Gauged Inflation

Details Gauged Inflation Gauged Inflation

2001-11-07

arxiv.org/abs/hep-ph/0111076v3

Phys.Rev. D66 (2002) 023527

Physics

High Energy Physics

High Energy Physics - Phenomenology

23 pages, 4 figures, subsection added, revision of text, to app. in PRD

Scientific paper

10.1103/PhysRevD.66.023527

We propose a model for cosmic inflation which is based on an effective description of strongly interacting, nonsupersymmetric matter within the framework of dynamical Abelian projection and centerization. The underlying gauge symmetry is assumed to be $SU(N+1)$ with $N \gg 1$. Appealing to a thermodynamical treatment, the ground-state structure of the model is classically determined by a potential for the inflaton field (dynamical monopole condensate) which allows for nontrivially BPS saturated and thereby stable solutions. For $T

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