Recasting direct detection limits within micrOMEGAs and implication for non-standard dark matter scenarios

Abstract Direct detection experiments obtain 90% upper limits on the elastic scattering cross sections of dark matter with nucleons assuming point-like interactions and standard astrophysical cosmological parameters. In this paper we provide a recasting from XENON1T, PICO-60, CRESST-III DarkSide-50 include them in micrOMEGAs. The code can then be used to directly impose constraints these generic models under different assumptions about DM velocity distribution or nucleus form factors. Moreover, new obtained presence light t-channel mediator millicharged particles.