Enhanced (p)reheating in DBI Inflation
A. C. Davis, Raquel H. Ribeiro

TL;DR
This paper investigates the process of preheating in DBI hybrid inflation, demonstrating that even with small couplings, narrow parametric resonance efficiently converts inflaton energy into matter fields, leading to reheating.
Contribution
It provides a detailed analysis of preheating dynamics in DBI inflation, highlighting the efficiency of narrow parametric resonance despite weak couplings.
Findings
Preheating occurs via narrow parametric resonance.
The process efficiently produces matter fields at late times.
Reheating temperature is estimated from inflaton decay.
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.
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
Taxonomy
TopicsCosmology and Gravitation Theories · Black Holes and Theoretical Physics · Galaxies: Formation, Evolution, Phenomena
