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arxiv: 1612.00998 · v1 · pith:KCL4BY3Znew · submitted 2016-12-03 · ✦ hep-th · astro-ph.CO· gr-qc· hep-ph

Note on Reheating in G-inflation

classification ✦ hep-th astro-ph.COgr-qchep-ph
keywords productiong-inflationinflatonparticlecouplingdrivenefficientevolving
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We study particle production at the end of inflation in kinetically driven G-inflation model and show that, in spite of the fact that there are no inflaton oscillations and hence no parametric resonance instabilities, the production of matter particles due to a coupling to the evolving inflaton field can be more efficient than pure gravitational Parker particle production.

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