Scalar Co-SIMP dark matter: models and sensitivities

• Published in: The journal of high energy physics Vol. 2023; no. 8; pp. 91 - 36
• Main Authors: Parikh, Aditya, Smirnov, Juri, Xu, W. Linda, Zhou, Bei
• Format: Journal Article
• Language: English
• Published: Berlin/Heidelberg Springer Berlin Heidelberg 16-08-2023; Springer Nature B.V; Springer Nature; SpringerOpen
• Subjects: ASTRONOMY AND ASTROPHYSICS; Classical and Quantum Gravitation; Cosmology of Theories BSM; Dark matter; Decoupling; Early Universe Particle Physics; Elementary Particles; High energy physics; Mathematical models; Models for Dark Matter; Overheating; Parameter sensitivity; Particle Nature of Dark Matter; Phase transitions; Physics; Physics and Astronomy; PHYSICS OF ELEMENTARY PARTICLES AND FIELDS; Quantum Field Theories; Quantum Field Theory; Quantum Physics; Regular Article - Theoretical Physics; Relativity Theory; Scalars; Sensitivity; Standard model (particle physics); String Theory; Thermal analysis; Threshold detectors (dosimeters); Cosmology of Theories BSM; Particle Nature of Dark Matter; Models for Dark Matter; Early Universe Particle Physics
• ISSN: 1029-8479; 1126-6708; 1029-8479
• DOI: 10.1007/JHEP08(2023)091

A
bstract
In this work, we present UV completions of the recently proposed number-changing Co-SIMP freeze-out mechanism. In contrast to the standard cannibalistic-type dark matter picture that occurs entirely in the dark sector, the 3 → 2 process setting the relic abundance in this case requires one Standard Model particle in the initial and final states. This prevents the dark sector from overheating and leads to rich experimental signatures. We generate the Co-SIMP interaction with a dark sector consisting of two scalars, with the mediator coupling to either nucleons or electrons. In either case,
the dark matter candidate is naturally light
: nucleophilic interactions favor the sub-GeV mass range and leptophilic interactions favor the sub-MeV mass range. Viable thermal models in these lighter mass regimes are particularly intriguing to study at this time, as new developments in low-threshold detector technologies will begin probing this region of parameter space. While particles in the sub-MeV regime can potentially impact light element formation and CMB decoupling, we show that a late-time phase transition opens up large fractions of parameter space. These thermal light dark matter models can instead be tested with dedicated experiments. We discuss the viable parameter space in each scenario in light of the current sensitivity of various experimental probes and projected future reach.