An introduction to atom interferometry
Atom interferometry is the technique that underlies most of our precision measurements. We exploit the fact that matter, like light, exhibits wave-like properties. Atoms, unlike light, are massive and bear gravitational signals in their interference patterns. To understand atom interferometry, we first must understand optical interferometry.
In optical interferometry, light waves are recombined after propagating along separate paths. Depending on the difference in the waves' phase accumulated along the two paths, the light may interfere constructively and appear bright or it may interfere destructively and appear dark.
In atom interferometry, we start with clouds of atoms laser-cooled to millionths of a degree above absolute zero. With pulses of light, we drive the atoms into quantum superpositions of having been kicked with the momentum of photons and not having been kicked. The atoms, in two places at one time, are in a superposition of recoiling backwards or staying still. By manipulating the state of the atoms using one of two types of such light pulses, termed Bragg and Raman transitions (see Figures 2 and 3), we steer the matter waves' paths and recombine the matter waves at the end of the experiment. The atoms' trajectories are shown in Figure 1. The interference signal manifests as a population difference between final momentum states.
The energy and couplings along the atoms' path and their interaction the light pulses serve to determine the phase shift between matter waves at the output of the interferometer. Any effect that modifies the potential energy, internal energy, or kinetic energy across the two arms of the interferometer appears in the interferometer phase.
Atom interferometers are used to measure gravitational acceleration, gravity gradients, accelerations, rotations, fundamental constants such as the gravitational constant and the fine structure constant, and can be used to measure or constrain new physics that couples to matter.