Spotted Inflation
Abstract
We describe new scenarios of generating curvature perturbations when inflaton (curvaton) has significant interactions. We consider a ``spot'', which arises from interactions associated with enhanced symmetric point (ESP) on the trajectory. Our first example uses the spot to induce a gap to the field equation. We observe that the gap in the field equation may cause generation of curvature perturbation if it appears not simultaneous in space. The mechanism is similar to the scenario of inhomogeneous phase transition. Then we observe that the spot interactions may initiate warm inflation in the cold Universe. Creation of cosmological perturbation is discussed in relation to the inflaton dynamics and the modulation associated with the spot interactions.
Cite
@article{arxiv.1008.0164,
title = {Spotted Inflation},
author = {Tomohiro Matsuda},
journal= {arXiv preprint arXiv:1008.0164},
year = {2010}
}
Comments
29pages, 2 figures, footnotes are added for clarification, accepted for publication in JCAP