Results from a numerical modeling study of ZnSe crystal growth by physical
vapor transport (PVT) are reported in this paper. The influence of a residu
al gas is included in the two-dimensional model. The simulations show that
the Stefan flux dominates the system and the subtle gravitational effects c
an be gauged by subtracting this flux from the calculated flow fields. Shea
r flows, due to solutal buoyancy, of the order of 50 mu m/s for the horizon
tal growth orientation and 10 mu m/s for the vertical orientation are predi
cted adjacent to the growing crystal. Whether these flows can fully account
for the observed gravity-related growth morphological effects and inhomoge
neous solute and dopant distributions is a matter of conjecture. A template
for future modeling efforts in this area is suggested which incorporates a
mathematical approach to the tracking of the growth front based on energy
of formation concepts. (C) 2000 Elsevier Science B.V. All rights reserved.