We extend previous classifications of inflationary models by means of their behavior at large N, where N is the number of e-foldings. In addition to the perturbative 1/N case, whose slow-roll parameters fall off as powers of 1/N, we introduce the constant, nonperturbative and logarithmic classes. This covers the large majority of inflationary models. Furthermore, we calculate the running of the spectral tilt for all these classes. Remarkably, we find that the tilt's runnings essentially cluster around the per-mil level. We comment on the implications for future experiments.</p
We not only reconstruct the slow-roll parameters for fit to the running spectral index from WMAP thr...
In single field slow-roll inflation, one expects that the spectral index ns − 1 is first order in sl...
The WMAP measurement of the CMB temperature anisotropy is intriguingly consistent with a larger runn...
We extend previous classifications of inflationary models by means of their behavior at large N, whe...
We extend previous classifications of inflationary models by means of their behavior at large N, whe...
We extend previous classifications of inflationary models by means of their behavior at large N, whe...
We extend previous classifications of inflationary models by means of their behavior at large N, whe...
The scalar spectral index n is an important parameter describing the nature of primordial density pe...
The 1/N inflation model can be used to couple CMB measurements to the number of e-foldings of inflat...
The next generation of cosmological observations are expected to improve the measurements of several...
The Inflationary power spectrum plays an important role in modern cosmology. In this thesis, we stud...
AbstractWe revisit large field inflation models with modulations in light of the recent discovery of...
I give a review of predictions of values of spectral parameters for a large number of inflationary m...
We investigate all single-field, slow-roll inflationary models whose slow-roll parameters scale as 1...
I give a review of predictions of values of spectral parameters for a large number of inflationary m...
We not only reconstruct the slow-roll parameters for fit to the running spectral index from WMAP thr...
In single field slow-roll inflation, one expects that the spectral index ns − 1 is first order in sl...
The WMAP measurement of the CMB temperature anisotropy is intriguingly consistent with a larger runn...
We extend previous classifications of inflationary models by means of their behavior at large N, whe...
We extend previous classifications of inflationary models by means of their behavior at large N, whe...
We extend previous classifications of inflationary models by means of their behavior at large N, whe...
We extend previous classifications of inflationary models by means of their behavior at large N, whe...
The scalar spectral index n is an important parameter describing the nature of primordial density pe...
The 1/N inflation model can be used to couple CMB measurements to the number of e-foldings of inflat...
The next generation of cosmological observations are expected to improve the measurements of several...
The Inflationary power spectrum plays an important role in modern cosmology. In this thesis, we stud...
AbstractWe revisit large field inflation models with modulations in light of the recent discovery of...
I give a review of predictions of values of spectral parameters for a large number of inflationary m...
We investigate all single-field, slow-roll inflationary models whose slow-roll parameters scale as 1...
I give a review of predictions of values of spectral parameters for a large number of inflationary m...
We not only reconstruct the slow-roll parameters for fit to the running spectral index from WMAP thr...
In single field slow-roll inflation, one expects that the spectral index ns − 1 is first order in sl...
The WMAP measurement of the CMB temperature anisotropy is intriguingly consistent with a larger runn...