Microscopic spectral density in random matrix models for chiral and diquark condensation
arXiv:hep-ph/0208085 · doi:10.1103/PhysRevD.67.085016
Abstract
We examine random matrix models of QCD which are capable of supporting both chiral and diquark condensation. A numerical study of the spectral densities near zero virtuality shows that the introduction of color in the interactions does not alter the one-body results imposed by chiral symmetry. A model with three colors has the spectral density predicted for the chiral ensemble with a Dyson index beta = 2; a pseudoreal model with two colors exhibits the spectral density of the chiral ensemble with beta = 1.
6 pages, 3 eps figures, uses revtex4 and graphicx. v2 : minor editions, Fig. 3 shows relative deviations rather than absolute. Version to appear in PRD
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Cited by in corpus (6)
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- Relativistic Cooper pairing in the microscopic limit of chiral random matrix theory
- Random matrix model for antiferromagnetism and superconductivity on a two-dimensional lattice