研究目的
Investigating the properties of long cavity frequency sweeping lasers and demonstrating various scenarios of coherence deterioration in such lasers.
研究成果
The study identified three dynamical regimes in a ring cavity swept source laser, including stable and unstable Nozaki-Bekki holes, and provided insight into the coherence properties of such devices. The results explain the mechanism of bi-stability observed in these lasers and their potential applications in imaging and sensing.
研究不足
The study focuses on specific configurations of long cavity lasers and their dynamical regimes, which may not cover all possible variations or applications. The experimental setup's complexity and the need for precise control of parameters like cavity length and frequency sweeping speed could limit reproducibility.
1:Experimental Design and Method Selection:
The study involved investigating static, quasi static, and synchronisation regimes of long cavity lasers, analyzing possible instabilities. Different laser configurations were considered to study the influence of cavity length, frequency sweeping speed, and detuning. A model based on a system of delayed differential equations was used for numerical simulation.
2:Sample Selection and Data Sources:
The laser consisted of a single mode fiber based ring cavity including a semiconductor optical amplifier and a narrow bandwidth tunable Fabry-Perot filter. The filter transmission was modulated by a signal generator.
3:List of Experimental Equipment and Materials:
Semiconductor optical amplifier (Covega), tunable Fabry-Perot filter (MicronOptics), signal generator (Agilent), optical isolators, 50:50 coupler, tunable laser source (TLS), real time oscilloscope, optical spectrum analyzer.
4:Experimental Procedures and Operational Workflow:
The laser's operation was studied depending on the SOA bias current and the power of the injected electric field. The filter scanning speed was 26 Hz with a scanning range of 5 nm around 1300 nm central wavelength.
5:Data Analysis Methods:
The analysis included studying the formation of dark pulses and their connection to Nozaki-Bekki holes, using numerical simulation that showed excellent agreement with experimental data.
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