Low scale inflation and the curvaton mechanism = Inflacion de baja energia y el mecanismo del curvaton
The primordial curvature perturbation may be due to a `curvaton' field, which dominates (or almost dominates) the energy density before it decays. In the simplest version of the curvaton model the scale of inflation has to be quite high corresponding to a Hubble parameter H>10^7 GeV. We here...
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| Formato: | Artículo (Article) |
| Lenguaje: | Desconocido (Unknown) |
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Journal of High Energy Physics; Vol. 2, No. 55
2005
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| Acceso en línea: | http://babel.banrepcultural.org/cdm/ref/collection/p17054coll23/id/445 |