2014
DOI: 10.1088/0953-4075/47/13/135601
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Classical study of atomic bound state dynamics in circularly polarized ultrastrong fields

Abstract: We investigate hydrogen-like atoms in ultrastrong fields up to 1000 au (3 × 1022 W cm−2). We find the influence of the magnetic component (Blaser) of the external ultrastrong field introduces perturbations for the bound states of the atom. For intensities up to 1 × 1019 W cm−2 the changes in the trajectory energies and Poincaré plots are on the order of a few per cent. While small, the changes from Blaser with circular polarized (CP) light can result in a several-fold decrease in the ionization probability at … Show more

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Cited by 5 publications
(3 citation statements)
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“…Ionization and propagation components of this model compare favorably with recent ultrastrong field experiments [17]. Monte Carlo trajectory ensembles in the model capture essential quantum aspects of the electron [23,24] and such semiclassical approaches have been compared to full quantum solutions with the Dirac equation [29]. Adding elastic rescattering is a natural extension of the model and the approach has advantages in its connection to the well-known three-step model [30].…”
Section: Relativistic Three-step Recollision Modelmentioning
confidence: 98%
See 1 more Smart Citation
“…Ionization and propagation components of this model compare favorably with recent ultrastrong field experiments [17]. Monte Carlo trajectory ensembles in the model capture essential quantum aspects of the electron [23,24] and such semiclassical approaches have been compared to full quantum solutions with the Dirac equation [29]. Adding elastic rescattering is a natural extension of the model and the approach has advantages in its connection to the well-known three-step model [30].…”
Section: Relativistic Three-step Recollision Modelmentioning
confidence: 98%
“…New approaches are required to overcome the numerous challenges such as three-dimensional spatial dynamics that extend relativistically from an atomic unit of length to that of an optical wavelength in a femtosecond. Theory treatments have ranged from one-electron time-dependent Dirac and Klein-Gordon solutions [22] to fully classical [23][24][25][26]. Recent "bcwalker@udel.edu calculations have addressed the fundamental physics including the role of electron spin [27].…”
Section: Introductionmentioning
confidence: 99%
“…In this work, we use the semiclassical trajectory ensemble method [8,9]. Briefly, bound state ionization is calculated by tunneling [10] and the space-time relativistic photoelectron is modeled semiclassically with a 10 4 trajectory Monte-Carlo ensemble having a position and momentum spread matched to the tunneling wave function probability as it appears in the continuum.…”
Section: Rescattering Inner Shell Excitationmentioning
confidence: 99%