Pre-inflation models and WMAP data
天体物理学
2007-05-23 v1
摘要
The effect of pre-inflation physics on the power spectrum of scalar perturbations is estimated and there is a possibility that the pre-inflation physics explains the Wilkinson Microwave Anisotropy Probe data if the length of inflation is near 60 e-folds. Considering various pre-inflation models with radiation-dominated or matter-dominated periods before inflation, the power spectrum of curvature perturbations for large scales is calculated, and the spectral index and running spectral index are derived.
关键词
引用
@article{arxiv.astro-ph/0404519,
title = {Pre-inflation models and WMAP data},
author = {Shiro Hirai},
journal= {arXiv preprint arXiv:astro-ph/0404519},
year = {2007}
}
备注
33 pages, 10 figures