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| author | Jaron Kent-Dobias <jaron@kent-dobias.com> | 2018-09-24 15:27:05 -0400 |
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| committer | Jaron Kent-Dobias <jaron@kent-dobias.com> | 2018-09-24 15:27:05 -0400 |
| commit | 1676b1bfc1544ba7049f198cb4ae75bea0513014 (patch) | |
| tree | 0b66bf74271c6049bb7d7de86833de5ba3e6a789 /monte-carlo.tex | |
| parent | 240f82255f0570d07139daab702459ab0ea2fce9 (diff) | |
| download | PRE_98_063306-1676b1bfc1544ba7049f198cb4ae75bea0513014.tar.gz PRE_98_063306-1676b1bfc1544ba7049f198cb4ae75bea0513014.tar.bz2 PRE_98_063306-1676b1bfc1544ba7049f198cb4ae75bea0513014.zip | |
many figure changes
Diffstat (limited to 'monte-carlo.tex')
| -rw-r--r-- | monte-carlo.tex | 12 |
1 files changed, 12 insertions, 0 deletions
diff --git a/monte-carlo.tex b/monte-carlo.tex index 7aca41a..010b588 100644 --- a/monte-carlo.tex +++ b/monte-carlo.tex @@ -545,6 +545,14 @@ conjecture. \label{fig:cluster_scaling} \end{figure*} +\begin{figure} + \include{fig_generator-times} +\end{figure} + +\begin{figure} + \include{fig_harmonic-susceptibilities} +\end{figure} + We have taken several disparate extensions of cluster methods to spin models in an external field and generalized them to work for any model of a broad class. The resulting representation involves the introduction of not a ghost @@ -563,6 +571,10 @@ perturbations on spin models can be tested numerically \cite{jose_renormalization_1977, blankschtein_fluctuation-induced_1982, bruce_coupled_1975, manuel_carmona_$n$-component_2000}. +\begin{figure*} + \include{fig_correlation-times} +\end{figure*} + \begin{acknowledgments} This work was supported by NSF grant NSF DMR-1719490. \end{acknowledgments} |