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Non-abelian discrete gauge symmetries and inflation

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arxiv hep-ph/0001333 v1 pith:5RNH6H2N submitted 2000-01-31 hep-ph astro-phhep-th

J.D. Cohn , E.D. Stewart This is my paper · ORCID
classification hep-phastro-phhep-th
keywords inflationdiscretegaugenon-abelianpotentialsymmetriescasedifficult
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Obtaining a potential flat enough to provide slow roll inflation is often difficult when gravitational effects are included. Non-abelian discrete gauge symmetries can guarantee the flatness of the inflaton potential in this case, and also provide special field values where inflation can end.

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  1. Corrections to inflationary models induced by non-minimal coupling between scalar field and curvature

    gr-qc 2026-07 conditional novelty 5.0 of 10

    Power-law non-minimal coupling F=(H/λ)^{2n} deforms inflationary potentials, shifts r and n_S while preserving n_T=-r/8 and GR-like reheating, enabling r(1-n_S) classification of models against Planck/ACT data.

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