Simulation of angular resolved RABBITT measurements in noble gas atoms
arXiv:1803.06063 · doi:10.1103/PhysRevA.97.063404
Abstract
We simulate angular resolved RABBITT (Reconstruction of Attosecond Beating By Interference of Two-photon Transitions) measurements on valence shells of noble gas atoms (Ne, Ar, Kr, and Xe). Our non-perturbative numerical simulation is based on solution of the time-dependent Schrödinger equation for a target atom driven by an ionizing XUV and dressing IR fields. From these simulations we extract the angular dependent magnitude and phase of the RABBITT oscillations and deduce the corresponding angular anisotropy β parameter and Wigner time delay for the single XUV photon absorption which initiates the RABBITT process. Said β and parameters are compared with calculations in the random phase approximation with exchange (RPAE) which includes inter-shell correlation. This comparison is used to test various effective potentials employed in the one-electron TDSE. In lighter atoms (Ne and Ar), several effective potentials are found to provide accurate simulation of RABBITT measurements for a wide range of photon energies up to 100 eV above the valence shell threshold. In heavier atoms (Kr and Xe), the onset of strong correlation with the d-shell restricts the validity of the single active electron approximation to several tens of eV above the valence shell threshold.
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- Propensity rules and interference effects in laser-assisted photoionization of helium and neon
- Reconstruction of attosecond pulses in the presence of interfering dressing fields using the 100 kHz ELI-ALPS HR-1 laser system
- Angle-resolved time delays for shake-up ionization of helium
- Polarization control of RABBITT in noble gas atoms
- Correlation enhancement of high-order harmonics generation in Xe
- Phase retrieval from angular streaking of XUV atomic ionization
- Effect of electron correlations on attosecond photoionization delays in the vicinity of the Cooper minima of argon
- Anisotropic Molecular Photoemission Dynamics Part. I Wigner meets the RABBIT
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