2002
DOI: 10.1007/978-3-642-59440-3_3
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Cited by 14 publications
(21 citation statements)
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“…The latter exponential factor suppresses the instanton excitation significantly. Similarly, at finite density, the exponential suppression factor has been found [57], and after integrating over the instanton size, the suppression factor should be T −14 or µ −14 . In any case these expressions are perturbative ones, and any quantitative estimate is not really trustworthy near T c .…”
Section: U(1) a Symmetry And The Quantum Anomalymentioning
confidence: 83%
“…The latter exponential factor suppresses the instanton excitation significantly. Similarly, at finite density, the exponential suppression factor has been found [57], and after integrating over the instanton size, the suppression factor should be T −14 or µ −14 . In any case these expressions are perturbative ones, and any quantitative estimate is not really trustworthy near T c .…”
Section: U(1) a Symmetry And The Quantum Anomalymentioning
confidence: 83%
“…It was pointed by Weinberg that in the superconducting system expression for the condensation free energy evaluated on the solution to the gap equation does not depend on the microscopic interaction between particles [28]. Later Schaefer demonstrated that the expression for the free energy of quark matter in the mean field approximation when evaluated on the solution to the gap equation coincides with the expression for free energy of quark matter with colorflavor antisymmetric short range interactions in the mean field approximation (NJL model) [29]. With this in mind, our approximation is equivalent to working in the model with a color-flavor antisymmetric short range interactions (NJL model) in the mean field approximation with a given value of gap parameter [7,29] and the role of gauge fields is only to ensure the gauge charge neutrality of the ground state [30,31].…”
Section: A Setup Approximations and Assumptionsmentioning
confidence: 99%
“…The phase diagram of quantum chromodynamics (QCD) is expected to contain color-superconducting regimes at sufficiently high densities and low temperatures [1,2,3,4,5,6,7]. Considering three (degenerate) quark flavors, the color-flavor locked (CFL) phase [8] is the ground-state for vanishing temperatures and asymptotically large densities [9,10]. At densities of potential relevance for compact stellar objects it is, however, not obvious how the splitting of Fermi surfaces due to finite quark masses and neutrality constraints is influencing the ground-state [11,12,13].…”
Section: Introductionmentioning
confidence: 99%