Generation of wideband frequency combs using single continuous-wave laser seed is described. The efficiency and noise suppression is achieved by specialized parametric mixer design. Performance limits of new parametric mixer technology are discussed.Keywords-parametric mixers, frequency synthesis, frequency comb.
I. CONTINUOUS-WAVE AND PULSE-SEEDED FREQUENCY COMB GENERATIONWideband frequency generation mandates nonlinear mixing process since conventional gain mechanisms span only limited spectral bandwidth. In practice, wideband frequency generation must be seeded by a laser source that possesses sufficient power and wavelength that matches specific nonlinear process. The aggregate comb noise is then defined by the contributions from the seed laser and the subsequent mixing process [1]. While distinct in origin, these contributions are not additive [2,3], since the device nonlinear noise response is uniquely defined by the seed source.Intuitively, minimum-noise generation calls for the seed laser with the lowest noise [1]. Even if we assume that physical mixer response can match any laser type, continuous-wave (CW) and pulsed laser emissions present different input conditions. Specifically, the noise properties of well-stabilized CW and mode-locked lasers (MLL) are inherently different, bringing distinct fluctuation types to the mixing process. In contrast to MLL lasers, CW devices operate near fundamental Schawlow-Townes (ST) limit [4,5,6]. Long before approaching the ST limit, the technical noise [4,5-7] will separate the performance of two types. Inter-modal dynamics of MLL lasers couples and exacerbates the noise originated with cavity and pumping fluctuations, ultimately making the suppression of MLL laser noise considerably more difficult than that of a single-frequency CW source [5][6][7]. Surprisingly, this simple observation is in direct conflict with the seed laser choice made with majority of frequency combs to date [8][9][10][11]. Indeed, starting from the early demonstration [8], reported work commonly relies [5,7] on pulsed (MLL) sources, in spite of its inherently higher noise levels.While suboptimal, the historic choice of MLL seeding can be easily understood in practical terms since efficient frequency comb generation dictates strict power and phasematching requirements [2,3,12].In ideal case, when wide-band phase matching condition is met, parametric efficiency depends exponentially on mixer figure of merit (FoM), defined by the product of optical power (P), effective interaction length (L) and mixer nonlinearity () [12]. With conventional comb generation, parametric process takes place in either crystalline or photonics crystal fiber (PCF) mixers possessing short physical length. To preserve FoM, these must be driven by high power seed -effectively eliminating the use of low-noise CW lasers as they cannot match peak powers developed by MLL emitters. Consequently, a high mixer FoM is historically achieved using MLL lasers with peak powers [8][9][10]. Unfortunately, this also greatly increases n...