EXCESS PHASE NOISE IN SELF-HETERODYNE DETECTION

Self-heterodyne detection is a popular method to determine the linewidth of a laser. However, the interpretation of self-heterodyne spectra is difficult if, apart from spontaneous emission, additional noise sources are present. Measurements on an external-cavity semiconductor laser show how, for a relatively long delay, the high-frequency (Lorentzian) wings of the self-heterodyne spectrum are a sensitive measure for the quantum-limited (Schawlow-Townes) laser linewidth. The quantum-limited laser linewidth is shown to be inversely proportional to the output power. Values below 5 kHz are routinely measured. The full width at half maximum (FWHM) laser linewidth is larger than this due to excess low-frequency fluctuations, which are shown to result from the presence of side modes.