Aspects of Neutralino Dark Matter
| dc.creator | Yuan, Kajia | |
| dc.date | 1993-09-01 | |
| dc.date.accessioned | 2026-07-07T03:56:22Z | |
| dc.date.available | 2026-07-07T03:56:22Z | |
| dc.description | The possible solution of dark matter problem with neutralinos of supersymmetric models within the supergravity framework is reviewed. A novel correlation between the neutralino relic abundance $Ω_χ$ and the soft supersymmetry breaking patterns is demonstrated. It is explained that, this generic result together with the proton-decay constraint could significantly reduce the allowed parameter space of the minimal $SU(5)$ supergravity model, and therefore makes this model more easily testable. The prospect of obtaining further cosmological constraints from underground experiments for the minimal $SU(5)$ supergravity model is also briefly discussed. | |
| dc.description | 15pp Latex text + 6 ps figs (included as a uuencoded file, also available upon request), CTP-TAMU-51/93 and ACT-19/93 | |
| dc.identifier | https://arxiv.org/abs/hep-ph/9308377 | |
| dc.identifier | http://arxiv.org/abs/hep-ph/9308377 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/44944 | |
| dc.subject | High Energy Physics - Phenomenology | |
| dc.subject | Astrophysics | |
| dc.title | Aspects of Neutralino Dark Matter | |
| dc.type | text |