Generation of an astronomical optical frequency comb in three fibre-based nonlinear stages

Keyphrases

• Pulse Compression 100%
• Fiber-based 100%
• Fiber Length 100%
• Input Power 100%
• Fiber Section 100%
• Highly Nonlinear Fiber 100%
• Ultrashort Pulses 100%
• Frequency Comb 100%
• Optical Frequency Comb 100%
• Adiabatic Pulses 100%
• Erbium-doped Fiber 50%
• Higher-order Dispersion 50%
• Self-phase Modulation 50%
• Anomalous Dispersion 50%
• Peak Power 50%
• Low Dispersion 50%
• Spectral Broadening 50%
• Optical Feedback 50%
• Fs Pulses 50%
• Kerr Nonlinearity 50%
• Input Field 50%
• Low Noise 50%
• Nonlinear Coefficient 50%
• Small Fibers 50%
• Intensity Noise 50%
• Astronomical Spectrographs 50%
• Sinusoidal Wave 50%
• Sinusoidal Inputs 50%
• Compression Techniques 50%
• Rare-earth Doped Fibers 50%
• Raman Nonlinearity 50%
• Nonlinear Length 50%
• Input Nonlinearity 50%
• Generalized Nonlinear Schrödinger Equation 50%
• Self-steepening 50%

Engineering

• Nonlinearity 100%
• Pulse Compression 100%
• Input Power 100%
• Fiber Section 100%
• Fibre Length 100%
• Optical Frequency 100%
• Solitary Wave 50%
• Phase Modulation 50%
• Erbium-Doped Fiber 50%
• Peak Power 50%
• Fits and Tolerances 50%
• Spectral Broadening 50%
• Intensity Noise 50%
• Final Stage 50%
• Sinusoidal Input 50%
• Compression Technique 50%
• Rare Earth-Doped Fibers 50%
• Start Pulse 50%

Physics

• Frequency Comb 100%
• Ultrashort Pulse 50%
• Solitary Wave 25%
• Erbium-Doped Fiber 25%
• Noise Intensity 25%
• Spectrographs 25%
• Spectral Broadening 25%
• Low Noise 25%
• Rare-Earth-Doped Fiber 25%