Optical heterodyne detection

ID: optical-heterodyne-detection

Optical heterodyne detection combines a signal field with a reference field at a different frequency, producing an electrical beat within a receiver's bandwidth. The reference is a local oscillator. A photodetector responds to the squared sum of the fields; averaging over optical carrier cycles removes the fast sum-frequency term but can retain the difference-frequency interference.
For constant powers incident on a linear detector of responsivity , a useful model is
The mode-overlap factor in optical heterodyne detection satisfies and includes spatial and polarization matching. The beat frequency is , while its phase carries a relative optical wave phase. Orthogonal polarizations can give and no beat despite nonzero power from both sources.
For an original chosen , , and , the beat's peak current is . The signal alone produces only of current, but the mixed DC level is about . A chosen frequency difference of is measurable electronically even though each carrier has an optical frequency. Increasing the reference also increases its noise and can overload the receiver; beat amplitude is not an unlimited sensitivity gain.
NIST's physical receiver-characterization experiment combined an external-cavity semiconductor laser and a Nd:YAG laser near . Variable attenuators, a beam splitter, a polarizer and single-mode fibre controlled the powers and matched the modes before the receiver. Sweeping the optical frequency difference generated a tunable test modulation.[ref]
The receiver must pass the beat frequency and preserve the intended overlap. A single real beat frequency supplies the magnitude of the frequency difference; identifying which optical frequency is higher needs additional information. At zero difference, the corresponding fixed-phase measurement is optical homodyne detection.

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