Implications of Recent Nucleon Spin Structure Measurements for Neutralino Dark Matter Detection

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dc.creatorKamionkowski, Marc
dc.creatorKrauss, Lawrence M.
dc.creatorRessell, M. Ted
dc.date1994-02-25
dc.date1994-06-22
dc.date.accessioned2026-07-07T08:59:55Z
dc.date.available2026-07-07T08:59:55Z
dc.descriptionPredicted rates for direct and indirect detection of dark-matter neutralinos depend in general on the spin content of the nucleon. Neutralinos that are predominantly $B$-ino are the likeliest candidates for detection via spin-dependent interactions. Uncertainties in the measured spin content of the nucleon may lead to dramatic uncertainties in the rates for detection of $B$-inos by scattering off of nuclei with unpaired neutrons. Rates for spin-dependent scattering of $B$-inos off of nuclei with unpaired protons are far more robust, as are rates for capture of $B$-inos in the Sun.
dc.description7 pages, TeX, Harvmac required, CWRU-P3-94, IASSNS-HEP-94/14, UCRL-JC-116940, revised to include updated data and analysis
dc.identifierhttps://arxiv.org/abs/hep-ph/9402353
dc.identifierhttp://arxiv.org/abs/hep-ph/9402353
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/147889
dc.subjectHigh Energy Physics - Phenomenology
dc.subjectAstrophysics
dc.subjectNuclear Theory
dc.titleImplications of Recent Nucleon Spin Structure Measurements for Neutralino Dark Matter Detection
dc.typetext

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