4.7 Article

Generation and characterization of isolated attosecond pulses at 100 kHz repetition rate

Journal

OPTICA
Volume 9, Issue 2, Pages 145-151

Publisher

OPTICAL SOC AMER
DOI: 10.1364/OPTICA.443521

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Funding

  1. U.S. Department of Defense [ONR N00014-17-1-2536]
  2. Horizon 2020 Framework Programme [674960]

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Researchers have generated and fully characterized extreme ultraviolet (XUV) attosecond pulses at a repetition rate of 100 kHz using near-single-cycle pulses. The high number of 10^6 XUV photons per pulse enables attosecond electron streaking experiments, revealing that the XUV pulses consist of a dominant single attosecond pulse.
The generation of coherent light pulses in the extreme ultraviolet (XUV) spectral region with attosecond pulse durations constitutes the foundation of the field of attosecond science. Twenty years after the first demonstration of isolated attosecond pulses, they continue to be a unique tool enabling the observation and control of electron dynamics in atoms, molecules, and solids. It has long been identified that an increase in the repetition rate of attosecond light sources is necessary for many applications in atomic and molecular physics, surface science, and imaging. Although high harmonic generation (HHG) at repetition rates exceeding 100 kHz, showing a continuum in the cutoff region of the XUV spectrum, was already demonstrated in 2013, the number of photons per pulse was insufficient to perform pulse characterization via attosecond streaking, let alone to perform a pump-probe experiment. Here we report on the generation and full characterization of XUV attosecond pulses via HHG driven by near-single-cycle pulses at a repetition rate of 100 kHz. The high number of 10(6) XUV photons per pulse on target enables attosecond electron streaking experiments through which the XUV pulses are determined to consist of a dominant single attosecond pulse. These results open the door for attosecond pump-probe spectroscopy studies at a repetition rate 1 or 2 orders of magnitude above current implementations. (C) 2022 Optical Society of America under the terms of the OSA Open Access Publishing Agreement

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