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NASA NTRS · 20020091866

Slow Light in Coupled Resonator Optical Waveguides

Abstract

Recently, we discovered that a splitting of the whispering gallery modes (WGMs) occurs in coupled resonator optical waveguides (CROWs), and that these split modes are of a higher Q than the single-resonator modes, leading to enormous circulating intensity magnification factors that dramatically reduce thresholds for nonlinear optical (NLO) processes. As a result of the enhancements in Q, pulses propagating at a split resonance can propagate much slower (faster) for over (under)-coupled structures, due to the modified dispersion near the split resonance. Moreover, when loss is considered, the mode-splitting may be thought of as analogous to the Autler-Townes splitting that occurs in atomic three-level lambda systems, i.e., it gives rise to induced transparency as a result of destructive interference. In under- or over-coupled CROWs, this coupled resonator induced transparency (CRIT) allows slow light to be achieved at the single-ring resonance with no absorption, while maintaining intensities such that NLO effects are maximized. The intensity magnification of the circulating fields and phase transfer characteristics are examined in detail.

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BibTeXRIS

Chang, Hongrok, Gates, Amanda L., Fuller, Kirk A., Gregory, Don A., Witherow, William K., Paley, Mark S., Frazier, Donald O., Smith, David D., Curreri, Peter A.. 2002-01-01. Slow Light in Coupled Resonator Optical Waveguides. https://ntrs.nasa.gov/citations/20020091866

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