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Update on scalar singlet dark matter

2013/06/30 by James M. Cline, Kimmo Kainulainen, Pat Scott +1 · 599 citations
Physics and Astronomy · #Astrophysics #Cosmology #Cosmology and Gravitation Theories #Dark Matter and Cosmic Phenomena #Dark energy #Dark matter #Electroweak interaction #Higgs boson #Large Hadron Collider #Parameter space #Particle physics #Particle physics theoretical and experimental studies #Physics #Physics beyond the Standard Model #Scalar (mathematics) #Scalar field dark matter #Standard Model (mathematical formulation) #Statistics #astro-ph.CO #hep-ph

paper · pdf · doi:10.1103/physrevd.88.055025

published in Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields 88(5) (American Physical Society) · 18 pages, 10 figures. v2: small updates to references and discussion, including a brief passage on continuum gamma rays from the Galactic Centre; matches the version accepted for publication in PRD. v3: updated references to match final published version. v4: corrected CTA observing time, improved clarity of Fermi CL/p-value description. v5: corrected central value of coupling f_N

openalex publication_date 2013/09/27 · arxiv created 2015/08/05 · arxiv updated 2015/08/07 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05

Abstract

One of the simplest models of dark matter is where a scalar singlet field S comprises some or all of the dark matter and interacts with the standard model through an |H|2S2 coupling to the Higgs boson. We update the present limits on the model from LHC searches for invisible Higgs decays, the thermal relic density of S, and dark matter searches via indirect and direct detection. We point out that the currently allowed parameter space is on the verge of being significantly reduced with the next generation of experiments. We discuss the impact of such constraints on possible applications of scalar singlet dark matter, including a strong electroweak phase transition, and the question of vacuum stability of the Higgs potential at high scales.

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