DETECTOR SENSITIVITYTo deal with the first issue of background signals, these detectors have been constructed deep underground using the Earth itself to provide a thick layer of shielding. This blocks out a significant proportion of ordinary particles whereas the potential DM particles, which are much less likely to interact with matter, can reach the detector.
The second issue of detector sensitivity is one with many innovative solutions. One of these is being explored as part of the
MIGDAL experiment at RAL. To understand it, the principle of a DM detector should first be explained. When a DM particle hits an atom in the detector’s tank it causes the atom’s nucleus to recoil which creates a signal, the strength of which depends on the mass of the DM particle.
There is a limit to how sensitive the detector is, namely, there is a threshold for the signal strength below which it won't be detected. If the DM particle has a low mass (<10 GeV) it will produce a signal below this experimental detection threshold. The Migdal effect would lower this threshold energy: when a nuclear recoil happens because the atom’s surrounding electron cloud will take some time to catch up with the nucleus, there is a small but distinct probability of one of those electrons getting excited and even ionised. This creates the possibility of a DM particle which is below the threshold energy to create a detectable signal but may be able to produce an electron via the Migdal effect. This would widen the range of the energy and mass of DM particles that could be detected.
The Neutron Irradiation Laboratory for Electronics (NILE) at ISIS is a new facility, which had already procured a DT generator (a desktop fusion device using deuterium and tritium to produce high-energy neutrons at 14.1 MeV) to use for testing the resilience of cosmic ray damage test and the effect of space weather on electronics, but they realised the DT generator would be ideally suited for testing the Migdal effect, in which a neutral particle scattering from a nucleus can produce atomic ionisation alongside the nuclear recoil. However, to probe the effect at the low nuclear recoil energies relevant to most dark matter scattering models (up to a few hundred keV) lower energy neutrons are needed from a DD generator (a fusion reactor using only deuterium as a fuel and producing 2.5MeV neutrons), provided in 2021 by UKRI’s World Class Laboratories funding. After installing the dark matter detector, in 2023 NILE was ready to receive its first neutrons, starting the hunt for dark matter.