4.4 Article

High harmonic generation in mixed XUV and NIR fields at a free-electron laser

期刊

JOURNAL OF OPTICS
卷 24, 期 2, 页码 -

出版社

IOP Publishing Ltd
DOI: 10.1088/2040-8986/ac4318

关键词

high harmonic generation; free-electron laser; XUV-assisted HHG

类别

资金

  1. Chemical Sciences, Geosciences, and Biosciences Division, Office of Basic Energy Sciences, Office of Science, U.S. Department of Energy (DOE) [DE-FG02-86ER13491]
  2. National Science Foundation (NSF) [PHYS-1753324]
  3. Initiative and Networking Fund of the Helmholtz Association [VH-NG-1104]
  4. BMBF [05K10KT2, 05K13KT2, 05K16KT3, 05K10KTB, FSP-302]

向作者/读者索取更多资源

We present the results of an experiment investigating the generation of high-order harmonics through XUV-assisted high-order harmonic generation. Our findings demonstrate that the overlap of XUV and NIR pulses enhances the harmonic yield, while the XUV preceding the NIR pulse decreases the HHG yield.
We present the results of an experiment investigating the generation of high-order harmonics by a femtosecond near-infrared (NIR) laser pulse in the presence of an extreme ultraviolet (XUV) field provided by a free-electron laser (FEL), a process referred to as XUV-assisted high-order harmonic generation (HHG). Our experimental findings show that the XUV field can lead to a small enhancement in the harmonic yield when the XUV and NIR pulses overlap in time, while a strong decrease of the HHG yield and a red shift of the HHG spectrum is observed when the XUV precedes the NIR pulse. The latter observations are in qualitative agreement with model calculations that consider the effect of a decreased number of neutral emitters but are at odds with the predicted effect of the correspondingly increased ionization fraction on the phase matching. Our study demonstrates the technical feasibility of XUV-assisted HHG experiments at FELs, which may provide new avenues to investigate correlation-driven electron dynamics as well as novel ways to study and control propagation effects and phase matching in HHG.

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