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Diquarks and Density

M. B. Hecht, C. D. Roberts, S. M. Schmidt

Published 2000-12-06, updated 2000-12-08Version 2

We describe aspects of the role that diquark correlations play in understanding baryon structure and interactions. The significance of diquarks in that application motivates a study of the possibility that dense hadronic matter may exhibit diquark condensation; i.e., quark-quark pairing promoted by a quark chemical potential. A Gorkov-Nambu-like gap equation is introduced for QCD and analysed for 2-colour QCD (QC2D) and, in two qualitatively different truncations, for QCD itself. Among other interesting features, we illustrate that QC2D with massive fermions undergoes a second-order transition to a superfluid phase when the chemical potential exceeds 0.5 m.pi. In the QCD application we illustrate that the sigma= <bar-q q> .neq. 0 phase, which determines the properties of the mass spectrum at zero temperature and chemical potential, is unstable with respect to the superfluid phase when the chemical potential exceeds approx. 2 sigma, and that at this point the diquark gap is large, approx. 0.5 sigma. The superfluid phase survives to temperatures greater than that expected in the core of compact stars.

Comments: 16 pages, LaTeX2e, Contribution to the Proceedings of "Physics of Neutron Star Interiors," a workshop at ECT$\ast$, Trento, Italy, June-July/2000, Eds. D. Blaschke, N.K. Glendenning and A. Sedrakian. No changes
Journal: Lect.Notes Phys.578:218-234,2001
Categories: nucl-th, hep-lat, hep-ph
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