Direct Detection of Cold Dark Matter
| dc.creator | Baudis, Laura | |
| dc.date | 2007-11-25 | |
| dc.date.accessioned | 2026-07-07T08:44:49Z | |
| dc.date.available | 2026-07-07T08:44:49Z | |
| dc.description | We know from cosmological and astrophysical observations that more than 80% of the matter density in the Universe is non-luminous, or dark. This non-baryonic dark matter could be composed of neutral, heavy particles, which were non-relativistic, or 'cold', when they decoupled from ordinary matter. I will review the direct detection methods of these hypothetical particles via their interactions with nuclei in ultra-low background, deep underground experiments. The emphasis is on most recent results and on the status of near future projects. | |
| dc.description | 10 pages, 11 figures; submitted for the SUSY07 proceedings | |
| dc.identifier | https://arxiv.org/abs/0711.3788 | |
| dc.identifier | http://arxiv.org/abs/0711.3788 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/142795 | |
| dc.subject | Astrophysics | |
| dc.title | Direct Detection of Cold Dark Matter | |
| dc.type | text |