Reconstructing the Primordial Power Spectrum
Astrophysics
2007-05-23 v1
Abstract
Cosmological models predict transfer functions by which primordial density perturbations develop into CMB anisotropy and Large-Scale Structure. We use the current set of observations to reconstruct the primordial power spectrum for standard CDM, CDM with a cosmological constant, open CDM, and standard CDM with a high baryon content.
Cite
@article{arxiv.astro-ph/9807328,
title = {Reconstructing the Primordial Power Spectrum},
author = {Eric Gawiser},
journal= {arXiv preprint arXiv:astro-ph/9807328},
year = {2007}
}
Comments
3 pages, to appear in Proceedings of 18th Texas Symposium on Relativistic Astrophysics (Chicago 1996)