Probing Dark Matter in the Economical 3-3-1 Model

2011/10/07 by D. T. Huong, Huong, D. T., C. S. Kim +6
Mathematics · Physics and Astronomy · #CMB cold spot #Cosmic microwave background #Cosmology and Gravitation Theories #Dark Matter and Cosmic Phenomena #Dark matter #FOS: Physical sciences #High Energy Physics - Phenomenology (hep-ph) #Mathematics #MicroMegas detector #Parameter space #Particle physics #Particle physics theoretical and experimental studies #Physics #Quantum mechanics #Range (aeronautics) #Scalar (mathematics) #Statistics #hep-ph

paper · pdf · doi:10.48550/arxiv.1110.1482

The order of references corrected. Manuscript text slightly modified

openalex publication_date 2011/10/07 · arxiv created 2011/10/13 · arxiv updated 2011/10/14 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28

Abstract

We show that the economical 3-3-1 model has a dark mater candidate. It is a real scalar H₁⁰ in which main part is bilepton (with lepton number 2) and its mass is in the range of some TeVs. We calculate the relic abundance of H₁⁰ dark matter by using micrOMEGAs 2.4 and figure out parameter space satisfying the WMAP constraints. Direct and indirect searches are studied for a special choice of parameters in the WMAP - allowed region.

Citations

• Dark Matter in the Simplest Little Higgs Model
• CalcHEP 2.3: MSSM, structure functions, event generation, batchs, and generation of matrix elements for other packages

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