Dark Matter from Supersymmetric Grand Unification

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dc.creatorKane, G. L.
dc.creatorKolda, Chris
dc.creatorRoszkowski, Leszek
dc.creatorWells, James D.
dc.date1994-05-23
dc.date1994-05-24
dc.date.accessioned2026-07-07T08:59:57Z
dc.date.available2026-07-07T08:59:57Z
dc.descriptionIn constrained minimal supersymmetry the lightest neutralino of bino-type is the only neutral candidate for dark matter. As a result, one is typically able to restrict all the supersymmetric mass spectra below roughly 1-2\tev\ {\em without} imposing an ill-defined fine-tuning constraint.
dc.descriptioninvited talk given by LR at the Astrophysics Symposium and Workshop on Dark Matter ``Critique of the Sources of Dark Matter in the Universe'', Los Angeles, California, February 16--18, 1994; 14 pages of text in Latex plus 4 figures in PS (3 included, 1 available by email); University of Michigan preprint UM-TH-94-17 (April 1994). CHANGES: 3 figures added, abstract in the listing corrected
dc.identifierhttps://arxiv.org/abs/hep-ph/9405363
dc.identifierhttp://arxiv.org/abs/hep-ph/9405363
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/147904
dc.subjectHigh Energy Physics - Phenomenology
dc.subjectAstrophysics
dc.titleDark Matter from Supersymmetric Grand Unification
dc.typetext

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