Determining the WIMP mass using the complementarity between direct and indirect searches and the ILC
| dc.creator | Bernal, N. | |
| dc.creator | Goudelis, A. | |
| dc.creator | Mambrini, Y. | |
| dc.creator | Munoz, C. | |
| dc.date | 2008-04-14 | |
| dc.date | 2009-01-06 | |
| dc.date.accessioned | 2026-07-07T12:38:35Z | |
| dc.date.available | 2026-07-07T12:38:35Z | |
| dc.description | We study the possibility of identifying dark matter properties from XENON-like 100 kg experiments and the GLAST satellite mission. We show that whereas direct detection experiments will probe efficiently light WIMPs, given a positive detection (at the 10% level for $m_χ \lesssim 50$ GeV), GLAST will be able to confirm and even increase the precision in the case of a NFW profile, for a WIMP-nucleon cross-section $σ_{χ-p} \lesssim 10^{-8}$ pb. We also predict the rate of production of a WIMP in the next generation of colliders (ILC), and compare their sensitivity to the WIMP mass with the XENON and GLAST projects. | |
| dc.description | 32 pages, new figures and a more detailed statistical analysis. Final version to appear in JCAP | |
| dc.identifier | https://arxiv.org/abs/0804.1976 | |
| dc.identifier | http://arxiv.org/abs/0804.1976 | |
| dc.identifier | JCAP 0901:046,2009 | |
| dc.identifier | doi:10.1088/1475-7516/2009/01/046 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/218811 | |
| dc.subject | High Energy Physics - Phenomenology | |
| dc.subject | Astrophysics | |
| dc.title | Determining the WIMP mass using the complementarity between direct and indirect searches and the ILC | |
| dc.type | text |