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Higgsino dark matter in a supergravity model with nonuniversal gaugino masses

2003/04/30 by Utpal Chattopadhyay, D. P. Roy · 10 citations
Physics and Astronomy · #Astrophysics #Cold dark matter #Cosmology #Cosmology and Gravitation Theories #Dark Matter and Cosmic Phenomena #Dark energy #Dark matter #Gaugino #Higgsino #Hot dark matter #Lightest Supersymmetric Particle #Neutralino #Particle physics #Particle physics theoretical and experimental studies #Physics #Supergravity #Supersymmetry #Warm dark matter #hep-ph

paper · pdf · doi:10.1103/physrevd.68.033010

published as Phys.Rev. D68 (2003) 033010 · Version to appear in Phys. Rev. D. A few references added in the bibliography and a comment added in Section 2. LaTex, 16 pages, 4 figures

arxiv created 2003/06/20 · openalex publication_date 2003/08/14 · arxiv updated 2009/11/30 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05

Abstract

We study a specific SUGRA model with nonuniversal gaugino masses as an alternative to the minimal SUGRA model in the context of supersymmetric dark matter. The lightest supersymmetric particle in this model turns out to be a Higgsino-dominated instead of a B-ino-dominated lightest neutralino. The thermal relic density of this Higgsino dark matter is somewhat lower than the cosmologically favored range, which means that it may be only a subdominant component of cold dark matter. Nonetheless, it predicts favorable rates of indirect detection, which can be seen in square-km-size neutrino telescopes.

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