New physics from the Cosmic Microwave Background
| dc.creator | Scott, Douglas | |
| dc.date | 1999-11-17 | |
| dc.date.accessioned | 2026-07-07T02:34:30Z | |
| dc.date.available | 2026-07-07T02:34:30Z | |
| dc.description | I review the present status of the Cosmic Microwave Background, with some emphasis on the current and future implications for particle physics. Conclusions are: gravitational instability in a dark matter dominated universe grew today's structure; the Universe remained neutral until z<~50; the CMB power spectrum peaks at 150<~l<~350; the large-scale structure of spacetime appears to be simple; something like inflation is something like proven; we will learn a great deal about cosmology, astrophysics and particle physics from MAP and Planck. | |
| dc.description | 18 pages using iopconf1.sty, including 2 colour and 2 b&w figures, to appear in "Beyond the Desert `99", edited by H.V. Klapdor-Kleingrothaus | |
| dc.identifier | https://arxiv.org/abs/astro-ph/9911325 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/9911325 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/15269 | |
| dc.subject | Astrophysics | |
| dc.subject | High Energy Physics - Phenomenology | |
| dc.title | New physics from the Cosmic Microwave Background | |
| dc.type | text |