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Molecular beam epitaxial growth of III-V semiconductor ... - KOBRA

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Hetero<strong>epitaxial</strong> Growth <strong>of</strong> <strong>III</strong>-V Semiconductor on Silicon Substrates<br />

with respect to their substrates. In highly mismatched material systems, gross<br />

misorientations are sometimes observed, due to the close matching in the atomic<br />

spacings for the substrate and the <strong>epitaxial</strong> layers in dierent crystallographic<br />

directions [31]. However, as noted before, the strain energy will grow as the overlayer<br />

thickness increase. As result, it will eventually be favorable for the overlayer<br />

to generate dislocations. In simplistic theories this occur at an overlayer thickness<br />

called critical thickness (d c ), which is approximately given by Eq. 3.11 [21].<br />

d c<br />

∼ a s<br />

= (3.11)<br />

2|ɛ|<br />

The most widely used theoretical model for the critical layer thickness is the<br />

force balance model <strong>of</strong> Matthews and Blakeslee [43].<br />

• Matthews and Blakeslee Force Balance Model :<br />

The Matthews and Blakeslee model is used most <strong>of</strong>ten to calculate the critical<br />

layer thickness for heteroepitaxy. Here it is considered that a pre-existing<br />

threading dislocation in the substrate replicates in the growing epi-layer and can<br />

bend over to create a chain <strong>of</strong> mist dislocations at the interface, once the critical<br />

layer thickness is reached. This process is shown schematically in Fig. 3.6. The<br />

glide force F G acting on the dislocation is dened by Eq. 3.12.<br />

2Gbfh(1 + ν) cos λ<br />

F G = (3.12)<br />

(1 − ν)<br />

Where λ is the angle between the Burgers vector b and the line in the interface<br />

plane that is perpendicular to the intersection <strong>of</strong> the glide plane with the interface,<br />

G is the shear modulus, ν is the Poisson ratio, b is the length <strong>of</strong> the Burgers vector<br />

for the threading dislocation and h is the lm thickness. On the other hand, the<br />

line tension <strong>of</strong> the mist segment <strong>of</strong> the dislocation F L expressed in Eq. 3.13 is<br />

acting with force in the opposite direction <strong>of</strong> the glide force F G [31].<br />

F L = Gb(1 − ν cos2 α)<br />

[ln(h/b) + 1] (3.13)<br />

4π(1 − ν)<br />

By equating the glide force F G in (see Eq. 3.12) to the line tension for the mist<br />

segment <strong>of</strong> the dislocation F L (see Eq. 3.13) and solve for the thickness. As<br />

36

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