Abstract
The exceptionally low-energy isomeric transition in 229Th at around 148.4 nm (refs. 1,2,3,4,5,6) offers a unique opportunity for coherent nuclear control and the realization of a nuclear clock7,8. Recent advances, most notably the incorporation of large ensembles of 229Th nuclei in transparent crystals6,9,10,11 and the development of pulsed vacuum ultraviolet (VUV) lasers12,13,14, have enabled initial laser spectroscopy of this transition15,16,17. However, the lack of an intense, narrow-linewidth VUV laser has precluded coherent nuclear manipulation8,18. Here we introduce and report a continuous-wave (CW) laser at 148.4 nm, generated by means of four-wave mixing (FWM)19 in cadmium vapour. The source delivers more than 100 nW of power with a projected linewidth well below 100 Hz and supports broad wavelength tunability. This represents a five-orders-of-magnitude improvement in linewidth over all previous single-frequency lasers below 190 nm (refs. 12,13,14,20). We develop a spatially resolved homodyne technique that places a stringent upper bound on FWM-induced phase noise, thereby supporting the feasibility of sub-hertz VUV linewidths. Our work addresses the central challenge towards a 229Th-based nuclear clock and establishes a widely tunable, ultranarrow-linewidth laser platform for potential applications across quantum information science21,22,23,24, condensed-matter physics25 and high-resolution VUV spectroscopy26.
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Data availability
The datasets generated and analysed during this study are available in the Figshare repository at https://doi.org/10.6084/m9.figshare.30795137.
Code availability
The plotting scripts used to generate the figures from the datasets are available in the Figshare repository at https://doi.org/10.6084/m9.figshare.30795137.
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Acknowledgements
We thank X. Zhang and S. Zhou for discussions, Z. Xu and X. Wen for advice on frequency doubling, M. K. Tey for support on electronics and C. Zhang, H. Wu and J. Ye for comments on the manuscript. This work is supported by the National Natural Science Foundation of China (NSFC no. 12341401), Beijing Science and Technology Planning Project (grant no. Z25110100040000) and the Tsinghua University Dushi Program, as well as by NSFC nos. 12274253, 92265205, 12504306 and 92565202.
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Q.X., G.P., X.L., B.H., W.B., J.S., H.S., G.Y., Y. Li, J.L., L.Y., Y.M. and S.D. designed the experiment, constructed the set-up and carried out the measurements. T.L., H.T., B.L. and Y. Lin built the ULE-cavity-stabilized 1,550-nm laser. Q.X. and S.D. wrote the manuscript, with input from all authors.
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Extended data figures and tables
Extended Data Fig. 1 Measurement of VUV power.
With the 710-nm beam shuttered, the PMT records a background count rate of 1.42(1) × 105 s−1. At t ≈ 3.5 s, the 710-nm beam is unshuttered and the count rate rises to 4.76(34) × 106 s−1. Control measurements verify that the background count is dominated by residual 375-nm stray light, that the PMT is insensitive at 710-nm and that it operates in the linear regime. Using the overall detection efficiency ηabs = 0.21(4) × 10−4 (Extended Data Table 1), we infer a VUV power of 290(60) nW at 148.4 nm.
Extended Data Fig. 2 Linewidth measurements of the 750-nm and 710-nm Ti:sapphire lasers.
a, 750-nm Ti:sapphire laser. b, 710-nm Ti:sapphire laser. Both lasers are Pound–Drever–Hall-locked to a 10-cm-long ULE cavity. Each is heterodyned with an optical frequency comb referenced to a ULE-stabilized fibre laser at 1,550 nm (linewidth 0.25(1) Hz). The optical beats are down-mixed to an intermediate frequency within the span of a dynamic signal analyser and the resulting spectra (blue points) are fitted with Lorentzians (blue lines), yielding FWHM linewidths of Δf750 = 1.05(7) Hz and Δf710 = 1.01(9) Hz after subtracting the comb contribution67.
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Xiao, Q., Penyazkov, G., Li, X. et al. Continuous-wave narrow-linewidth vacuum ultraviolet laser source. Nature (2026). https://doi.org/10.1038/s41586-026-10107-4
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DOI: https://doi.org/10.1038/s41586-026-10107-4


