫∫∫"index_4.gif" ∇· "index_5.gif" dV = ∫∫"index_6.gif""index_7.gif"
We will work out such an example for a cylindrical volume interacting with a point in space, in other words, the London Interaction Potential for a finite cylinder. We will perform as many exact integrals as possible and reduce the cost of the numerical integration.  To do this, we must find a vector potential "index_8.gif" such that ∇· "index_9.gif" = -1/|"index_10.gif" where "index_11.gif" is a position in the integrated volume and  "index_12.gif" is a point at which the potential is measured.  (A fairly general method to do this and similar problems can be found in Argento C; Jagota A; Carter WC ``Surface formulation for molecular interactions of macroscopic bodies'' J.Mech. Physics Solids 1997,  pp 1161-1183 .

The following is a ``guess'' at the vector potential; it will be verified as the correct one by checking its divergence.  We use (CX,CY,CZ) to represent points in the cylinder and (X,Y,Z) to be points in space

"index_13.gif"

"index_14.gif"

"index_15.gif"

The following verifies that the correct vector potential is obtained, the divergence must be taked with respect to the coodinates of the integration:

"index_16.gif"

"index_17.gif"

We will integrate over a cylinder of radius R and length L along the z-axis, with its middle at the origin.  First, let's use the radius of the cylinder to scale all the length variables: Let (X,Y,Z)/R = (x,y,z); (CX,CY,CZ)/R = (cx,cy,cz), and L/R = λ (the cylinder's aspect ratio).

"index_18.gif"

"index_19.gif"

Therefore, φ("index_20.gif") =  ∫∫∫"index_21.gif" "index_22.gif" dV = ∫∫"index_23.gif""index_24.gif"  = (∫∫"index_25.gif"  "index_26.gif" + ∫∫"index_27.gif"   "index_28.gif")/"index_29.gif"
is the total interaction between a point an a cylinder.  We can exploit the symmetry of the cylinder: we know that the potential will be indendent of the angular coordinate in cylindrical coordinates; it will be a function of ρ = "index_30.gif"and z.

We will do three integrals over the cylindrical surfaces using this expression to define the cylinder: (cx,cy,cz) = (Cos[θ], Sin[θ], cz):
The cylindrical surface  is the domain  θ ∈ (0, 2π), cz ∈ (-"index_31.gif" , "index_32.gif")
The two caps r ∈ (0,1),  θ ∈ (0, 2π), cz=±"index_33.gif"


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