General Dark Matter-Electron Interactions
In conventional dark matter direct detection experiments, the desired signals are rare collisions between dark matter (DM) particles from the galactic halo and nuclei in a target, e.g. in liquid xenon or in crystals. However, if the mass of the hypothetical DM particle falls below about 1 GeV (roughly the mass of the proton), a scenario called sub-GeV DM, these collisions deposit only very little energy in the detector. For most experiments, this means that they cannot detect sub-GeV DM.
Many ideas have been proposed to extend detection sensitivity to sub-GeV masses. The most studied strategy is to look for collisions between DM particles and electrons instead of nuclei. Experiments such as SENSEI have probed DM down to 1 MeV (roughtly twice the mass of an electron).
On the theoretical side, collisions between DM and electrons are much harder to describe than nuclear recoils. The reason for this is the fact that electrons are not sitting still but are bound in atoms with discrete energy levels. Incoming DM particles might induce transitions between these energy levels leading to either electron excitation or ionization, which in turn could trigger a detector.
Our project focusses on the theoretical modelling of the DM-electron interaction. In the literature, one typically assumes a specific model to make predictions for DM-electron scatterings in detectors. We chose another way and formulated an effective model-independent framework, which can be mapped to many different DM models. Using this general description of DM-electron interactions, we find four atomic responses to general DM-electron interactions, only one of which was known before.
This could have wide implications, even for condensed matter physics. If DM gets discovered in the (hopefully not too far) future, and it turns out to interact with electrons via non-standard interactions, DM could serve as a probe to test new material properties. Hidden properties that could not be probed via the electromagnetic interaction.