When talking about dark matter (DM), there's a standard line that gets used from popular talks through to journal papers: we only know about its gravitational interactions. That is, we've measured its existence and abundance from how it affects galaxy rotation curves, or the structure of the cosmic microwave background; but we have no direct information about any
other types of coupling it might have to the ordinary stuff we are made of
1.
Of course, there are a lot of searches of various types looking for those interactions. One of the most basic is
direct detection, building a very sensitive and low-background experiment and looking for dark matter scattering off the atoms in your apparatus. It is here that one of the more enticing, puzzling and long-standing mysteries of dark matter is to be found; the fact that several experiments claim signals, that seem to be ruled out by other searches that found nothing
2.
My attention was drawn by the publication on the arXiv today of
another paper in the
signal column.