Tunable coherence laser interferometry: demonstrating 40dB of straylight suppression and compatibility with resonant optical cavities
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arXiv
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2025
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| author | Voigt, Daniel Eggers, Leonie Isleif, Katharina-Sophie Koehlenbeck, Sina M. Ast, Melanie Gerberding, Oliver |
| author_facet | Voigt, Daniel Eggers, Leonie Isleif, Katharina-Sophie Koehlenbeck, Sina M. Ast, Melanie Gerberding, Oliver |
| contents | A major limitation of laser interferometers using continuous wave lasers are parasitic light fields, such as ghost beams, scattered or stray light, which can cause non-linear noise. This is especially relevant for laser interferometric ground-based gravitational wave detectors. Increasing their sensitivity, particularly at frequencies below 10 Hz, is threatened by the influence of parasitic photons. These can up-convert low-frequency disturbances into phase and amplitude noise inside the relevant measurement band. By artificially tuning the coherence of the lasers, using pseudo-random-noise (PRN) phase modulations, this influence of parasitic fields can be suppressed. As it relies on these fields traveling different paths, it does not sacrifice the coherence for the intentional interference. We demonstrate the feasibility of this technique experimentally, achieving noise suppression levels of 40 dB in a Michelson interferometer with an artificial coherence length below 30 cm. We probe how the suppression depends on the delay mismatch and length of the PRN sequence. We also prove that optical resonators can be operated in the presence of PRN modulation by measuring the behavior of a linear cavity with and without such a modulation. By matching the resonators round-trip length and the PRN sequence repetition length, the classic response is recovered. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2501_11528 |
| institution | arXiv |
| publishDate | 2025 |
| record_format | arxiv |
| spellingShingle | Tunable coherence laser interferometry: demonstrating 40dB of straylight suppression and compatibility with resonant optical cavities Voigt, Daniel Eggers, Leonie Isleif, Katharina-Sophie Koehlenbeck, Sina M. Ast, Melanie Gerberding, Oliver Optics Instrumentation and Methods for Astrophysics General Relativity and Quantum Cosmology Instrumentation and Detectors A major limitation of laser interferometers using continuous wave lasers are parasitic light fields, such as ghost beams, scattered or stray light, which can cause non-linear noise. This is especially relevant for laser interferometric ground-based gravitational wave detectors. Increasing their sensitivity, particularly at frequencies below 10 Hz, is threatened by the influence of parasitic photons. These can up-convert low-frequency disturbances into phase and amplitude noise inside the relevant measurement band. By artificially tuning the coherence of the lasers, using pseudo-random-noise (PRN) phase modulations, this influence of parasitic fields can be suppressed. As it relies on these fields traveling different paths, it does not sacrifice the coherence for the intentional interference. We demonstrate the feasibility of this technique experimentally, achieving noise suppression levels of 40 dB in a Michelson interferometer with an artificial coherence length below 30 cm. We probe how the suppression depends on the delay mismatch and length of the PRN sequence. We also prove that optical resonators can be operated in the presence of PRN modulation by measuring the behavior of a linear cavity with and without such a modulation. By matching the resonators round-trip length and the PRN sequence repetition length, the classic response is recovered. |
| title | Tunable coherence laser interferometry: demonstrating 40dB of straylight suppression and compatibility with resonant optical cavities |
| topic | Optics Instrumentation and Methods for Astrophysics General Relativity and Quantum Cosmology Instrumentation and Detectors |
| url | https://arxiv.org/abs/2501.11528 |