Unified Model for Inflation and Dark Matter
| dc.creator | Zsembinszki, Gabriel | |
| dc.date | 2006-11-21 | |
| dc.date | 2007-03-29 | |
| dc.date.accessioned | 2026-07-07T10:20:56Z | |
| dc.date.available | 2026-07-07T10:20:56Z | |
| dc.description | We present a model which contains a new complex scalar field $Ψ$, interacting with a new real scalar field, $χ$, and an effective potential whose symmetry is almost exact, being explicitly broken by Planck-scale effects. We study the possibility of relating {\em inflation} with the {\em dark matter} of the universe. We find that for exponentially small explicit breaking, the model accounts for a period of inflation in the early universe and gives a dark matter candidate particle. | |
| dc.description | 16 pages, 2 figures, revtex4; more references added, minor changes in the text | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0611664 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0611664 | |
| dc.identifier | J.Phys.A40:5219,2007 | |
| dc.identifier | doi:10.1088/1751-8113/40/19/020 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/175010 | |
| dc.subject | Astrophysics | |
| dc.subject | High Energy Physics - Phenomenology | |
| dc.title | Unified Model for Inflation and Dark Matter | |
| dc.type | text |