Precision of Inflaton Potential Reconstruction from CMB Using the General Slow-Roll Approximation
Astrophysics
2008-11-26 v3 High Energy Physics - Phenomenology
Abstract
Through a principal component analysis, we study how accurately CMB observables can constrain inflaton potentials in a model independent manner. We apply the general slow-roll approximation in our analysis where we allow, in contrast to the standard slow-roll approximation, the possibility of variations in and take into account the fact that horizon crossing is not an instantaneous event. Our analysis provides a set of modes to be used in fitting observables. We find that of order five of these modes will be constrained by future observations, so a fully general data analysis package could use the amplitudes of just a handful of modes as free parameters and retain all relevant information in the data.
Keywords
Cite
@article{arxiv.astro-ph/0505158,
title = {Precision of Inflaton Potential Reconstruction from CMB Using the General Slow-Roll Approximation},
author = {Kenji Kadota and Scott Dodelson and Wayne Hu and Ewan D. Stewart},
journal= {arXiv preprint arXiv:astro-ph/0505158},
year = {2008}
}