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Low-scale Quintessential Inflation
In quintessential inflationary model, the same master field that drives inflation becomes, later on, the dynamical source of the (present) accelerated expansion. Quintessential inflationary models require a curvature scale at the end of inflation around $10^{-6}M_{\rm P}$ in order to explain the lar...
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| Lenguaje: | eng |
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2003
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| Acceso en línea: | https://dx.doi.org/10.1103/PhysRevD.67.123512 http://cds.cern.ch/record/603279 |