Semiconductor Crystal Growth and Segregation Problems on Earth And in Space

1981 ◽  
Vol 9 ◽  
Author(s):  
Harry C. Gatos

ABSTRACTCrystals grown from the melt exhibit compositional and structural defects which limit the exploitation of their full potential in solid state electronics. The origin of these defects is related primarily to gravity-induced convective currents in the melt. In semiconductor compounds additional problems are introduced from variations in stoichiometry. Progress has been made recently in relating qualitatively, and in some instances quantitatively, the growth parameters to the materials properties of the crystals, and in turn to their electronic properties. Overcoming the presence of gravitational forces in space eliminates or minimizes convective interference and, thus, the quantitative assessment of the key growth parameters controlling the chemical and structural perfection of single crystals becomes possible. Results (obtained on earth) will be presented on the growth-property relationships of elemental and compound semiconductors. The advantages, as well as the limitations, that zero gravity conditions present for crystal growth will be discussed.

1998 ◽  
Author(s):  
Ch. Stenzel ◽  
H. Lenski ◽  
P. Dold ◽  
Th. Kaiser ◽  
K.-W. Benz ◽  
...  

1994 ◽  
Vol 348 ◽  
Author(s):  
N.V. Kilassen

ABSTRACTThe studies of the dependence of the optical properties of various scintillators on intrinsic structural defects have been reviewed. The greater part of the review is devoted to the defects introduced by plastic deformation. A wide range of variations in the light output, spectral distribution, kinetics and other properties has been observed. These defects can be induced during crystal growth, annealing, processing, etc. The proper regulation of the superstructure of intrinsic defects can ensure the production of high quality scintillators having required properties.


1997 ◽  
Vol 492 ◽  
Author(s):  
Sukit Llmpijumnong ◽  
Walter R. L. Lambrecht

ABSTRACTThe energy differences between various SiC polytypes are calculated using the full-potential linear muffin-tin orbital method and analyzed in terms of the anisotropie next nearest neighbor interaction (ANNNI) model. The fact that J1 + 2J2 < 0 with J1 > 0 implies that twin boundaries in otherwise cubic material are favorable unless twins occur as nearest neighbor layers. Contrary to some other recent calculations we find J1 > |J2|. We discuss the consequences of this for stabilization of cubic SiC in epitaxial growth, including considerations of the island size effects.


2019 ◽  
Vol 55 (2) ◽  
pp. 1900115
Author(s):  
Christiane Frank-Rotsch ◽  
Natasha Dropka ◽  
Frank-Michael Kießling ◽  
Peter Rudolph

2010 ◽  
Vol 62 (12) ◽  
pp. 955-960 ◽  
Author(s):  
Thierry Duffar ◽  
Amal Nadri

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