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| author | Jaron Kent-Dobias <jaron@kent-dobias.com> | 2018-05-15 13:42:47 -0400 |
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| committer | Jaron Kent-Dobias <jaron@kent-dobias.com> | 2018-05-15 13:42:47 -0400 |
| commit | aa3a9b340fafc65c9cee72c1d8c10f5d6f179d77 (patch) | |
| tree | ae52893a3e3ada881f6127469c716b5a62eb6d9f /monte-carlo.tex | |
| parent | 36e1822423a973dee2861933bf6ffd96ddb04b9d (diff) | |
| download | PRE_98_063306-aa3a9b340fafc65c9cee72c1d8c10f5d6f179d77.tar.gz PRE_98_063306-aa3a9b340fafc65c9cee72c1d8c10f5d6f179d77.tar.bz2 PRE_98_063306-aa3a9b340fafc65c9cee72c1d8c10f5d6f179d77.zip | |
added reference to ising.jsarxiv_v2
Diffstat (limited to 'monte-carlo.tex')
| -rw-r--r-- | monte-carlo.tex | 5 |
1 files changed, 4 insertions, 1 deletions
diff --git a/monte-carlo.tex b/monte-carlo.tex index a305aa8..222d6ed 100644 --- a/monte-carlo.tex +++ b/monte-carlo.tex @@ -395,7 +395,10 @@ Since the symmetry group and the spins are described by the same elements, performing the algorithm on the Ising model in a field is fully described by just using the `ghost spin' representation. This algorithm or algorithms based on the same decomposition of the Hamiltonian have been applied -by several researchers \cite{alexandrowicz_swendsen-wang_1989, wang_clusters_1989, ray_metastability_1990}. +by several researchers \cite{alexandrowicz_swendsen-wang_1989, +wang_clusters_1989, ray_metastability_1990}. The algorithm has been +implemented by one of the authors in an existing interactive Ising +simulator at \texttt{https://mattbierbaum.github.io/ising.js} \cite{bierbaum_ising.js_nodate}. \emph{The $\mathrm O(n)$ model.} In the $\mathrm O(n)$ model spins are described by vectors on the $(n-1)$-sphere $S^{n-1}$. Its symmetry group is $O(n)$, $n\times n$ orthogonal |