Low-scale inflation in a model of dark energy and dark matter
| dc.creator | Hung, P. Q. | |
| dc.creator | Masso, Eduard | |
| dc.creator | Zsembinszki, Gabriel | |
| dc.date | 2006-09-28 | |
| dc.date | 2006-12-05 | |
| dc.date.accessioned | 2026-07-07T10:23:42Z | |
| dc.date.available | 2026-07-07T10:23:42Z | |
| dc.description | We present a complete particle physics model that explains three major problems of modern cosmology: inflation, dark matter and dark energy, and also gives a mechanism for leptogenesis. The model has a new gauge group $SU(2)_Z$ that grows strong at a scale $Λ\sim 10^{-3}$ eV. We focus on the inflationary aspects of the model. Inflation occurs with a Coleman-Weinberg potential at a low scale, down to $\sim 6\times 10^5\gev$, being compatible with observational data. | |
| dc.description | 5 two-column pages, RevTex4; two reference added and minor changes made in the text; published in JCAP | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0609777 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0609777 | |
| dc.identifier | JCAP0612:004,2006 | |
| dc.identifier | doi:10.1088/1475-7516/2006/12/004 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/175926 | |
| dc.subject | Astrophysics | |
| dc.subject | High Energy Physics - Phenomenology | |
| dc.title | Low-scale inflation in a model of dark energy and dark matter | |
| dc.type | text |