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Published February 24, 2023 | Published + Supplemental Material
Journal Article Open

Mid-infrared cross-comb spectroscopy

Abstract

Dual-comb spectroscopy has been proven beneficial in molecular characterization but remains challenging in the mid-infrared region due to difficulties in sources and efficient photodetection. Here we introduce cross-comb spectroscopy, in which a mid-infrared comb is upconverted via sum-frequency generation with a near-infrared comb of a shifted repetition rate and then interfered with a spectral extension of the near-infrared comb. We measure CO₂ absorption around 4.25 µm with a 1-µm photodetector, exhibiting a 233-cm⁻¹ instantaneous bandwidth, 28000 comb lines, a single-shot signal-to-noise ratio of 167 and a figure of merit of 2.4 × 10⁶ Hz^(1/2). We show that cross-comb spectroscopy can have superior signal-to-noise ratio, sensitivity, dynamic range, and detection efficiency compared to other dual-comb-based methods and mitigate the limits of the excitation background and detector saturation. This approach offers an adaptable and powerful spectroscopic method outside the well-developed near-IR region and opens new avenues to high-performance frequency-comb-based sensing with wavelength flexibility.

Additional Information

© The Author(s) 2023. This article is licensed under a Creative Commons Attribution 4.0 International License, which permits use, sharing, adaptation, distribution and reproduction in any medium or format, as long as you give appropriate credit to the original author(s) and the source, provide a link to the Creative Commons license, and indicate if changes were made. The images or other third party material in this article are included in the article's Creative Commons license, unless indicated otherwise in a credit line to the material. If material is not included in the article's Creative Commons license and your intended use is not permitted by statutory regulation or exceeds the permitted use, you will need to obtain permission directly from the copyright holder. To view a copy of this license, visit http://creativecommons.org/licenses/by/4.0/. M.L., R.M.G., A.R., and A.M. gratefully acknowledge support from AFOSR award FA9550-20-1-0040 and NSF Grant No. 1846273. The author thank support from NASA/JPL. The authors thank Luis Ledezma and Selina Zhou at Caltech for helpful discussion. The authors thank Zhiquan Yuan, Lue Wu, and Prof. Kerry J. Vahala at Caltech for loaning equipment. C.R.M. is grateful for support from the Arnold O. Beckman Postdoctoral Fellowship. R.M.G. is thankful for support from the NSF Graduate Research Fellowship Program. Contributions. M.L. and A.M. conceived the project. M.L. and R.M.G. performed the CCS measurements and analyzed the results with assistance from L.C., C.R.M. and A.R. M.L. conducted theoretical analysis and numerical simulation with assistance from R.M.G. All authors participated in preparing the manuscript. The project was supervised by A.M. Data availability. The data that support the plots within these paper and other findings of this study are available from the corresponding author upon request. Code availability. The code that supports cross-comb signal processing and other findings of this study are available from the corresponding author upon request. Competing interests. A.M., M.L., and A.R. are inventors on a patent application (US patent application no. 17/533,926) that covers the concept and implementation of the cross-comb spectroscopy described here. The remaining authors declare no competing interests.

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Supplemental Material - 41467_2023_36811_MOESM1_ESM.pdf

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Additional details

Created:
August 22, 2023
Modified:
October 18, 2023