Dark matter produced by the freeze-out of inverse decays has a full phase structure, with couplings as small as m_chi over the Planck mass, that is robust to kinetic decoupling and testable through dark photon searches.
(12) and (27) dominate the relic abundance
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Phases of Dark Matter from Inverse Decays
Dark matter produced by the freeze-out of inverse decays has a full phase structure, with couplings as small as m_chi over the Planck mass, that is robust to kinetic decoupling and testable through dark photon searches.