Neutralino Relic Density in the CPVMSSM at the ILC
| dc.creator | Belanger, G. | |
| dc.creator | Kittel, O. | |
| dc.creator | Kraml, S. | |
| dc.creator | Martyn, H. U. | |
| dc.creator | Pukhov, A. | |
| dc.date | 2009-01-30 | |
| dc.date.accessioned | 2026-07-07T12:36:27Z | |
| dc.date.available | 2026-07-07T12:36:27Z | |
| dc.description | We discuss ILC measurements for a specific MSSM scenario with CP phases, where the lightest neutralino, a candidate for dark matter, annihilates through t-channel exchange of light staus. These prospective ILC measurements are used to fit the underlying model parameters. A collider prediction of the relic density of the neutralino from this fit gives 0.116<Omega h2<0.19 at 95%CL. | |
| dc.description | 4 pages, 2 figures, Proceedings of LCWS08, chicago | |
| dc.identifier | https://arxiv.org/abs/0901.4838 | |
| dc.identifier | http://arxiv.org/abs/0901.4838 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/218098 | |
| dc.subject | High Energy Physics - Phenomenology | |
| dc.title | Neutralino Relic Density in the CPVMSSM at the ILC | |
| dc.type | text |