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Fermion production during preheating after hybrid inflation

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arxiv hep-ph/0002076 v2 pith:OWCFQVYV submitted 2000-02-07 hep-ph astro-ph

classification hep-phastro-ph
keywords productionduringfermioninflationpreheatinghybridinflatoncoherent
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At the end of inflation, the coherent oscillations of the inflaton field may resonantly amplify the long wavelength modes of both bosons and fermions coupled to it. We study the resonant production of both kinds of particles during preheating in a model of hybrid inflation. The coherent time evolution of the inflaton and the Higgs fields after inflation induce a very different production of fermions depending on whether they are coupled to the Higgs or to the inflaton. For reasonable values of the model parameters, the fermion production through parametric resonance can be very efficient. We study the relative growth of the fermion and boson energy densities during preheating in hybrid models. During the initial stage of preheating, fermion production dominates the relative energy density, while the exponential growth of bosonic modes soon takes over.

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  1. Fermion (non)reheating with a quartic inflaton potential

    hep-ph 2025-12 conditional novelty 6.0 of 10

    In the quartic T-model, inflaton decay to fermions is strongly suppressed by Pauli blocking and parametric resonance, so fermion-only reheating is effectively impossible unless y ≳ 0.2 or a scalar channel is added.

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