Thermodynamical Limit for Correlated Gaussian Random Energy Models
arXiv:math-ph/0206007 · doi:10.1007/s00220-003-0803-y
Abstract
Let $\{E_{\s}(N)\}_{\s\inΣ_N}$ be a family of centered unit Gaussian random variables defined by the covariance matrix of elements $\displaystyle c_N(\s,τ):=\av{E_{\s}(N)E_τ(N)}$, and $H_N(\s) = - \sqrt{N} E_{\s}(N)$ the corresponding random Hamiltonian. Then the quenched thermodynamical limit exists if, for every decomposition , and all pairs $(\s,\t)\in Σ_N\times Σ_N$: $$ c_N(\s,τ)\leq \frac{N_1}{N} c_{N_1}(π_1(\s),π_1(τ))+ \frac{N_2}{N} c_{N_2}(π_2(\s),π_2(τ)) $$ where $π_k(\s), k=1,2$ are the projections of $\s\inΣ_N$ into . The condition is explicitly verified for the Sherrington-Kirckpatrick, the even -spin, the Derrida REM and the Derrida-Gardner GREM models.
15 pages, few remarks and two references added. To appear in Commun. Math. Phys
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