Speaker
Description
Precision gravitational wave measurement transforms research beyond general relativity and cosmology. Advances are made by applying quantum enhanced interferometry into the LIGO, Virgo and KAGRA detectors. Here, we develop an atomic sensor that employs a p-orbital Bose-Einstein condensate in an optical lattice to project gravitational wave signals into an orbital squeezed state. This entangled state couples linearly to the spacetime distortion signals received via a Michelson interferometer. Simulation data show that this sensor improves sensitivity over LIGO's quantum noise by approximately one order of magnitude and detection volume by ∼1E3 in key frequency regimes. Additionally, it reduces the required laser power by five orders of magnitude. These results suggest that atomic orbital squeezing offers a compelling alternative to conventional techniques, offering a qualitatively different avenue for gravitational wave-based detection of dark matter, black holes, and the equation of state in neutron stars.
