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Higher Derivative Four-Fermion Model in Curved Spacetime

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arxiv hep-th/9411216 v1 pith:CZRLV4I6 submitted 1994-11-29 hep-th

classification hep-th
keywords curvaturecurvedmodelspacetimederivativefour-fermionhigherphase
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abstract

We discuss the phase structure of a higher derivative four-fermion model in four dimensions in curved spacetime in frames of the $\frac{1}{N_c}$-expansion. First, we evaluate in our model the effective potential of two composite scalars in the linear curvature approximation using a local momentum representation in curved spacetime for the higher-derivative propagator which naturally appears. The symmetry breaking phenomenon and phase transition induced by curvature are numerically investigated. A numerical study of the dynamically generated fermionic mass, which depends on the coupling constants and on the curvature, is also presented.

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  1. Chiral symmetry and curvature bounds in de Sitter spacetime

    hep-th 2026-07 reject novelty 4.0 of 10

    In the NJL model on de Sitter with an exponential proper-time cutoff, requiring a real constituent fermion mass imposes Λ_cosmo ≤ 6Λ_UV²/e².

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