WIMP Velocity Impact on Direct Dark Matter Searches

dc.creatorBrhlik, Michal
dc.creatorRoszkowski, Leszek
dc.date1999-03-24
dc.date.accessioned2026-07-07T10:33:50Z
dc.date.available2026-07-07T10:33:50Z
dc.descriptionWe examine the effect of some uncertainties in the input astrophysical parameters on direct detection searches for WIMPs in the Galactic halo. We concentrate on the possible WIMP annual modulation signal recently reported by the DAMA Collaboration. We find that allowing for a reasonable uncertainty in a WIMP Maxwellian velocity distribution leads to significantly relaxed constraints on the WIMP mass as compared to the original DAMA analysis.
dc.description11 pages, 3 eps figures
dc.identifierhttps://arxiv.org/abs/hep-ph/9903468
dc.identifierhttp://arxiv.org/abs/hep-ph/9903468
dc.identifierPhys.Lett.B464:303-310,1999
dc.identifierdoi:10.1016/S0370-2693(99)01048-5
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/179261
dc.subjectHigh Energy Physics - Phenomenology
dc.subjectAstrophysics
dc.titleWIMP Velocity Impact on Direct Dark Matter Searches
dc.typetext

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