High-order harmonic generation in Xe, Kr, and Ar driven by a 2.1-\mu m source: high-order harmonic spectroscopy under macroscopic effects

TL;DR

This study combines experimental and numerical methods to analyze high-order harmonic generation in Xe, Kr, and Ar driven by a 2.1-rac;m infrared source, revealing how atomic structure and macroscopic effects influence spectral shaping and efficiency.

Contribution

It introduces a comprehensive approach to understanding macroscopic effects on high-harmonic spectra and extracts photo-recombination cross-sections from experimental data.

Findings

Macroscopic effects shift the Cooper minimum in Kr from 80 eV to 60-70 eV.

High-harmonic conversion efficiencies are approximately 10^{-9} near the cutoff.

Spectral shaping is influenced by atomic structure and propagation effects.

Abstract

We experimentally and numerically study the atomic response and pulse propagation effects of high-order harmonics generated in Xe, Kr, and Ar driven by a 2.1-\mu m infrared femtosecond light source. The light source is an optical parametric chirped-pulse amplifier, and a modified strong-field approximation and 3-dimensional pulse propagation code are used for the numerical simulations. The extended cutoff in the long-wavelength driven high-harmonic generation has revealed the spectral shaping of high-order harmonics due to the atomic structure (or photo-recombination cross-section) and the macroscopic effects, which are the main factors of determining the conversion efficiency besides the driving wavelength. Using precise numerical simulations to determine the macroscopic electron wavepacket, we are able to extract the photo-recombination cross-sections from experimental high-order harmonic spectra in the presence of macroscopic effects. We have experimentally observed that the macroscopic effects shift the observed Cooper minimum of Kr from 80 eV to 60-70 eV and wash out the Cooper minimum of Ar. Measured high-harmonic conversion efficiencies per harmonic near the cutoff are ~10^{-9} for all three gases.