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Neutralino dark matter in supersymmetric models with non--universal scalar mass terms

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arxiv hep-ph/9508249 v1 pith:WCODRRS5 submitted 1995-08-07 hep-ph astro-ph

V. Berezinsky , A. Bottino , J. Ellis , N. Fornengo , G. Mignola , S. Scopel This is my paper · ORCID
classification hep-phastro-ph
keywords neutralinodarkmassmatterrelicscalarsupersymmetricterms
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Neutralino dark matter is studied in the context of a supergravity scheme where the scalar mass terms are not constrained by universality conditions at the grand unification scale. We analyse in detail the consequences of the relaxation of this universality assumption on the supersymmetric parameter space, on the neutralino relic abundance and on the event rate for the direct detection of relic neutralinos.

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Cited by 1 Pith paper

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  1. A pilot sample of Planck-selected strongly lensed sub-mm galaxies: NOEMA observations and physical characterisation

    astro-ph.GA 2026-07 conditional novelty 5.0 of 10

    Four Planck-selected dusty star-forming galaxies are confirmed as strongly lensed at z≈2.3–3.3 via NOEMA CO line detections; a lens model for one source yields µ≈11.

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