Analysis of the extended defects in 3C-SiC.pdf - Nelson Mandela ...
Analysis of the extended defects in 3C-SiC.pdf - Nelson Mandela ...
Analysis of the extended defects in 3C-SiC.pdf - Nelson Mandela ...
Create successful ePaper yourself
Turn your PDF publications into a flip-book with our unique Google optimized e-Paper software.
10<br />
<strong>in</strong> which <strong>the</strong> rate <strong>of</strong> change <strong>of</strong> <strong>the</strong> concentration with time is described. This is useful<br />
s<strong>in</strong>ce it enables <strong>the</strong> change <strong>in</strong> concentration to be determ<strong>in</strong>ed at different time<br />
<strong>in</strong>tervals. Fur<strong>the</strong>rmore <strong>the</strong> diffusion coefficient may be given as,<br />
D<br />
Q<br />
/ kT<br />
D0e<br />
(2.5)<br />
where D0 is called <strong>the</strong> pre-exponential factor and is temperature <strong>in</strong>dependent and Q is<br />
<strong>the</strong> energy <strong>of</strong> activation for diffusion which depends on <strong>the</strong> diffus<strong>in</strong>g species.<br />
In general <strong>the</strong> formation energy <strong>of</strong> <strong>in</strong>terstitials is considerably higher than that <strong>of</strong><br />
vacancies but <strong>the</strong>ir migration energy is far lower. This is due to <strong>the</strong> considerable<br />
lattice stra<strong>in</strong> created by <strong>the</strong> <strong>in</strong>terstitial and thus reliev<strong>in</strong>g this stra<strong>in</strong> by means <strong>of</strong><br />
migration should be highly probable. If <strong>in</strong>terstitials are formed <strong>the</strong>rmally or by o<strong>the</strong>r<br />
means <strong>the</strong>y will rapidly migrate to s<strong>in</strong>ks. Such s<strong>in</strong>ks will <strong>in</strong>clude <strong>the</strong> surface, o<strong>the</strong>r<br />
<strong>in</strong>terstitials or vacancies and <strong>extended</strong> <strong>defects</strong>. If <strong>the</strong> <strong>in</strong>terstitials come <strong>in</strong>to contact<br />
<strong>the</strong>y will form stable clusters and if <strong>the</strong>y come <strong>in</strong>to contact with vacancies mutual<br />
annihilation will occur. If two <strong>in</strong>terstitials form a cluster it is termed a di-<strong>in</strong>terstitial<br />
and if three form a cluster it is a tri-<strong>in</strong>terstitial etc. The probability <strong>of</strong> migration <strong>of</strong><br />
<strong>the</strong>se clusters with<strong>in</strong> <strong>the</strong> lattice become <strong>in</strong>creas<strong>in</strong>gly less probable as <strong>the</strong>y <strong>in</strong>crease <strong>in</strong><br />
size and will when reach<strong>in</strong>g a sufficient size act as a s<strong>in</strong>k for <strong>the</strong> migration <strong>of</strong> o<strong>the</strong>r<br />
po<strong>in</strong>t <strong>defects</strong>. The same process holds for vacancy migration with <strong>the</strong> only difference<br />
be<strong>in</strong>g that <strong>the</strong> migration energy for vacancies are much higher than that <strong>of</strong> <strong>in</strong>terstitials.<br />
In general <strong>the</strong> migration energy <strong>of</strong> substitutional impurities <strong>in</strong> <strong>the</strong> lattice is also higher<br />
than that <strong>of</strong> <strong>the</strong> <strong>in</strong>terstitial.<br />
2.4. Dislocations<br />
2.4.1 Introduction<br />
In this section <strong>the</strong> <strong>the</strong>ory <strong>of</strong> dislocations is presented. Concepts <strong>of</strong> dislocation l<strong>in</strong>e and<br />
Burgers vector are expla<strong>in</strong>ed and also different types <strong>of</strong> dislocations <strong>in</strong> a crystal are<br />
discussed. The motion <strong>of</strong> dislocations through <strong>the</strong> processes <strong>of</strong> glide and climb is