Predictions of single field inflation for the tensor/scalar ratio and the running spectral index
Résumé
We study the single field slow-roll inflation models that better agree with the available CMB and LSS data including the three years WMAP data: new inflation and hybrid inflation. We study these models as effective field theories in the Ginsburg-Landau context: a trinomial potential turns out to be a simple and well motivated model. The spectral index ns of the adiabatic fluctuations, the ratio r of tensor to scalar fluctuations and the running index dns/dlnf k are studied in detail. We derive explicit formulas for ns, r and dns/dlnf k and provide relevant plots. In new inflation, and for the chosen central value ns=0.95, we predict 0.03
Domaines
Astrophysique [astro-ph]Origine | Fichiers éditeurs autorisés sur une archive ouverte |
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