Abstract

We analyze how bound-state excitation, electron exchange and the residual binding potential influence above-threshold ionization (ATI) in helium prepared in an excited p state, oriented parallel and perpendicular to a linearly polarized mid-IR field. Using the ab initio B-spline algebraic diagrammatic construction, and several one-electron methods with effective potentials, including the Schrödinger solver Qprop, modified versions of the strong-field approximation (SFA) and the Coulomb quantum-orbit strong-field approximation, we find that these specific physical mechanisms leave significant imprints in ATI spectra and photoelectron momentum distributions. Examples are changes of up to two orders of magnitude in the high-energy photoelectron region, and ramp-like structures that can be traced back to Coulomb-distorted trajectories. The present work also shows that electron exchange renders rescattering less effective, causing suppressions in the ATI plateau. Due to the long-range potential, the electron continuum dynamics are no longer confined to the polarization axis, in contrast to the predictions of traditional approaches. Thus, one may in principle probe excited-state configurations perpendicular to the driving-field polarization without the need for orthogonally polarized fields.

Highlights

  • Above-threshold ionization (ATI) is a strong-field phenomenon in which an atom absorbs more photons than are energetically required for it to ionize

  • Our main goal was to understand the limitations of the rescattering model in its simplest form, i.e., that dictated by the strong-field approximation (SFA), and what subtleties must be taken into consideration

  • The SFA predicts a sharp decrease in the ATI signal for energies above the direct ATI cutoff 2Up for all cases, and a strong suppression in the high-energy ATI plateau, which extends up to the energy of 10Up, for the perpendicular initial state

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Summary

Introduction

Above-threshold ionization (ATI) is a strong-field phenomenon in which an atom absorbs more photons than are. We use approaches that incorporate the residual binding potential and/or the core dynamics: the B spline algebraic diagrammatic construction (ADC) (B-spline TD-ADC), the one-electron Schrödinger solver Qprop [41, 42], the SFA and the Coulomb quantum-orbit strong-field approximation (CQSFA). They will allow for an assessment of what the simple rescattering picture leaves out.

Theory
B-spline ADC
One-electron models
Results
ATI spectra
Photoelectron momentum distributions
Conclusions
Data availability statement
Full Text
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