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Integration over Surfaces

Integration of a function over a surface is a straightforward generalization of $ \int \int f(x,y) dx dy = \int f(x,y) dA$ . The set of all little rectangles $ dx dy$ defines a planar surface. A non-planar surface $ \vec{x}(u,v)$ is composed of a set of little parallelogram patches with sides given by the infinitesimal vectors

\begin{displaymath}\begin{split}\vec{r_u} du = & \ensuremath{\frac{\partial{\vec...
...nsuremath{\frac{\partial{\vec{x}}}{\partial{v}}} dv \end{split}\end{displaymath} (15-2)

Because the two vectors $ \vec{r_u}$ and $ \vec{r_v}$ are not necessarily perpendicular, their cross-product is needed to determine the magnitude of the area in the parallelogram:

$\displaystyle dA = \norm {\vec{r_u} \times \vec{r_v}} du dv$ (15-3)

and the integral of some scalar function, $ g(u,v) = g(x(u,v),y(u,v)) = g(\vec{x}(u,v))$ , on the surface is

$\displaystyle \int g(u,v) dA = \int \int g(u,v) \norm {\vec{r_u} \times \vec{r_v}} du dv$ (15-4)

However, the operation of taking the norm in the definition of the surface patch $ dA$ indicates that some information is getting lost--this is the local normal orientation of the surface. There are two choices for a normal (inward or outward).

When calculating some quantity that does not have vector nature, only the magnitude of the function over the area matters (as in Eq. 15-4). However, when calculating a vector quantity, such as the flow through a surface, or the total force applied to a surface, the surface orientation matters and it makes sense to consider the surface patch as a vector quantity:

\begin{displaymath}\begin{split}\vec{A}(u,v) & = \norm {\vec{A}} \hat{n}(u,v) = ...
...{n}(u,v)\ d\vec{A} & =\vec{r_u} \times \vec{r_v}\ \end{split}\end{displaymath} (15-5)

where $ \hat{n}(u,v)$ is the local surface unit normal at $ \vec{x}(u,v)$ .


MATHEMATICA$ ^{\text{\scriptsize {\textregistered }}}$ Example
(notebook Lecture-15)
(html Lecture-15)
(xml+mathml Lecture-15)
Integrals of Anisotropic Surface Energy The surface energy of single crystals often depends on the surface orientation. This is especially the case for materials that have covalent and/or ionic bonds.

To find the total surface energy of such a single crystal, one has to integrate an orientation-dependent surface energy over the surface of a body.

This example compares the total energy of such an anisotropic surface energy integrated over a sphere and a cube that enclose the same volume.

  1. Enter the parametric equation of the sphere in terms of longitude $ v \in (0, 2 \pi)$ and latitude $ u \in (-\pi/2, \pi/2)$ .
  2. Calculate the tangent plane vectors $ \vec{r_u}$ and $ \vec{r_v}$
  3. Calculate their cross product for subsequent use in the surface integral:

    $\displaystyle \int \int g(\hat{n}(u,v)) \norm {\vec{r_u} \times \vec{r_v}} du dv
$

  4. Use the vectors to calculate the local unit normal.
  5. Integrate a model function:

    $\displaystyle \gamma_{anis}(\hat{n}) = 1 + \gamma_{111} n_1^2 n_2^2 n_3^3
$

    over a sphere
  6. Compare this result to the integration over a cube with the same volume.

The above calculation compares two fixed shapes--to find the surface which has the least energy for enclosing a given volume, one would employ a construction known as the Wulff Theorem.



© W. Craig Carter 2003-, Massachusetts Institute of Technology