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Dynamical Fractional Chaotic Inflation -- Dynamical Generation of a Fractional Power-Law Potential for Chaotic Inflation

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arxiv 1407.3084 v1 pith:MOGZAYSK submitted 2014-07-11 hep-ph astro-ph.COhep-th

classification hep-phastro-ph.COhep-th
keywords inflationchaoticdynamicalpotentialfieldfractionaldynamicsgauge
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Chaotic inflation based on a simple monomial scalar potential, V(phi) ~ phi^p, is an attractive large-field model of inflation capable of generating a sizable tensor-to-scalar ratio r. Therefore, assuming that future CMB observations will confirm the large r value reported by BICEP2, it is important to determine what kind of dynamical mechanism could possibly endow the inflaton field with such a simple effective potential. In this paper, we answer this question in the context of field theory, i.e. in the framework of dynamical chaotic inflation (DCI), where strongly interacting supersymmetric gauge dynamics around the scale of grand unification dynamically generate a fractional power-law potential via the quantum effect of dimensional transmutation. In constructing explicit models, we significantly extend our previous work, as we now consider a large variety of possible underlying gauge dynamics and relax our conditions on the field content of the model. This allows us to realize almost arbitrary rational values for the power p in the inflaton potential. The present paper may hence be regarded as a first step towards a more complete theory of dynamical chaotic inflation.

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    β-shifted normal ordering yields quantum lifts for noninteger power-law potentials with α>2, and tames the divergent Stokes amplitude in the σ=4 Pöschl-Teller model into an O(g^{3/4}) scaling.

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