Reconstructing the Primordial Power Spectrum
| dc.creator | Gawiser, Eric | |
| dc.date | 1998-07-31 | |
| dc.date.accessioned | 2026-07-07T02:27:30Z | |
| dc.date.available | 2026-07-07T02:27:30Z | |
| dc.description | 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. | |
| dc.description | 3 pages, to appear in Proceedings of 18th Texas Symposium on Relativistic Astrophysics (Chicago 1996) | |
| dc.identifier | https://arxiv.org/abs/astro-ph/9807328 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/9807328 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/12720 | |
| dc.subject | Astrophysics | |
| dc.title | Reconstructing the Primordial Power Spectrum | |
| dc.type | text |