Reconstructing the Primordial Power Spectrum
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.
- Publication:
-
Eighteenth Texas Symposium on Relativistic Astrophysics
- Pub Date:
- 1998
- DOI:
- arXiv:
- arXiv:astro-ph/9807328
- Bibcode:
- 1998tsra.conf..285G
- Keywords:
-
- Astrophysics
- E-Print:
- 3 pages, to appear in Proceedings of 18th Texas Symposium on Relativistic Astrophysics (Chicago 1996)