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The two-field regime of natural inflation

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arxiv 1510.08775 v1 pith:DKQLGS6J submitted 2015-10-29 astro-ph.CO hep-phhep-th

The two-field regime of natural inflation

classification astro-ph.CO hep-phhep-th
keywords inflationbreakinghierarchynaturalpredictionscasecomparableconsistent
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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The simplest two-field completion of natural inflation has a regime in which both fields are active and in which its predictions are within the Planck 1-$\sigma$ confidence contour. We show this for the original model of natural inflation, in which inflation is achieved through the explicit breaking of a U(1) symmetry. We consider the case in which the mass coming from explicit breaking of this symmetry is comparable to that from spontaneous breaking, which we show is consistent with a hierarchy between the corresponding energy scales. While both masses are comparable when the observable modes left the horizon, the mass hierarchy is restored in the last e-foldings of inflation, rendering the predictions consistent with the isocurvature bounds. For completeness, we also study the predictions for the case in which there is a large hierarchy of masses and an initial period of inflation driven by the (heavy) radial field.

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