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R-symmetric Axion/Natural Inflation in Supergravity via Deformed Moduli Dynamics

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arxiv 1409.0330 v1 pith:27NHJ6TA submitted 2014-09-01 hep-ph astro-ph.COhep-th

R-symmetric Axion/Natural Inflation in Supergravity via Deformed Moduli Dynamics

classification hep-ph astro-ph.COhep-th
keywords inflatoncondensationdeformeddynamicsgeneratedinflationmodelmoduli
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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We construct a natural inflation model in supergravity where the inflaton is identified with a modulus field possessing a shift symmetry. The superpotential for the inflaton is generated by meson condensation due to strong dynamics with deformed moduli constraints. In contrast to models based on gaugino condensation, the inflaton potential is generated without $R$-symmetry breaking and hence does not depend on the gravitino mass. Thus, our model is compatible with low scale supersymmetry.

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Cited by 1 Pith paper

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  1. An Intermediate Scale R-axion \& the QCD Axion

    hep-th 2026-07 conditional novelty 7.0

    A mixed F- and D-term uplift in supergravity evades the Planckian lower bound on the R-axion decay constant, allowing it to be the QCD axion and dark matter.