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Closing in on supersymmetric electroweak baryogenesis with dark matter searches and the Large Hadron Collider

2011/08/31 by Jonathan Kozaczuk, Stefano Profumo · 17 citations
Physics and Astronomy · #Astrophysics #Baryogenesis #Chargino #Cosmology #Cosmology and Gravitation Theories #Dark Matter and Cosmic Phenomena #Dark energy #Dark matter #Electroweak interaction #Gaugino #Higgsino #Large Hadron Collider #Lightest Supersymmetric Particle #Minimal Supersymmetric Standard Model #Neutralino #Particle physics #Particle physics theoretical and experimental studies #Physics #Scalar field dark matter #Supersymmetry #Weakly interacting massive particles #astro-ph.CO #hep-ph

paper · pdf · doi:10.1088/1475-7516/2011/11/031

published in Journal of Cosmology and Astroparticle Physics 2011(11), 031 (Institute of Physics) · 29 pages, 8 figures; v2: discussion and figure added to match version published in JCAP

arxiv created 2011/11/16 · openalex publication_date 2011/11/16 · arxiv updated 2011/11/18 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05

Abstract

We study the impact of recent direct and indirect searches for particle dark matter on supersymmetric models with resonant neutralino- or chargino-driven electroweak baryogenesis (EWB) and heavy sfermions. We outline regions of successful EWB on the planes defined by gaugino and higgsino mass parameters, and calculate the portions of those planes excluded by dark matter search results, and the regions soon to be probed by current and future experiments. We conclude that dark matter searches robustly exclude a wino-like lightest supersymmetric particle in successful EWB regions. Bino-like dark matter is still a possibility, although one that will be probed with a modest improvement in the sensitivity of current direct and indirect detection experiments. We also calculate the total production cross section of chargino and neutralino pairs at the Large Hadron Collider, with a center of mass energy of 7 and 14 TeV.

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