Technical limitations to homodyne detection at audio frequencies.
Homodyne detection relies on the beat between a relatively strong local oscillator (LO) field at the carrier frequency and a signal beam with sidebands centered around the carrier frequency. This type of signal detection, or signal readout, is widely used in quantum optics applications and is expected to be used in advanced interferometric gravitational wave detectors. We investigate experimentally the limitations to making such measurements in a laboratory environment at audio frequencies. We find that beam jitter noise, electronic noise of the photodetectors, and the LO intensity noise can limit the homodyne detection in this frequency band, and we discuss potential solutions.
McKenzie
Kirk
K
Center for Gravitational Physics, Department of Physics, Faculty of Science, The Australian National University, ACT 0200, Australia. kirk.mckenzie@anu.edu.au
Gray
Malcolm B
MB
Lam
Ping Koy
PK
McClelland
David E
DE