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Motion of Surfaces

Interfacial motion arises in two different ways: 1) as the motion of two-dimensional level sets during gradient flow of an integral over volume; 2) as a velocity normal to a surface, where the velocity is gradient flow of a surface integral. The first method is discussed in Section 3.2.1.

The second approach has been discussed above and appears in tables I and in table II in small slope approximation and as the graph of a function z(x,y), respectively, for isotropic surfaces. For anisotropic surfaces, the energy functional is a surface integral: tex2html_wrap_inline1340 . The interfacial surface energy density, tex2html_wrap_inline1342 , does not necessarily have continuous derivatives of the surface orientation tex2html_wrap_inline1344 ; in fact, tex2html_wrap_inline1342 need not be continuous. Furthermore, the surface S can have edges and corners where its derivatives are discontinuous; furthermore it can have flat facets. In this case, the variational derivative is the instantaneous increase in interfacial area due to a normal velocity v, weighted by the surface energy density, and is called the `weighted mean curvature' tex2html_wrap_inline1352 [6]. When tex2html_wrap_inline1354 is isotropic, tex2html_wrap_inline1352 is equal to tex2html_wrap_inline1358 , where tex2html_wrap_inline1360 is the geometric mean curvature. In two dimensions, tex2html_wrap_inline1605 , when tex2html_wrap_inline1354 is twice differentiable with respect to the polar angle tex2html_wrap_inline1366 , which is the the Herring formulation[7]. Generally, tex2html_wrap_inline1368 , where tex2html_wrap_inline1370 is the Cahn-Hoffman capillarity vector[6, 8, 9, 4].

The anisotropic version of gradient flow for the surface integrals is summarized in the following table:

tabular363





W. Craig Carter
Tue Sep 30 16:07:27 EDT 1997