Deryagin, Grigoriev, and Rubakov (DGR) have shown that in finite-density QCD at infinite N-c the Fermi surface is unstable with respect to the formation of chiral waves with wavenumber twice the Fermi momentum, while the BCS instability is suppressed. We show here that at large, but finite N-c, the DGR instability only occurs in a finite window of chemical potentials from above Lambda(QCD) to mu(crit) similar to exp(gamma ln(2)N(c) + O(lnN(c)lnlnN(c)))Lambda(QCD), where gamma approximate to 0.02173. Our analysis shows that, at least in the perturbative regime, the instability occurs only at extremely large N-c, N-c greater than or similar to 1000N(f), where N-f is the number of flavors. We conclude that the DGR instability is not likely to occur in QCD with three colors, where the ground state at finite density is expected to be a color superconductor. We speculate on the possible structure of the ground state of finite-density QCD with very large N-c. (C) 2000 Elsevier Science B.V. All rights reserved.
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Austrian Acad Sci, Inst High Energy Phys, Nikolsdorfergasse 18, A-1050 Vienna, AustriaAustrian Acad Sci, Inst High Energy Phys, Nikolsdorfergasse 18, A-1050 Vienna, Austria
Lucha, Wolfgang
Melikhov, Dmitri
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Moscow MV Lomonosov State Univ, DV Skobeltsyn Inst Nucl Phys, Moscow 119991, Russia
Joint Inst Nucl Res, Dubna 141980, Russia
Univ Vienna, Fac Phys, Boltzmanngasse 5, A-1090 Vienna, AustriaAustrian Acad Sci, Inst High Energy Phys, Nikolsdorfergasse 18, A-1050 Vienna, Austria
Melikhov, Dmitri
Sazdjian, Hagop
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Univ Paris Saclay, CNRS, IN2P3, IJCLab, F-91405 Orsay, FranceAustrian Acad Sci, Inst High Energy Phys, Nikolsdorfergasse 18, A-1050 Vienna, Austria