  The GAPS experiment is designed to carry out a sensitive dark matter search
by measuring low-energy cosmic ray antideuterons and antiprotons. GAPS will
provide a new avenue to access a wide range of dark matter models and masses
that is complementary to direct detection techniques, collider experiments and
other indirect detection techniques. Well-motivated theories beyond the
Standard Model contain viable dark matter candidates which could lead to a
detectable signal of antideuterons resulting from the annihilation or decay of
dark matter particles. The dark matter contribution to the antideuteron flux is
believed to be especially large at low energies (E < 1 GeV), where the
predicted flux from conventional astrophysical sources (i.e. from secondary
interactions of cosmic rays) is very low. The GAPS low-energy antiproton search
will provide stringent constraints on less than 10 GeV dark matter, will
provide the best limits on primordial black hole evaporation on Galactic length
scales, and will explore new discovery space in cosmic ray physics.
  Unlike other antimatter search experiments such as BESS and AMS that use
magnetic spectrometers, GAPS detects antideuterons and antiprotons using an
exotic atom technique. This technique, and its unique event topology, will give
GAPS a nearly background-free detection capability that is critical in a
rare-event search. GAPS is designed to carry out its science program using
long-duration balloon flights in Antarctica. A prototype instrument was
successfully flown from Taiki, Japan in 2012. GAPS has now been approved by
NASA to proceed towards the full science instrument, with the possibility of a
first long-duration balloon flight in late 2020. Here we motivate low-energy
cosmic ray antimatter searches and discuss the current status of the GAPS
experiment and the design of the payload.
