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http://dspace.mediu.edu.my:8181/xmlui/handle/10261/3596Full metadata record
| DC Field | Value | Language |
|---|---|---|
| dc.creator | Bernal, Nicolás | - |
| dc.creator | Goudelis, A. | - |
| dc.creator | Mambrini, Yann | - |
| dc.creator | Muñoz, Carlos | - |
| dc.date | 2008-04-15T16:18:07Z | - |
| dc.date | 2008-04-15T16:18:07Z | - |
| dc.date | 2008-04-14 | - |
| dc.date.accessioned | 2017-01-31T01:02:22Z | - |
| dc.date.available | 2017-01-31T01:02:22Z | - |
| dc.identifier | arXiv:0804.1976v1 | - |
| dc.identifier | http://hdl.handle.net/10261/3596 | - |
| dc.identifier.uri | http://dspace.mediu.edu.my:8181/xmlui/handle/10261/3596 | - |
| dc.description | 26 pages, 14 figures. | - |
| 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 $m_{\chi} \lesssim 50$ 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 $\sigma_{\chi-p} \lesssim 10^{-8}$ 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 | The authors would like to thank the ENTApP Network of the ILIAS project RII3-CT-2004-506222 and he French ANR project PHYS@COL&COS for financial support. Y.M. would like to thank financial support via the "Marie Curie Host Fellowship for Transfer of Knowledge", MTKD-CT-2005-029466. The work of A. G. is sponsored by the hepTOOLS Research Training Network MRTN-CT-2006-035505. The work of C. M. was supported in part by the Spanish DGI of the MEC under Proyectos Nacionales FPA2006-01105 and FPA2006-05423, by the European Union under the RTN programs MRTN-CT-2004-503369 and UniverseNet MRTN-CT-2006-035863, and by the Comunidad de Madrid under Proyecto HEPHACOS S-0505/ESP-0346. | - |
| dc.description | Peer reviewed | - |
| dc.format | 384963 bytes | - |
| dc.format | application/pdf | - |
| dc.language | eng | - |
| dc.relation | Preprint | - |
| dc.rights | openAccess | - |
| dc.subject | Dark matter | - |
| dc.subject | WIMP mass | - |
| dc.subject | XENON Experiment | - |
| dc.subject | GLAST Experiment | - |
| dc.title | Determining the WIMP mass using the complementarity between direct and indirect searches and the ILC | - |
| dc.type | Pre-print | - |
| Appears in Collections: | Digital Csic | |
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