2010/05/31 by Shinya Kanemura, Shigeki Matsumoto, Takehiro Nabeshima +1 · 6 citations
Physics and Astronomy · #Astrophysics #Cosmology #Cosmology and Gravitation Theories #Dark Matter and Cosmic Phenomena #Dark energy #Dark matter #Higgs boson #Large Hadron Collider #Light dark matter #Mixed dark matter #Particle physics #Particle physics theoretical and experimental studies #Physics #Physics beyond the Standard Model #Scalar field dark matter #WIMP #Warm dark matter #Weakly interacting massive particles #hep-ph
paper · pdf · doi:10.1103/physrevd.82.055026
published as Phys.Rev.D82:055026,2010 · 14 pages, 10 figures
arxiv created 2010/05/31 · openalex publication_date 2010/09/29 · arxiv updated 2014/11/21 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05
Even if new physics beyond the standard model indeed exists, the energy scale of new physics might be beyond the reach at the Large Hadron Collider (LHC), and the LHC could find only the Higgs boson but nothing else. This is the so-called ``nightmare scenario.'' On the other hand, the existence of the dark matter has been established from various observations. One of the promising candidates for thermal relic dark matter is a stable and electric charge-neutral weakly interacting massive particle (WIMP) with mass below the TeV scale. In the nightmare scenario, we introduce a WIMP dark matter singlet under the standard model gauge group, which only couples to the Higgs doublet at the lowest order, and investigate the possibility that such WIMP dark matter can be a clue to overcome the nightmare scenario via various phenomenological tests such as the dark matter relic abundance, the direct detection experiments for the dark matter particle, and the production of the dark matter particle at the LHC.