pith. sign in

arxiv: 0908.4217 · v1 · submitted 2009-08-28 · ✦ hep-th · astro-ph.CO· hep-ph

Enhanced (p)reheating in DBI Inflation

classification ✦ hep-th astro-ph.COhep-ph
keywords inflatonpreheatingfieldsinflationmatterreheatingresonanceapproximations
0
0 comments X
read the original abstract

We study preheating in DBI hybrid inflation. Preheating occurs since the matter fields are non-minimally coupled to the inflaton. Despite the coupling being small, preheating happens as a narrow parametric resonance in which matter fields and inflaton modes are exponentially created. We show that, within the approximations used, the process is very efficient at late times. The resonance stage gives way to the decay of the inflaton into bosonic or fermionic degrees of freedom and the corresponding reheating temperature is determined.

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.