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arxiv: 1502.06135 · v2 · pith:EBLYF553new · submitted 2015-02-21 · ✦ hep-th · astro-ph.CO· gr-qc· hep-ph

Preheating with Fractional Powers

classification ✦ hep-th astro-ph.COgr-qchep-ph
keywords inflatonfieldpotentialfractionalinstabilitypreheatinganharmonicassume
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We consider preheating in models in which the potential for the inflaton is given by a fractional power, as is the case in axion monodromy inflation. We assume a standard coupling between the inflaton field and a scalar matter field. We find that in spite of the fact that the oscillation of the inflaton about the field value which minimizes the potential is anharmonic, there is nevertheless a parametric resonance instability, and we determine the Floquet exponent which describes this instability as a function of the parameters of the inflaton potential.

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