Probing the supersymmetric parameter space by WIMP direct detection

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dc.creatorBottino, A.
dc.creatorDonato, F.
dc.creatorFornengo, N.
dc.creatorScopel, S.
dc.date2000-10-18
dc.date2001-04-10
dc.date.accessioned2026-07-07T10:32:45Z
dc.date.available2026-07-07T10:32:45Z
dc.descriptionWe discuss to which extent the present experiments of direct search for WIMPs, when interpreted in terms of relic neutralinos, probe interesting regions of the supersymmetric parameter space, which are also being progressively explored at accelerators. Our analysis is performed in a number of different supersymmetric schemes. We derive the relevant neutralino cosmological properties, locally and on the average in the universe. We prove that part of the susy configurations probed by current WIMP experiments entail relic neutralinos of cosmological interest. The main astrophysical and particle physics uncertainties, relevant for a proper comparison between theory and experimental data, are stressed and taken into account.
dc.description23 pages, 5 figures, typeset with ReVTeX. Updated to match version accepted for publication in PRD. The version on the archive has low resolution figures. The paper with high-resolution figures can be found at http://www.to.infn.it/~fornengo/papers/probing.ps.gz
dc.identifierhttps://arxiv.org/abs/hep-ph/0010203
dc.identifierhttp://arxiv.org/abs/hep-ph/0010203
dc.identifierPhys.Rev.D63:125003,2001
dc.identifierdoi:10.1103/PhysRevD.63.125003
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/178860
dc.subjectHigh Energy Physics - Phenomenology
dc.subjectAstrophysics
dc.titleProbing the supersymmetric parameter space by WIMP direct detection
dc.typetext

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