Physics – High Energy Physics – High Energy Physics - Phenomenology
Scientific paper
2002-04-17
Physics
High Energy Physics
High Energy Physics - Phenomenology
10 pages, 1 figure, Talk at DM2002, Cape Town, South Africa
Scientific paper
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) with N$\gg$1. Appealing to a thermodynamical treatment, the ground-state structure of the model is determined by a potential for the inflaton field (monopole condensate) which allows for nontrivially BPS saturated and thereby stable solutions. For $T
Hofmann Ralf
Keil Mathias Th.
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