Abstract
The coarsening dynamics of a faceted vicinal crystalline surface
growing into its melt by attachment kinetics is considered. The
convective Cahn-Hilliard equation (
) is derived as a
small amplitude expansion of such surface evolutions restricted to 1-D
morphologies. It takes the form
 |
(
) |
where the local surface slope

serves as the order parameter, subscripts denote partial derivative with respect to time

and space

respectively, and

denotes the

-derivative. The
effective free energy

takes the form of a symmetric
double well with minima at

, thereby capturing the anisotropy of the crystal surface energy. Also, the dimensionless small parameter

multiplying the convective term

is a dimensionless measure of the growth strength.
A sharp interface theory for
is derived through
a matched asymptotic analysis. The theory predicts a nearest neighbor
interaction between two non-symetrically related phase boundaries
(kink and anti-kink), whose characteristic separation
grows as coalescing kink/anti-kinks
annihilate one another. Theoretical predictions on the resulting
(skew-symetric) coarsening dynamical system
include
- The characteristic length
, provided
is appropriately small with respect to the Peclet length scale
.
- Binary coalescence of phase boundaries is impossible
- Ternary coalescence may only occur through the kink-ternary interaction; two kinks meet an anti-kink resulting in a kink.
Direct numerical simulations performed on both

and

confirm each of these predictions.
Last, a linear stability analysis of
identifies a pinching mechanism as the dominant instability, which in turn leads to kink-ternaries. We propose a self-similar period-doubling pinch ansatz as a model for the coarsening process, from which an analytical coarsening law for the characteristic length scale
emerges. It predicts both the scaling constant
of the
regime, i.e.,
, as well as the crossover to logarithmically slow coarsening as
crosses
. Our analytical coarsening law stands in good qualitative agreement with large scale numerical simulations that have been performed on
.
In part, joint work with Felix Otto and Stephen H. Davis.
April 15, 2003
Time: 4:30 P.M.
Location: PPB 300
PLEASE NOTE TIME.