Gravitational-wave detectors and quantum noise
The ultimate sensitivity of a gravitational-wave detector is set, in the end, by quantum noise. How far can that limit be pushed down? I work on this through the optical spring and through the methods of quantum measurement.
gravitational-wave detectorstandard quantum limitoptical springdetuned cavityback-action evasion
Macroscopic quantum mechanics
Quantum noise is not only noise; it is also a signal. I turn the precision-measurement techniques built for gravitational-wave detectors onto milligram-scale mirrors, and ask how far an object of that size still obeys quantum mechanics.
milligram oscillatorquantum radiation pressure noiseoptical trapping
Atom interferometry
Using matter waves instead of light gives a larger signal. To push the sensitivity of an atom interferometer I work on a phase-modulation readout scheme and analyze the limit it sets, and on applying it to gyroscopes that measure rotation.
atom interferometerphase-modulation readoutinertial sensing
Dark matter searches with precision measurement
An interferometer sensitive enough for gravitational waves will register other things too. With optical cavities and levitated nanoparticles I look for traces of dark matter that no experiment has caught so far.
axionvector dark matterlevitated nanoparticle