المستودع الأكاديمي جامعة المدينة

Determining the WIMP mass using the complementarity between direct and indirect searches and the ILC

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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


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