A Global Analysis of Resonance-enhanced Light Scalar Dark Matter
arXiv:2205.10149 · doi:10.1007/JHEP01(2023)106
Abstract
We study a minimal model for a light scalar dark matter, requiring a light scalar mediator to address the core-cusp problem and interact with the standard model particles. We analyze the model comprehensively by focusing on the Breit-Wigner resonance for dark matter annihilation and self-scattering channels, considering the thermal relic abundance condition that includes the early kinetic decoupling effect, as well as the present and future constraints from collider, direct, and indirect dark matter detections. We found that the scalar dark matter with the mass of 0.3-2 GeV remains uncharted, which will be efficiently tested by the near future MeV gamma-ray observations.
30 pages, 8 figures
References in corpus (11)
- The Local Dark Matter Density
- On the local dark matter density
- A taste of dark matter: Flavour constraints on pseudoscalar mediators
- A new determination of the local dark matter density from the kinematics of K dwarfs
- Precise WIMP Dark Matter Abundance and Standard Model Thermodynamics
- Joint CMB and BBN Constraints on Light Dark Sectors with Dark Radiation
- Resonance enhancement of dark matter interactions: the case for early kinetic decoupling and velocity dependent resonance width
- Linear Sigma Dark Matter
- Forbidden Scalar Dark Matter and Dark Higgses
- Is light thermal scalar dark matter possible?
- The search for Light Dark Matter with NEWS-G
Cited by in corpus (5)
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- Light Thermal Self-Interacting Dark Matter in the Shadow of Non-Standard Cosmology