summaryrefslogtreecommitdiff
path: root/bezout.tex
diff options
context:
space:
mode:
authorJaron Kent-Dobias <jaron@kent-dobias.com>2020-12-09 15:24:16 +0100
committerJaron Kent-Dobias <jaron@kent-dobias.com>2020-12-09 15:24:16 +0100
commit3ee1888e22f2571011de7aabd602502d89062cb5 (patch)
tree549fd444ef5a3dd480be29bf9357d73220a1d463 /bezout.tex
parent5f9db45efcf9ffb2d97a854185a1c505d66b20d2 (diff)
downloadPRR_3_023064-3ee1888e22f2571011de7aabd602502d89062cb5.tar.gz
PRR_3_023064-3ee1888e22f2571011de7aabd602502d89062cb5.tar.bz2
PRR_3_023064-3ee1888e22f2571011de7aabd602502d89062cb5.zip
Fixed an unclosed "teal" environment.
Diffstat (limited to 'bezout.tex')
-rw-r--r--bezout.tex2
1 files changed, 1 insertions, 1 deletions
diff --git a/bezout.tex b/bezout.tex
index 2368a1d..a7ffd08 100644
--- a/bezout.tex
+++ b/bezout.tex
@@ -345,7 +345,7 @@ is the logarithm of the number of configurations of a given $(a,H_0)$.
This problem may be solved exactly with replicas, {\em but it may also be simulated} \cite{Bray_1980_Metastable}.
Consider for example the ground-state energy for given $a$, that is, the energy in the limit $\beta_R \rightarrow \infty$ taken adjusting $\beta_I$ so that $\Im H_0=0$ . For $a=1$ this coincides with the ground-state of the real problem.
-{\color{teal} {\bf somewhere} In Figure \ref{fig:desert} we show that for $\kappa<1$ there is always a gap of $a$ close to one for which there are no solutions: this is natural, given that the $y$ contribution to the volume shrinks to zero as that of an $N$-dimensional sphere $\sim(a-1)^N$.
+{\bf somewhere} In Figure \ref{fig:desert} we show that for $\kappa<1$ there is always a gap of $a$ close to one for which there are no solutions: this is natural, given that the $y$ contribution to the volume shrinks to zero as that of an $N$-dimensional sphere $\sim(a-1)^N$.
For the case $K=1$ -- i.e. the analytic continuation of the usual real computation -- the situation
is more interesting. In the range of values of $\Re H_0$ where there are exactly real solutions this gap closes, and this is only possible if the density of solutions diverges at $a=1$.
Another remarkable feature of the limit $\kappa=1$ is that there is still a gap without solutions around