X-Git-Url: https://hackdaworld.org/gitweb/?p=lectures%2Flatex.git;a=blobdiff_plain;f=posic%2Fthesis%2Fsummary_outlook.tex;fp=posic%2Fthesis%2Fsummary_outlook.tex;h=f5dc9aa8085cf913c9072882b81cef0f263311ba;hp=8d5b28e4a08554a6b846f370609eb6ac5f8adbe6;hb=74eed718613ff04a1e09a6a5663ac4d38f733e61;hpb=a498ec4871627a0d0dc230022a5166af1db7d702

diff --git a/posic/thesis/summary_outlook.tex b/posic/thesis/summary_outlook.tex
index 8d5b28e..f5dc9aa 100644
--- a/posic/thesis/summary_outlook.tex
+++ b/posic/thesis/summary_outlook.tex
@@ -96,7 +96,7 @@ Thus, elevated temperatures might lead to configurations of C$_{\text{s}}$ and a
 % maybe preliminary conclusions here ...
 
 Classical potential MD calculations targeting the direct simulation of SiC precipitation in Si are adopted.
-Therefore, the necessary amount of C is gradually incorporated into a large c-Si host.
+Therefor, the necessary amount of C is gradually incorporated into a large c-Si host.
 Simulations at temperatures used in IBS result in structures dominated by the C$_{\text{i}}$ \hkl<1 0 0> DB and its combinations if C is inserted into the total volume.
 Incorporation into volumes $V_2$ and $V_3$, which correspond to the volume of the expected precipitate and the volume containing the necessary amount of Si, lead to an amorphous SiC-like structure within the respective volume.
 Both results are not expected with respect to the outcome of the IBS experiments.