Animations showing the relative change in the Dark Matter (DM) direct detection rate, caused by DM particles scattering in the Earth. The maps are equal-area Mollweide projections of the whole Earth.
We assume a CRESST-II-like detector in calculating the rate and we consider 3 different DM-nucleon interactions from the NREFT of arXiv:1203.3542: O1, O8 and O12.
In all cases, the DM mass is 0.5 GeV, with DM-nucleon interaction strength set to give a 10% average scattering probability. This part of the parameter space is not currently excluded (as of 17/11/2016).
Files suffixed with 'noD' include only the effects of attenuation and not deflection. The remaining files include both attenuation and deflection.