“…Especially in space missions with limited optical power, the beam waist, and consequently the ensemble size, needs to be kept small in order to reach sufficiently high Rabi frequencies. Moreover, beam splitters based on Bragg diffraction [13,[95][96][97] and Bloch oscillations [98,99] feature relatively long interrogation times, resulting in a sharp velocity acceptance such that the velocity width of the atomic distribution typically needs to be much smaller than the recoil velocity [100], equivalent to a few tens of nK. With DKC, these requirements are readily met as described in the previous sections of this paper as well as implemented in various experiments [45,[101][102][103][104].…”