2011
DOI: 10.1364/ol.36.002026
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Widely tunable extreme UV frequency comb generation

Abstract: Extreme UV (XUV) frequency comb generation in the wavelength range of 51 to 85 nm is reported based on high-order harmonic generation of two consecutive IR frequency comb pulses that were amplified in an optical parametric chirped pulse amplifier. The versatility of the system is demonstrated by recording direct XUV frequency comb excitation signals in He, Ne, and Ar with visibilities of up to 61%.

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Cited by 8 publications
(4 citation statements)
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“…This is based on parametric amplification of two frequency-comb pulses combined with harmonic upconversion. A wide and continuous tunability from 85 to 51 nm was demonstrated for the method with spectroscopy in argon, neon, and helium [54]. In the current paper a full and detailed description is given of the precision spectroscopy performed in helium [53].…”
Section: Introductionmentioning
confidence: 99%
“…This is based on parametric amplification of two frequency-comb pulses combined with harmonic upconversion. A wide and continuous tunability from 85 to 51 nm was demonstrated for the method with spectroscopy in argon, neon, and helium [54]. In the current paper a full and detailed description is given of the precision spectroscopy performed in helium [53].…”
Section: Introductionmentioning
confidence: 99%
“…Based on parametric amplification, Ramsey-comb spectroscopy combines high frequency precision with wide wavelength coverage at mJ-level pulse energy. Because of the high peak energy, the frequency range of this method can straightforwardly and efficiently be extended via nonlinear crystals to the ultraviolet, or with high-harmonic generation in a gas jet to the extreme ultraviolet [23] (taking T > 100 ns to avoid phase shifts from ionisation in the gas jet). Therefore there are many interesting targets for the Ramsey-comb method, such as the 1S-2S two-photon transition in He + to provide new information on the proton-size puzzle [24,25], or the twophoton X-EF transition in molecular hydrogen to put tighter constraints on speculative 5 th forces beyond the Standard Model [26].…”
Section: Figure 2: Schematic Of the Experimental Setupmentioning
confidence: 99%
“…However, for our purposes we need spectra with no spurious or missing levels, which demands FC coverage from the visible to the mid-UV and, perhaps, even into the vacuum-UV or extreme-UV for ionized species. Such FCs already exist in the visible and near-IR, and rapid progress has been made in extending FCs to the mid-IR [27], to the VUV [28], and even into the XUV [29][30][31]. As this technology continues to improve, measuring the necessary spectra seems quite achievable.…”
Section: Sensitivity and Experimental Realizationmentioning
confidence: 99%