1994
DOI: 10.1088/0305-4470/27/18/020
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Quenched random graphs

Abstract: Spin models on quenched random graphs are related to many important optimization problems. We give a new derivation of their mean-field equations that elucidates the role of the natural order parameter in these models.

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Cited by 27 publications
(61 citation statements)
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“…To calculate the partition function Z(β) of the Ising model at inverse temperature β on the graph of figure 1, we consider the leaves of the uncovered local tree i.e. vertices at distance D from the root (in figure 1 the maximum drawn distance is D = 2) [11,8,9,12,10,13]. At sufficiently large β, a spontaneous, say, positive magnetization m is expected to be present in the bulk.…”
Section: Loops With Multiple Crossingsmentioning
confidence: 99%
“…To calculate the partition function Z(β) of the Ising model at inverse temperature β on the graph of figure 1, we consider the leaves of the uncovered local tree i.e. vertices at distance D from the root (in figure 1 the maximum drawn distance is D = 2) [11,8,9,12,10,13]. At sufficiently large β, a spontaneous, say, positive magnetization m is expected to be present in the bulk.…”
Section: Loops With Multiple Crossingsmentioning
confidence: 99%
“…It would obviously be better to have a more trustworthy formalism for investigating quenched problems where such troubles did not arise and one could confidently calculate with an arbitrary number of replicas. Such a formalism is actually inherent in the matrix model approach in a limit that is opposite in a sense to that usually considered, namely N → 1 [8]. In this limit the fat graphs that build the surfaces or their duals in the matrix model integrals degenerate to "thin" graphs -in other words zero dimensional Feynman diagrams.…”
Section: Introductionmentioning
confidence: 99%
“…In this limit the fat graphs that build the surfaces or their duals in the matrix model integrals degenerate to "thin" graphs -in other words zero dimensional Feynman diagrams. Such graphs have in fact been considered before in the context of spin glass theories [9], without utilizing the methods of field theory and large order expansions of [8]. The generic problems in the matrix model approach for c > 1 can be traced to the difficulty in evaluating angular integrals that arise from diagonalizing the matrices, and these disappear for N = 1.…”
Section: Introductionmentioning
confidence: 99%
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“…In particular, one finds mean-field like behaviour for the spin models due to the locally-tree-like structure of the graphs. This approach is based on the simple observation [3] that the thin graphs appear as the Feynman diagrams in the perturbative expansion of matrix models when the N → 1 (scalar) limit is taken. An alternative N → ∞ limit is perhaps more familiar for matrix models in the context of two-dimensional gravity, where the resulting "fat" graphs are of interest because of their relation to surfaces and string worldsheets.…”
Section: Introductionmentioning
confidence: 99%