Abstract
In this brief review of recent theoretical developments associated with the search for dark matter I describe the following: why baryons are now ruled out as dark matter candidates; SUSY WIMPS and signatures in the MSSM and NMSSM why claimed indirect signatures are probably not WIMP related, why axions may be of new interest, how WIMP detection might tell us about the galactic halo, and how theorists are preparing to avoid the next generation of experimental constraints. (Invited review talk, Neutrino 2006, Santa Fe 2006).
| Original language | English (US) |
|---|---|
| Title of host publication | NEUTRINO 2006 - Proceedings of the 22nd International Conference on Neutrino Physics and Astrophysics |
| Pages | 149-154 |
| Number of pages | 6 |
| State | Published - 2006 |
| Externally published | Yes |
| Event | 22nd International Conference on Neutrino Physics and Astrophysics, NEUTRINO 2006 - Santa Fe, NM, United States Duration: Jun 13 2006 → Jun 19 2006 |
Other
| Other | 22nd International Conference on Neutrino Physics and Astrophysics, NEUTRINO 2006 |
|---|---|
| Country/Territory | United States |
| City | Santa Fe, NM |
| Period | 6/13/06 → 6/19/06 |
ASJC Scopus subject areas
- Astronomy and Astrophysics