Bright high-repetition-rate source of narrowband extreme-ultraviolet harmonics beyond 22 eV

Novel table-top sources of extreme-ultraviolet light based on high-harmonic generation yield unique insight into the fundamental properties of molecules, nanomaterials or correlated solids, and enable advanced applications in imaging or metrology. Extending high-harmonic generation to high repetitio...

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Veröffentlicht in:Nature communications 2015-06, Vol.6 (1), p.7459-7459, Article 7459
Hauptverfasser: Wang, He, Xu, Yiming, Ulonska, Stefan, Robinson, Joseph S., Ranitovic, Predrag, Kaindl, Robert A.
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Sprache:eng
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Zusammenfassung:Novel table-top sources of extreme-ultraviolet light based on high-harmonic generation yield unique insight into the fundamental properties of molecules, nanomaterials or correlated solids, and enable advanced applications in imaging or metrology. Extending high-harmonic generation to high repetition rates portends great experimental benefits, yet efficient extreme-ultraviolet conversion of correspondingly weak driving pulses is challenging. Here, we demonstrate a highly-efficient source of femtosecond extreme-ultraviolet pulses at 50-kHz repetition rate, utilizing the ultraviolet second-harmonic focused tightly into Kr gas. In this cascaded scheme, a photon flux beyond ≈3 × 10 13  s −1 is generated at 22.3 eV, with 5 × 10 −5 conversion efficiency that surpasses similar harmonics directly driven by the fundamental by two orders-of-magnitude. The enhancement arises from both wavelength scaling of the atomic dipole and improved spatio-temporal phase matching, confirmed by simulations. Spectral isolation of a single 72-meV-wide harmonic renders this bright, 50-kHz extreme-ultraviolet source a powerful tool for ultrafast photoemission, nanoscale imaging and other applications. Table-top extreme-ultraviolet (XUV) light sources with high repetition rates are sought for fundamental studies, metrology and imaging. Here, Wang et al . demonstrate the efficient generation of bright XUV harmonics at 50-kHz repetition rate, with very high photon flux and spectral definition.
ISSN:2041-1723
2041-1723
DOI:10.1038/ncomms8459