2017/04/30 by Chia-Feng Chang, Xiao-Gang He, Jusak Tandean · 20 citations
Mathematics · Physics and Astronomy · #Boson #Computer science #Cosmology and Gravitation Theories #Dark Matter and Cosmic Phenomena #Database #Geometry #Higgs boson #Large Hadron Collider #Mathematics #Nuclear physics #Parameter space #Particle physics #Particle physics theoretical and experimental studies #Physics #Pseudoscalar #Quark #Scalar (mathematics) #Spin (aerodynamics) #Statistics #Thermodynamics #hep-ex #hep-ph
paper · pdf · doi:10.1103/physrevd.96.075026
published in Physical review. D/Physical review. D. 96(7) (American Physical Society) · 13 pages, 3 figures, somewhat expanded, references added, matches publication
openalex created_date 2017/04/28 · openalex publication_date 2017/10/18 · arxiv created 2017/11/30 · arxiv updated 2017/12/01 · openalex updated_date 2026/08/05
We study an economical model of weakly interacting massive particle dark matter (DM) which has spin 3/2 and interacts with the 125 GeV Higgs boson via effective scalar and pseudoscalar operators. We apply constraints on the model from the relic density data, LHC measurements of the Higgs boson, and direct and indirect searches for DM, taking into account the effective nature of the DM-Higgs couplings. We show that this DM is currently viable in most of the mass region from about 58 GeV to 2.3 TeV and will be probed more stringently by ongoing and upcoming experiments. Nevertheless, the presence of the DM-Higgs pseudoscalar coupling could make parts of the model parameter space elusive from future tests. We find that important aspects of this scenario are quite similar to those of its more popular spin-1/2 counterpart.