Astrophysical search strategies for accelerator blind dark matter
| dc.creator | Wells, James D. | |
| dc.date | 1998-08-06 | |
| dc.date.accessioned | 2026-07-07T02:27:34Z | |
| dc.date.available | 2026-07-07T02:27:34Z | |
| dc.description | A weakly interacting dark-matter particle may be difficult to discover at an accelerator because it either (1) is too massive, (2) has no standard-model gauge interactions, or (3) is almost degenerate with other states. In each of these cases, searches for annihilation products in the Galactic halo are useful probes of dark-matter properties. Using the example of supersymmetric dark matter, I discuss how astrophysical searches for dark matter may provide discovery and mass information inaccessible to collider physics programs such as the Tevatron and LHC. | |
| dc.description | 4 pages, Talk given at 3rd International Symposium on Sources and Detection of Dark Matter in the Universe (DM 98), Santa Monica, CA, 18-20 Feb 1998 | |
| dc.identifier | https://arxiv.org/abs/astro-ph/9808052 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/9808052 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/12745 | |
| dc.subject | Astrophysics | |
| dc.title | Astrophysical search strategies for accelerator blind dark matter | |
| dc.type | text |