English

Inflationary Reheating and Fermions

High Energy Physics - Phenomenology 2009-10-31 v1 Astrophysics High Energy Physics - Theory

Abstract

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.

Keywords

Cite

@article{arxiv.hep-ph/9905256,
  title  = {Inflationary Reheating and Fermions},
  author = {Patrick B. Greene},
  journal= {arXiv preprint arXiv:hep-ph/9905256},
  year   = {2009}
}

Comments

3 pages, LaTeX, uses aipproc.sty and epsf.sty, 4 eps figs included. Based on an invited talk at the 2nd International Workshop on Particle Physics and the Early Universe (Cosmo-98), Monterey CA, Nov. 1998. Proceedings in press

R2 v1 2026-07-22T14:50:58.327Z