Preheating after N-flation
| dc.creator | Battefeld, Diana | |
| dc.creator | Kawai, Shinsuke | |
| dc.date | 2008-03-03 | |
| dc.date | 2008-04-17 | |
| dc.date.accessioned | 2026-07-07T11:40:36Z | |
| dc.date.available | 2026-07-07T11:40:36Z | |
| dc.description | We study preheating in N-flation, assuming the Marčenko-Pastur mass distribution, equal energy initial conditions at the beginning of inflation and equal axion-matter couplings, where matter is taken to be a single, massless bosonic field. By numerical analysis we find that preheating via parametric resonance is suppressed, indicating that the old theory of perturbative preheating is applicable. While the tensor-to-scalar ratio, the non-Gaussianity parameters and the scalar spectral index computed for N-flation are similar to those in single field inflation (at least within an observationally viable parameter region), our results suggest that the physics of preheating can differ significantly from the single field case. | |
| dc.description | 14 pages, 14 figures, references added, fixed typos | |
| dc.identifier | https://arxiv.org/abs/0803.0321 | |
| dc.identifier | http://arxiv.org/abs/0803.0321 | |
| dc.identifier | Phys.Rev.D77:123507,2008 | |
| dc.identifier | doi:10.1103/PhysRevD.77.123507 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/200304 | |
| dc.subject | Astrophysics | |
| dc.subject | High Energy Physics - Theory | |
| dc.title | Preheating after N-flation | |
| dc.type | text |