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Modular inflation and the orthogonal axion as curvaton

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arxiv hep-ph/0511310 v1 pith:7PRBBWRB submitted 2005-11-28 hep-ph astro-ph

Modular inflation and the orthogonal axion as curvaton

classification hep-ph astro-ph
keywords inflationcurvatonaxionfieldmodularorthogonalscalecandidate
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We study a particular supersymmetric realization of the Peccei-Quinn symmetry which provides a suitable candidate for the curvaton field. The class of models considered also solves the mu problem, while generating the Peccei-Quinn scale dynamically. The curvaton candidate is a pseudo Nambu-Goldstone boson corresponding to an angular degree of freedom orthogonal to the axion field. Its order parameter increases substantially following a phase transition during inflation. This results in a drastic amplification of the curvaton perturbations. Consequently, the mechanism is able to accommodate low-scale inflation with Hubble parameter at the TeV scale. Hence, we investigate modular inflation using a string axion field as the inflaton with inflation scale determined by gravity mediated soft supersymmetry breaking. We find that modular inflation with the orthogonal axion as curvaton can indeed account for the observations for natural values of the parameters.

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  1. George, I and the curvaton

    hep-ph 2026-07 accept novelty 1.0

    A retrospective summary of joint papers that developed the curvaton as an alternative source of cosmic curvature perturbations, including axion and vector realizations.