Introduction to Non-Baryonic Dark Matter
| dc.creator | Gondolo, Paolo | |
| dc.date | 2004-03-02 | |
| dc.date.accessioned | 2026-07-07T02:12:28Z | |
| dc.date.available | 2026-07-07T02:12:28Z | |
| dc.description | These lectures on non-baryonic dark matter matter are divided into two parts. In the first part, I discuss the need for non-baryonic dark matter in light of recent results in cosmology, and I present some of the most popular candidates for non-baryonic dark matter. These include neutrinos, axions, neutralinos, WIMPZILLAs, etc. In the second part, I overview several observational techniques that can be employed to search for WIMPs (weakly interacting massive particles) as non-baryonic dark matter. Among these techniques, I discuss the direct detection of WIMP dark matter, and its indirect detection through high-energy neutrinos, gamma-rays, positrons, etc. | |
| dc.description | Lectures delivered at the NATO Advanced Study Institute "Frontiers of the Universe", 8-20 Sept 2003, Cargese, France; 50 pages, 28 figures | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0403064 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0403064 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/7463 | |
| dc.subject | Astrophysics | |
| dc.title | Introduction to Non-Baryonic Dark Matter | |
| dc.type | text |