Paleo-detectors: Searching for Dark Matter with Ancient Minerals
  We explore paleo-detectors as an approach to the direct detection of Weakly
Interacting Massive Particle (WIMP) dark matter radically different from
conventional detectors. Instead of instrumenting a (large) target mass in a
laboratory in order to observe WIMP-induced nuclear recoils in real time, the
approach is to examine ancient minerals for traces of WIMP-nucleus interactions
recorded over timescales as large as 1 Gyr. Here, we discuss the paleo-detector
proposal in detail, including background sources and possible target materials.
In order to suppress backgrounds induced by radioactive contaminants such as
uranium, we propose to use minerals found in marine evaporites or in
ultra-basic rocks. We estimate the sensitivity of paleo-detectors to
spin-independent and spin-dependent WIMP-nucleus interactions. The sensitivity
to low-mass WIMPs with masses $m_\chi \lesssim 10$ GeV extends to WIMP-nucleon
cross sections many orders of magnitude smaller than current upper limits. For
heavier WIMPs with masses $m_\chi \gtrsim 30$ GeV cross sections a factor of a
few to $\sim 100$ smaller than current upper limits can be probed by
paleo-detectors.
