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Note on Reheating in G-inflation

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arxiv 1612.00998 v1 pith:KCL4BY3Z submitted 2016-12-03 hep-th astro-ph.COgr-qchep-ph

Hossein Bazrafshan Moghaddam , Robert Brandenberger , Jun'ichi Yokoyama This is my paper
classification hep-thastro-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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Cited by 1 Pith paper

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  1. Noncanonical Approaches To Inflation

    gr-qc 2019-06 unverdicted novelty 3.0 of 10

    A review thesis covering Mukhanov parametrization, general scalar-tensor theories, and new slow-roll techniques for canonical and noncanonical inflation observables.

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