We investigate all single-field, slow-roll inflationary models whose slow-roll parameters scale as 1/N in the limit of a large number of e-folds N. We proof that all such models belong to two universality classes, characterised by a single parameter. One class contains small field models like hilltop inflation, while the other class consists of large field models like chaotic inflation. We give the leading expressions for the spectral index and tensor-to-scalar ratio r, which are universal for each class, plus subleading corrections for a number of models. This predicts r either to be unobservably small, r < 0.01, or close to the present observational limit, r ≈ 0.07
We show that the cosmological evolution of a scalar field in a potential can be obtained from a reno...
We provide strong evidence for universality of the inflationary field range: given an accurate measu...
We provide strong evidence for universality of the inflationary field range: given an accurate measu...
We investigate all single-field, slow-roll inflationary models whose slow-roll parameters scale as 1...
We investigate all single-field, slow-roll inflationary models whose slow-roll parameters scale as 1...
We investigate all single-field, slow-roll inflationary models whose slow-roll parameters scale as 1...
We investigate all single-field, slow-roll inflationary models whose slow-roll parameters scale as 1...
We show that the cosmological evolution of a scalar field in a potential can be obtained from a reno...
We show that the cosmological evolution of a scalar field in a potential can be obtained from a reno...
We study to what extent the spectral index ns and the tensor-to-scalar ratio r determine the field...
We study to what extent the spectral index ns and the tensor-to-scalar ratio r determine the field e...
We study to what extent the spectral index ns and the tensor-to-scalar ratio r determine the field e...
We study to what extent the spectral index ns and the tensor-to-scalar ratio r determine the field e...
We study to what extent the spectral index ns and the tensor-to-scalar ratio r determine the field e...
We study to what extent the spectral index ns and the tensor-to-scalar ratio r determine the field e...
We show that the cosmological evolution of a scalar field in a potential can be obtained from a reno...
We provide strong evidence for universality of the inflationary field range: given an accurate measu...
We provide strong evidence for universality of the inflationary field range: given an accurate measu...
We investigate all single-field, slow-roll inflationary models whose slow-roll parameters scale as 1...
We investigate all single-field, slow-roll inflationary models whose slow-roll parameters scale as 1...
We investigate all single-field, slow-roll inflationary models whose slow-roll parameters scale as 1...
We investigate all single-field, slow-roll inflationary models whose slow-roll parameters scale as 1...
We show that the cosmological evolution of a scalar field in a potential can be obtained from a reno...
We show that the cosmological evolution of a scalar field in a potential can be obtained from a reno...
We study to what extent the spectral index ns and the tensor-to-scalar ratio r determine the field...
We study to what extent the spectral index ns and the tensor-to-scalar ratio r determine the field e...
We study to what extent the spectral index ns and the tensor-to-scalar ratio r determine the field e...
We study to what extent the spectral index ns and the tensor-to-scalar ratio r determine the field e...
We study to what extent the spectral index ns and the tensor-to-scalar ratio r determine the field e...
We study to what extent the spectral index ns and the tensor-to-scalar ratio r determine the field e...
We show that the cosmological evolution of a scalar field in a potential can be obtained from a reno...
We provide strong evidence for universality of the inflationary field range: given an accurate measu...
We provide strong evidence for universality of the inflationary field range: given an accurate measu...