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| author | Jaron Kent-Dobias <jaron@kent-dobias.com> | 2018-09-24 18:05:19 -0400 |
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| committer | Jaron Kent-Dobias <jaron@kent-dobias.com> | 2018-09-24 18:05:19 -0400 |
| commit | a5e04f76b0dac4fdd6be00018aa0f54e7202c92d (patch) | |
| tree | 32e1170c4079fc97ece830ec54264d2ad1249f9c /monte-carlo.tex | |
| parent | 975e4834c0b54cd06aaf28157789a7d4130adc1a (diff) | |
| parent | 2062625bdcad4341c456d687ff3542285f143e78 (diff) | |
| download | PRE_98_063306-a5e04f76b0dac4fdd6be00018aa0f54e7202c92d.tar.gz PRE_98_063306-a5e04f76b0dac4fdd6be00018aa0f54e7202c92d.tar.bz2 PRE_98_063306-a5e04f76b0dac4fdd6be00018aa0f54e7202c92d.zip | |
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| -rw-r--r-- | monte-carlo.tex | 12 |
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diff --git a/monte-carlo.tex b/monte-carlo.tex index d202ef5..370ac0f 100644 --- a/monte-carlo.tex +++ b/monte-carlo.tex @@ -534,6 +534,14 @@ 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 @@ -552,6 +560,7 @@ perturbations on spin models can be tested numerically \cite{jose_renormalization_1977, blankschtein_fluctuation-induced_1982, bruce_coupled_1975, manuel_carmona_$n$-component_2000}. +<<<<<<< HEAD \appendix \section{$\mathrm O(n)$ model at high field} @@ -620,6 +629,9 @@ whence \end{align} \section{Calculating autocorrelation time} +\begin{figure*} + \include{fig_correlation-times} +\end{figure*} \begin{acknowledgments} This work was supported by NSF grant NSF DMR-1719490. |