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Paper detail

Towards Axionic Starobinsky-like Inflation in String Theory

It is shown that Starobinsky-like potentials can be realized in non-geometric flux compactifications of string theory, where the inflaton involves an axion whose shift symmetry can protect UV-corrections to the scalar potential. For that purpose we evaluate the backreacted, uplifted F-term axion-monodromy potential, which interpolates between a quadratic and a Starobinsky-like form. Limitations due to the requirements of having a controlled approximation of the UV theory and of realizing single-field inflation are discussed.

preprint2015arXivOpen access
Ralph BlumenhagenAnamaria FontMichael FuchsDaniela HerschmannErik Plauschinn
astro-ph.COhep-phhep-th
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Ralph BlumenhagenAnamaria FontMichael FuchsDaniela HerschmannErik Plauschinn

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