Annual Modulation Signature for the Direct Detection of Milky Way Wimps and Supergravity Models

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dc.creatorArnowitt, R.
dc.creatorNath, Pran
dc.date1999-02-03
dc.date.accessioned2026-07-07T11:47:52Z
dc.date.available2026-07-07T11:47:52Z
dc.descriptionAn analysis is given of the annual modulation signal for the direct detection of relic neutralinos within the framework of supergravity unified models. It is shown that both the minimal and the non-minimal SUGRA models can generate neutralino-proton cross-sections at the level compatible with the signals reported in the DAMA experiment at the Gran Sasso National Laboratory. Effects of proton stability on the analysis of the DAMA data in the minimal and the non-minimal SUGRA models are also discussed.
dc.description14 pages, 5 figures
dc.identifierhttps://arxiv.org/abs/hep-ph/9902237
dc.identifierhttp://arxiv.org/abs/hep-ph/9902237
dc.identifierPhys.Rev.D60:044002,1999
dc.identifierdoi:10.1103/PhysRevD.60.044002
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/202725
dc.subjectHigh Energy Physics - Phenomenology
dc.subjectAstrophysics
dc.titleAnnual Modulation Signature for the Direct Detection of Milky Way Wimps and Supergravity Models
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