Direct Dark Matter Detection

Millenium Dark Matter Simulation

Dark matter is all around us

Dark matter dominates structure formation in the Universe. Our galaxy is in the middle of a huge dark matter halo, indeed it would not have formed without it. Thus we might be able to establish the prescence of the dark matter particles zooming through our laboratory (and going through the Earth) by detecting the rare interactions between them and our target in a sensitive low-background experiment. Dark matter particle searches that look for these type of detectable interactions are called Direct Detection Experiments.

Direct Detection is a very well motivated dark matter search strategy, as interactions between DM and standard model particles arrise naturally from many supersymmetric theories which predict that the lightest supersymmetric particle (LSP) is stable. Other models such as assymetric dark matter or hidden sector models also predict the possibility of this interaction. If the dark matter cross section to the standard model is sufficiently high, direct detection in the laboratory is possible.

Direct detection requirements

Dark matter can ineract with our detectors through a nuclear recoil or an electron recoil. Integrating the differential recoil spectrum of most models we find that the expected rate in a dark matter detector is less than one event per kg of detector per year. Backgrounds in a normal laboratory are millions of times higher. Thus, we operate our detectors far underground to shield from cosmic rays, and use extensive shielding around our detector to shield from the radioactivity in the laboratory. Furthermore, the purity of the materials used for the detector, its housing, any nearby electronics, etc. must be very tightly controlled.

Since the vast majority of backgrounds are photons and electrons and thus produce electron recoils, a dark matter detector than can discriminate between electron and nuclear recoils will have better background control. A massive target is clearly preffered. Lower energy thresholds will increase the sensitivity of the experiment to lighter dark matter candidates, since the recoil spectrum gets steeper with lower dark matter mass.

In summary, when designing a dark matter direct detection experiment, the requirements are:

  1. Low background rate
  2. Large exposure (mass × time)
  3. Low energy threshold
  4. Discrimination between signal and backgrounds

Next: Indirect Detection