Eric Gawiser
Published 1998-07-31Version 1
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.
Comments: 3 pages, to appear in Proceedings of 18th Texas Symposium on Relativistic Astrophysics (Chicago 1996)
Reconstructing the primordial power spectrum
Recovering the Inflationary Potential and Primordial Power Spectrum With a Slow Roll Prior: Methodology and Application to WMAP 3 Year Data
A Bayesian analysis of the primordial power spectrum
