Low power on large scales in just enough inflation models
Cosmology and Nongalactic Astrophysics
2012-06-27 v3
Abstract
An early stage of kinetic energy domination for inflation is applied to single-field quadratic and hybrid-type potentials considering only the amount of inflation necessary to solve the problems of the standard cosmological scenario. Using initial conditions inside the 1-sigma interval of the best-fit cosmological parameters for the potentials, low values for the quadrupole component can be obtained.
Keywords
Cite
@article{arxiv.1202.0698,
title = {Low power on large scales in just enough inflation models},
author = {Erandy Ramirez},
journal= {arXiv preprint arXiv:1202.0698},
year = {2012}
}
Comments
8 pages, 8 figures references and new acknowledgement added, accepted for publication