Determination of scattering mechanisms in AlInGaN/GaN heterostructures grown on sapphire substrate

2021 ◽  
Vol 864 ◽  
pp. 158895
Author(s):  
F. Sonmez ◽  
E. Arslan ◽  
S. Ardali ◽  
E. Tiras ◽  
E. Ozbay
Author(s):  
A. Agrawal ◽  
A. Ali ◽  
R. Misra ◽  
P. E. Schiffer ◽  
B. R. Bennett ◽  
...  

1998 ◽  
Vol 103 (1) ◽  
pp. 225-235 ◽  
Author(s):  
Timothy K. Stanton ◽  
Dezhang Chu ◽  
Peter H. Wiebe ◽  
Linda V. Martin ◽  
Robert L. Eastwood

1988 ◽  
Vol 67 (6) ◽  
pp. 651-655 ◽  
Author(s):  
C.D. Kourkoutas ◽  
G.J. Papaioannou ◽  
P.C. Euthymiou ◽  
G.E. Zardas
Keyword(s):  

2015 ◽  
Vol 9 (3) ◽  
pp. 157-168 ◽  
Author(s):  
Johann Schön

Nanomaterials bridge the gaps between crystalline materials, thin films, and molecules, and are of great importance in the design of new classes of materials, since the existence of many modifications of a nano-object for the same overall composition allows us to tune the properties of the nanomaterial. However, the structural analysis of nano-size systems is often difficult and their structural stability is frequently relatively low. Thus, a study of their energy landscape is needed to determine or predict possible structures, and analyse their stability, via the determination of the minima on the landscape and the generalized barriers separating them. In this contribution, we introduce the major concepts of energy landscapes for chemical systems, and present summaries of four applications to nano-materials: a MgO monolayer on a sapphire substrate, possible quasitwo- dimensional carbon-silicon networks, the ab initio energy landscape of Cu4Ag4-clusters, and the possible arrangements of ethane molecules on an ideally smooth substrate.


1966 ◽  
Vol 25 ◽  
pp. 93-97
Author(s):  
Richard Woolley

It is now possible to determine proper motions of high-velocity objects in such a way as to obtain with some accuracy the velocity vector relevant to the Sun. If a potential field of the Galaxy is assumed, one can compute an actual orbit. A determination of the velocity of the globular clusterωCentauri has recently been completed at Greenwich, and it is found that the orbit is strongly retrograde in the Galaxy. Similar calculations may be made, though with less certainty, in the case of RR Lyrae variable stars.


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