Asymmetric Dark Matter May Not Be Light
  It is often said that asymmetric dark matter is light compared to typical
weakly interacting massive particles. Here we point out a simple scheme with a
neutrino portal and $\mathcal{O}(60 \text{ GeV})$ asymmetric dark matter which
may be ''added'' to any standard baryogenesis scenario. The dark sector
contains a copy of the Standard Model gauge group, as well as (at least) one
matter family, Higgs, and right-handed neutrino. After baryogenesis, some
lepton asymmetry is transferred to the dark sector through the neutrino portal
where dark sphalerons convert it into a dark baryon asymmetry. Dark hadrons
form asymmetric dark matter and may be directly detected due to the vector
portal. Surprisingly, even dark anti-neutrons may be directly detected if they
have a sizeable electric dipole moment. The dark photons visibly decay at
current and future experiments which probe complementary parameter space to
dark matter direct detection searches. Exotic Higgs decays are excellent
signals at future $e^+ e^-$ Higgs factories.
