Numerical analysis of crystal growth of an InAs-GaAs binary semiconductor under microgravity conditions

We investigate the possibility of growing a uniform binary compound crystal in space, proposing a new crystal growth method. We develop a numerical ca lculation method for the growth of binary crystals, in which convection ind uced by temperature and concentration differences in the solution is taken into account. How to determine the shape and movement of the solution-cryst al interface during the crystal growth is clearly explained for binary crys tals, which is more complicated than for single-component crystals. The bou ndary fit method is employed to solve this moving boundary phase transition problem. The calculation method is applied to the crystal growth analysis of an InAs-GaAs binary semiconductor and the effect of buoyancy convection induced under microgravity conditions on the crystal growth process is inve stigated. It is found that the concentration held is disturbed and, as a re sult, the solution-crystal interface is deformed by buoyancy convection, ev en when the gravitational acceleration is as low as 10(-6) g, which is supp osed to be the gravity level in the International Space Station which will start operation in 2004. It is also found that the direction of the residua l gravity has a strong effect on the concentration held in the solution and the crystal growth process. Next, we analyse the influence of g-jitters an d the Soret effect on the crystal growth process. In fact, it is found that g-jitters and the Soret effect have little influence on the macroscopic cr ystal growth process. The dependence of the generation of supercooling in t he solution on convection is also investigated. It is found that supercooli ng is not induced by convection if residual gravity is 10-6 g. Finally, we discuss the possibility of growing high-quality InGaAs crystals of uniform compositions in space.