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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. |