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Preliminary simulation and optimization studies of the Directional DarkMatter Detector and the Directional Neutron Observer are presented. Thesestudies show that the neutron interaction with the gas-target in thesedetectors is treated correctly by GEANT4 and that by lowering the pressure, thesensitivity to low-mass WIMP candidates is increased. The use of negative iondrift might allow us to search the WIMP mass region suggested by the results ofthe non-directional experiments DAMA/LIBRA, CoGeNT and CRESST-II.

Simulation of the Directional Dark Matter Detector (D3) and Directional Neutron Observer (DiNO)