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Register a new userIntegrated photonic interposers for processing octave-spanning microresonator frequency combs
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Microcombs - optical frequency combs generated in microresonators - have advanced tremendously in the last decade, and are advantageous for applications in frequency metrology, navigation, spectroscopy, telecommunications, and microwave photonics. Crucially, microcombs offer the prospect of fully integrated miniaturized optical systems with unprecedented reductions in cost, size, weight, and power. However, this goal has been consistently hindered by the use of bulk free-space and fiber-optic components to process microcombs, limiting form factors to the table-top. Here, we address this challenge by introducing an integrated photonics interposer architecture to process microcombs and replace discrete components. Taking microcomb-based optical frequency synthesis in the telecom C-band around 1550 nm as our target application, we develop an interposer architecture that collects, routes, and interfaces octave-wide optical signals between photonic chiplets and heterogeneously integrated devices that constitute the synthesizer. We have implemented the octave spanning spectral filtering of a microcomb, central to the interposer, in the popular silicon nitride photonic platform, and have confirmed the requisite performance of the individual elements of the interposer. Moreover, we show that the thick silicon nitride needed for bright dissipative Kerr soliton generation can be integrated with the comparatively thin silicon nitride interposer layer through octave-bandwidth adiabatic evanescent coupling, indicating a path towards future system-level consolidation. Our interposer architecture addresses the immediate need for on-chip microcomb processing to successfully miniaturize microcomb systems. As microcombs and integrated devices evolve, our approach can be readily adapted to other metrology-grade applications based on optical atomic clocks and high-precision navigation and spectroscopy.
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A generalized Lugiato-Lefever equation is numerically solved with a Newton-Raphson method to model Kerr frequency combs. We obtain excellent agreement with past experiments, even for an octave-spanning comb. Simulations are much faster than with any other technique despite including more modes than ever before. Our study reveals that Kerr combs are associated with temporal cavity solitons and dispersive waves, and opens up new avenues for the understanding of Kerr comb formation.
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