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arxiv: hep-ph/9905256 · v1 · submitted 1999-05-05 · ✦ hep-ph · astro-ph· hep-th

Inflationary Reheating and Fermions

classification ✦ hep-ph astro-phhep-th
keywords fermionsproductioncreatedfermioninflationinflatonpreheatingalthough
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Coherent oscillations of the inflaton field at the end of inflation can parametrically excite fermions in much the same way that bosons are created in preheating. Although Pauli-blocking prohibits the occupation number of created fermions from growing exponentially, fermion production occurs in a manner significantly different from the expectations of simple perturbation theory. Here, I discuss the nature of fermion production after inflation and possible applications including the efficient transfer of inflaton energy and the production of super-massive fermions during fermionic preheating.

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