1998/07/31 by Eric Gawiser, Gawiser, Eric
Physics and Astronomy · #Astrophysics (astro-ph) #FOS: Physical sciences #astro-ph
paper · pdf · doi:10.48550/arxiv.astro-ph/9807328
3 pages, to appear in Proceedings of 18th Texas Symposium on Relativistic Astrophysics (Chicago 1996)
arxiv created 1998/07/31 · arxiv updated 2009/12/01
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.