Weak-Light Phase-Locking Time Delay Interferometry with Optical Frequency Combs
In the future space-borne gravitational wave (GW) detector, the optical transponder scheme, i.e., the phase-locking scheme, will be utilized so as to maintain the signal-to-noise ratio (SNR). In this case, the whole constellation will share one common laser equivalently, which enables the considerab...
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MDPI AG
2022-09-01
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author | Mingyang Xu Hanzhong Wu Yurong Liang Dan Luo Panpan Wang Yujie Tan Chenggang Shao |
author_facet | Mingyang Xu Hanzhong Wu Yurong Liang Dan Luo Panpan Wang Yujie Tan Chenggang Shao |
author_sort | Mingyang Xu |
collection | DOAJ |
description | In the future space-borne gravitational wave (GW) detector, the optical transponder scheme, i.e., the phase-locking scheme, will be utilized so as to maintain the signal-to-noise ratio (SNR). In this case, the whole constellation will share one common laser equivalently, which enables the considerable simplification of time delay interferometry (TDI) combinations. Recently, and remarkably, the unique combination of TDI and optical frequency comb (OFC) has shown a bright prospect for the future space-borne missions. When the laser frequency noise and the clock noise are synchronized using OFC as the bridge, the data streams will be reasonably simplified. However, in the optical transponder scheme, the weak-light phase-locking (WLPL) loops could bring additional noises. In this work, we analyze the phase-locking scheme with OFC and transfer characteristics of the noises including the WLPL noise. We show that the WLPL noise can be efficiently reduced by using the specific TDI combination, and the cooperation of phase-locking and frequency combs can greatly simplify the post-processing. |
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spelling | doaj.art-9389312669c84a07a88f3f122efd54a72023-11-23T21:47:43ZengMDPI AGSensors1424-82202022-09-012219734910.3390/s22197349Weak-Light Phase-Locking Time Delay Interferometry with Optical Frequency CombsMingyang Xu0Hanzhong Wu1Yurong Liang2Dan Luo3Panpan Wang4Yujie Tan5Chenggang Shao6MOE Key Laboratory of Fundamental Physical Quantities Measurement, Hubei Key Laboratory of Gravitation and Quantum Physics, National Precise Gravity Measurement Facility, School of Physics, Huazhong University of Science and Technology, Wuhan 430074, ChinaMOE Key Laboratory of Fundamental Physical Quantities Measurement, Hubei Key Laboratory of Gravitation and Quantum Physics, National Precise Gravity Measurement Facility, School of Physics, Huazhong University of Science and Technology, Wuhan 430074, ChinaMOE Key Laboratory of Fundamental Physical Quantities Measurement, Hubei Key Laboratory of Gravitation and Quantum Physics, National Precise Gravity Measurement Facility, School of Physics, Huazhong University of Science and Technology, Wuhan 430074, ChinaMOE Key Laboratory of Fundamental Physical Quantities Measurement, Hubei Key Laboratory of Gravitation and Quantum Physics, National Precise Gravity Measurement Facility, School of Physics, Huazhong University of Science and Technology, Wuhan 430074, ChinaMOE Key Laboratory of Fundamental Physical Quantities Measurement, Hubei Key Laboratory of Gravitation and Quantum Physics, National Precise Gravity Measurement Facility, School of Physics, Huazhong University of Science and Technology, Wuhan 430074, ChinaMOE Key Laboratory of Fundamental Physical Quantities Measurement, Hubei Key Laboratory of Gravitation and Quantum Physics, National Precise Gravity Measurement Facility, School of Physics, Huazhong University of Science and Technology, Wuhan 430074, ChinaMOE Key Laboratory of Fundamental Physical Quantities Measurement, Hubei Key Laboratory of Gravitation and Quantum Physics, National Precise Gravity Measurement Facility, School of Physics, Huazhong University of Science and Technology, Wuhan 430074, ChinaIn the future space-borne gravitational wave (GW) detector, the optical transponder scheme, i.e., the phase-locking scheme, will be utilized so as to maintain the signal-to-noise ratio (SNR). In this case, the whole constellation will share one common laser equivalently, which enables the considerable simplification of time delay interferometry (TDI) combinations. Recently, and remarkably, the unique combination of TDI and optical frequency comb (OFC) has shown a bright prospect for the future space-borne missions. When the laser frequency noise and the clock noise are synchronized using OFC as the bridge, the data streams will be reasonably simplified. However, in the optical transponder scheme, the weak-light phase-locking (WLPL) loops could bring additional noises. In this work, we analyze the phase-locking scheme with OFC and transfer characteristics of the noises including the WLPL noise. We show that the WLPL noise can be efficiently reduced by using the specific TDI combination, and the cooperation of phase-locking and frequency combs can greatly simplify the post-processing.https://www.mdpi.com/1424-8220/22/19/7349weak-light phase-lockingoptical frequency combtime delay interferometry |
spellingShingle | Mingyang Xu Hanzhong Wu Yurong Liang Dan Luo Panpan Wang Yujie Tan Chenggang Shao Weak-Light Phase-Locking Time Delay Interferometry with Optical Frequency Combs Sensors weak-light phase-locking optical frequency comb time delay interferometry |
title | Weak-Light Phase-Locking Time Delay Interferometry with Optical Frequency Combs |
title_full | Weak-Light Phase-Locking Time Delay Interferometry with Optical Frequency Combs |
title_fullStr | Weak-Light Phase-Locking Time Delay Interferometry with Optical Frequency Combs |
title_full_unstemmed | Weak-Light Phase-Locking Time Delay Interferometry with Optical Frequency Combs |
title_short | Weak-Light Phase-Locking Time Delay Interferometry with Optical Frequency Combs |
title_sort | weak light phase locking time delay interferometry with optical frequency combs |
topic | weak-light phase-locking optical frequency comb time delay interferometry |
url | https://www.mdpi.com/1424-8220/22/19/7349 |
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