| Article ID | Journal | Published Year | Pages | File Type |
|---|---|---|---|---|
| 9861420 | Physics Letters B | 2005 | 7 Pages |
Abstract
Reheating after inflation can occur through inflaton decay or efficient parametric resonant production of particles from the oscillation of the inflaton. If the particles produced interact with scalars that were light during inflation, then significant super-horizon density perturbations are generated during this era. These perturbations can be highly non-Gaussian.
Related Topics
Physical Sciences and Engineering
Physics and Astronomy
Nuclear and High Energy Physics
Authors
Lotty Ackerman, Christian W. Bauer, Michael L. Graesser, Mark B. Wise,