Inflationary models with a flat potential enforced by non-abelian discrete gauge symmetries

Abstract

Non-abelian discrete gauge symmetries can provide the inflaton with a flat potential even when one takes into account gravitational strength effects. The discreteness of the symmetries also provide special field values where inflation can end via a hybrid type mechanism. An interesting feature of this method is that it can naturally lead to extremely flat potentials and so, in principle, to inflation at unusually low energy scales. Two examples of effective field theories with this mechanism are given, one with a hybrid exit and one with a mutated hybrid exit. They include an explicit example in which the single field consistency condition is violated.

24 pages, uses revtex.sty, submitted to PRD (Nov. 1999) Final version to appear in PRD. Background information on supergravity expanded

References in corpus (6)

• The Case for a Positive Cosmological Lambda-term
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• Cosmological Moduli Problem and Thermal Inflation Models
• Hybrid Inflation in Supergravity with $(SU(1,1)/U(1){)}^m$ Khler Manifolds
• Non-abelian discrete gauge symmetries and inflation
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• Hybrid natural inflation from non Abelian discrete symmetry
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• Hybrid Natural Low Scale Inflation
• Evading the Lyth Bound in Hybrid Natural Inflation
• A Permutation on Hybrid Natural Inflation
• Gauged Inflation