From: hackbard <hackbard@sage.physik.uni-augsburg.de>
Date: Tue, 31 May 2011 16:11:44 +0000 (+0200)
Subject: finished xxx mig
X-Git-Url: https://hackdaworld.org/cgi-bin/gitweb.cgi?a=commitdiff_plain;h=bddc8d909e9a701c50ee4f68163343067faf9f69;p=lectures%2Flatex.git

finished xxx mig
---

diff --git a/posic/thesis/defects.tex b/posic/thesis/defects.tex
index 5780990..b8a58fb 100644
--- a/posic/thesis/defects.tex
+++ b/posic/thesis/defects.tex
@@ -1181,6 +1181,8 @@ Again, conclusions concerning the probability of formation are drawn by investig
 Since C$_{\text{s}}$ is unlikely to exhibit a low activation energy for migration the focus is on C$_{\text{i}}$.
 Pathways starting from the next most favored configuration, i.e. \cs{} located at position 2, into configuration a and b are investigated, which show activation energies above \unit[2.2]{eV} and \unit[2.5]{eV}.
 The respective barriers and structures are shown in Fig.~\ref{fig:051-xxx}.
+Again, the non-magnetic configuration is obtained.
+If not forced by the CRT algorithm, the structures beyond \perc{50} displacement of the transition into configuration a would likewise settle into configuration b.
 \begin{figure}[tp]
 \begin{center}
 \includegraphics[width=0.7\textwidth]{comb_mig_051-xxx_conf.ps}