Finite Density Effect in the Gross-Neveu Model in a Weakly Curved $R^1\times S^2$ Spacetime

dc.creatorKim, Dae Kwan
dc.creatorKlimenko, K. G.
dc.date1997-10-25
dc.date1997-11-08
dc.date.accessioned2026-07-07T10:53:52Z
dc.date.available2026-07-07T10:53:52Z
dc.descriptionThe three-dimensional Gross-Neveu model in $R^{1} \times S^{2}$ spacetime is considered at finite particles number density. We evaluate an effective potential of the composite scalar field $σ(x)$, which is expressed in terms of a scalar curvature $R$ and nonzero chemical potential $μ$. We then derive the critical values of $(R,μ)$ at which the system undergoes the first order phase transition from the phase with broken chiral invariance to the symmetric phase.
dc.descriptionRevTeX, minor changes, new references are added
dc.identifierhttps://arxiv.org/abs/hep-th/9710193
dc.identifierhttp://arxiv.org/abs/hep-th/9710193
dc.identifierJ.Phys.A31:5565,1998
dc.identifierdoi:10.1088/0305-4470/31/25/007
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/185626
dc.subjectHigh Energy Physics - Theory
dc.subjectHigh Energy Physics - Phenomenology
dc.titleFinite Density Effect in the Gross-Neveu Model in a Weakly Curved $R^1\times S^2$ Spacetime
dc.typetext

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