Sommerfeld Enhancement in Spin-1 Electroweak Dark Matter
This paper investigates a renormalizable spin-1 electroweak dark matter model where Sommerfeld enhancement and annihilation into heavy vector bosons allow for thermal relic abundances at masses between 3.6 and 9.2 TeV, a range distinct from lower-mass spin-0 or spin-1/2 scenarios, with the entire viable parameter space being testable by the Cherenkov Telescope Array Observatory via a characteristic double-peak gamma-ray signature.