Density of States near the Anderson Transition in a Space of Dimensionality d=4-epsilon

dc.creatorSuslov, I. M.
dc.date1999-12-08
dc.date.accessioned2026-07-07T03:15:27Z
dc.date.available2026-07-07T03:15:27Z
dc.descriptionAsymptotically exact results are obtained for the average Green function and the density of states in a Gaussian random potential for the space dimensionality d=4-epsilon over the entire energy range, including the vicinity of the mobility edge. For N\sim 1 (N is an order of the perturbation theory) only the parquet terms corresponding to the highest powers of 1/epsilon are retained. For large N all powers of 1/epsilon are taken into account with their coefficients calculated in the leading asymptotics in N. This calculation is performed by combining the condition of renormalizability of the theory with the Lipatov asymptotics.
dc.description11 pages, PDF
dc.identifierhttps://arxiv.org/abs/cond-mat/9912132
dc.identifierhttp://arxiv.org/abs/cond-mat/9912132
dc.identifierZh.Eksp.Teor.Fiz. 111 (1997) 1896-1914
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/30034
dc.subjectDisordered Systems and Neural Networks
dc.subjectMesoscale and Nanoscale Physics
dc.subjectHigh Energy Physics - Phenomenology
dc.subjectHigh Energy Physics - Theory
dc.titleDensity of States near the Anderson Transition in a Space of Dimensionality d=4-epsilon
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